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arXiv:2606.25677v1 [math.RT] 24 Jun 2026

The representation theory of the wreath product of a finite group with the monoid of all partial functions on a finite set as an EI-category algebra

Itamar Stein

🖂  Steinita@gmail.com
Mathematics Unit, Shamoon College of Engineering, 77245 Ashdod, Israel
Abstract

Let GG be a finite group. We provide a description of the ordinary quiver of the complex monoid algebra of the wreath product GPTnG\wr\operatorname{PT}_{n}, where PTn\operatorname{PT}_{n} denotes the monoid of all partial functions on an nn-element set. This description depends on the multiplicities of simple GG-modules appearing in the decomposition of tensor products of simple GG-modules. We also prove that the global dimension of this algebra is n1n-1. Both results are obtained by analyzing the associated Ehresmann EI-category related to the monoid. Finally, we describe the quiver of the algebra of the wreath product of GG with the submonoid of all order-preserving partial functions.

1 Introduction

A central aim in the study of monoid representations is to connect them with the general representation theory of associative algebras. Investigating the invariants of the monoid algebra of a finite monoid MM is of particular interest. Throughout this paper, all modules are over the field of complex numbers \mathbb{C}, so we consider the complex monoid algebra M\mathbb{C}M.

Among invariants of an algebra, the (ordinary) quiver plays a foundational role. A standard way to present a finite-dimensional algebra is via a quiver, which is a directed graph, bound by a set of relations on its paths. In this context, the quiver can be viewed as the generators part in a generators-and-relations presentation of the algebra. Even without explicit knowledge of the relations, the quiver alone encodes a significant amount of data about the algebra.

Determining the quiver of a monoid algebra is a fundamental problem in the representation theory of finite monoids [31, Chapter 17]. To date, descriptions of the quiver have been obtained for many monoids and families of monoids [4, 13, 14, 15, 16, 17, 19, 22, 24, 26, 30, 32]. In particular, in [26], the author described the quiver of the monoid algebra PTn\mathbb{C}\operatorname{PT}_{n}, where PTn\operatorname{PT}_{n} is the monoid of all partial functions on an nn-element set. In this paper, we aim to generalize this result to the complex monoid algebra of the partial wreath product GPTnG\wr\operatorname{PT}_{n} of any finite group GG with PTn\operatorname{PT}_{n}.

Partial wreath products of groups with (partial) transformation semigroups play a crucial role in the Krohn-Rhodes decomposition theory of finite automata and Krohn-Rhodes complexity theory [18]. This monoid was also studied recently in [2, Section 9].

To compute the quiver of the monoid algebra of GPTnG\wr\operatorname{PT}_{n}, we follow the general framework established in [26] for PTn\operatorname{PT}_{n}. However, the introduction of the finite group GG into the structure introduces complications in the underlying representation theory.

After reviewing the necessary preliminaries in Section 2, we introduce several branching rules in Section 3 that will be used in our proof.

The computation of the quiver is carried out in Section 4. Since (GPTn)\mathbb{C}(G\wr\operatorname{PT}_{n}) is a finite EE-Ehresmann and right restriction semigroup, its algebra is isomorphic to that of its associated Ehresmann category.

This category is the wreath product of GG with the category of all onto functions between subsets of an nn-element set (see also [23]). This is an EI-category, meaning that every endomorphism monoid is a group. To determine the quiver of an EI-category algebra, a well-known method (see [16, Section 6.3.1] and [11]) reduces the problem to the representation theory of its endomorphism groups. We follow this approach here.

The endomorphism groups in this case are of the form GSkG\wr S_{k}, where SkS_{k} is the symmetric group. This computation utilizes known branching rules for GSkG\wr S_{k} to establish our main result. The description of the quiver itself is given in Theorem 4.10 and relies on the decomposition of tensor products of simple GG-modules.

We remark that the similar problem of finding the quiver of the wreath product of GG with the category of injective functions between subsets of an nn-element set was solved in [27, Section 6]. However, in that case, the structure of the group GG plays a minimal role in the description.

In Section 5, we prove that the global dimension of (GPTn)\mathbb{C}(G\wr\operatorname{PT}_{n}) is n1n-1 by applying the EI-category framework to lift known results on the global dimension of PTn\operatorname{PT}_{n} from [29].

Finally, in Section 6, we compute the quiver of the complex monoid algebra (GPOn)\mathbb{C}(G\wr\operatorname{PO}_{n}), where POn\operatorname{PO}_{n} is the monoid of all order-preserving partial functions on an nn-element set. The method is identical to that applied in the case of PTn\operatorname{PT}_{n}, but the branching rules are simpler in this setting.

Acknowledgement: The author is grateful to Professor Stuart Margolis for several discussions on the monoid GPTnG\wr\operatorname{PT}_{n}.

2 Preliminaries

2.1 Partial wreath product

Let 𝒜\mathcal{A} be a small category. We denote by 𝒜0\mathcal{A}^{0} and 𝒜1\mathcal{A}^{1} the sets of objects and morphisms of 𝒜\mathcal{A}, respectively. For a,b𝒜0a,b\in\mathcal{A}^{0}, we write 𝒜(a,b)\mathcal{A}(a,b) for the hom-set of morphisms with domain aa and range bb. Recall that a monoid can be viewed as a category with a single object. Following [25], we denote by 𝐏𝐟𝐧\operatorname{\mathbf{Pfn}} the category whose objects are finite sets and whose morphisms are partial functions, and by 𝐒𝐞𝐭\operatorname{\bf{Set}} the subcategory consisting of total functions as morphisms.

Let GG be a finite group with identity element 1G1_{G}, and let PT(𝒳,G)\operatorname{PT}(\mathcal{X},G) denote the set of all partial functions from 𝒳\mathcal{X} to GG. For every fPT(𝒳,G)f\in\operatorname{PT}(\mathcal{X},G), we denote by dom(f)\operatorname{dom}(f) its domain. The set PT(𝒳,G)\operatorname{PT}(\mathcal{X},G) is a monoid under pointwise multiplication, where for any f1,f2PT(𝒳,G)f_{1},f_{2}\in\operatorname{PT}(\mathcal{X},G), the product f1f2f_{1}\cdot f_{2} has domain dom(f1)dom(f2)\operatorname{dom}(f_{1})\cap\operatorname{dom}(f_{2}) and is defined by:

(f1f2)(x)=f1(x)f2(x)for all xdom(f1)dom(f2).(f_{1}\cdot f_{2})(x)=f_{1}(x)\cdot f_{2}(x)\quad\text{for all }x\in\operatorname{dom}(f_{1})\cap\operatorname{dom}(f_{2}).

The identity element of this monoid is the constant function mapping every x𝒳x\in\mathcal{X} to 1G1_{G}.

Let H:𝒜𝐏𝐟𝐧H:\mathcal{A}\to\operatorname{\mathbf{Pfn}} be a functor. Define a new category GH𝒜G\wr_{H}\mathcal{A} in the following way. The set of objects is the same as the set of objects of 𝒜\mathcal{A}, that is, (GH𝒜)0=𝒜0(G\wr_{H}\mathcal{A})^{0}=\mathcal{A}^{0}. Given two objects a,b𝒜0a,b\in\mathcal{A}^{0}, the hom-set (GH𝒜)(a,b)(G\wr_{H}\mathcal{A})(a,b) is

{(f,m)fPT(H(a),G),m𝒜(a,b),wheredom(f)=dom(H(m))}.\{(f,m)\mid f\in\operatorname{PT}(H(a),G),\,m\in\mathcal{A}(a,b),\,\text{where}\,\operatorname{dom}(f)=\operatorname{dom}(H(m))\}.

Now, given two morphisms (f,m)(GH𝒜)(a,b)(f,m)\in(G\wr_{H}\mathcal{A})(a,b) and (f,m)(GH𝒜)(b,c)(f^{\prime},m^{\prime})\in(G\wr_{H}\mathcal{A})(b,c) the composition is

(f,m)(f,m)=((fH(m))f,mm).(f^{\prime},m^{\prime})\cdot(f,m)=((f^{\prime}\circ H(m))\cdot f,m^{\prime}m).

It is routine to verify that this composition is well defined and that GH𝒜G\wr_{H}\mathcal{A} is indeed a category. If ida\operatorname{id}_{a} is the identity morphism of a𝒜0a\in\mathcal{A}^{0} and 𝟏H(a):H(a)G{\bf 1}_{H(a)}:H(a)\to G is the function defined by 𝟏H(a)(x)=1G{\bf 1}_{H(a)}(x)=1_{G} for every xH(a)x\in H(a), then the identity morphism of the object a(GH𝒜)0a\in(G\wr_{H}\mathcal{A})^{0} is (𝟏H(a),ida)({\bf 1}_{H(a)},\operatorname{id}_{a}). The category GH𝒜G\wr_{H}\mathcal{A} is called the partial wreath product of GG and 𝒜\mathcal{A} with respect to HH. We will apply this construction in two special cases. In the first case, HH is a functor H:𝒜𝐒𝐞𝐭H:\mathcal{A}\to\operatorname{\bf{Set}}. In this case, the construction reduces to the standard wreath product of a group with a category (see, for example, [23, 34]). In the second case, 𝒜\mathcal{A} is a monoid MM with identity element 1M1_{M}. Here the construction is well-known, even when GG and MM are semigroups. It appears in [5] in the language of transformation semigroups, and in [10] under the name of 0-wreath products. See also [2, Section 9.1] and references therein. In this case, a functor H:M𝐏𝐟𝐧H:M\to\operatorname{\mathbf{Pfn}} is an incomplete MM-action. That is, it consists of a set 𝒳\mathcal{X} and a monoid homomorphism φ:MPT𝒳\varphi:M\to\operatorname{PT}_{\mathcal{X}}. For mMm\in M and x𝒳x\in\mathcal{X}, we will write mxm\bullet x instead of φ(m)(x)\varphi(m)(x). For every mMm\in M, we write

dom(m)=dom(φ(m))𝒳.\operatorname{dom}(m)=\operatorname{dom}(\varphi(m))\subseteq\mathcal{X}.

The monoid MM acts on the right of PT(𝒳,G)\operatorname{PT}(\mathcal{X},G) by fm=fφ(m)f\ast m=f\circ\varphi(m). Explicitly, for x𝒳x\in\mathcal{X}, the partial function fmf\ast m is given by

(fm)(x)={f(mx)mxandf(mx)are both definedundefinedotherwise.(f\ast m)(x)=\begin{cases}f(m\bullet x)&m\bullet x\kern 5.0pt\text{and}\kern 5.0ptf(m\bullet x)\kern 5.0pt\text{are both defined}\\ \text{undefined}&\text{otherwise}.\end{cases}

In this case, the partial wreath product G𝒳MG\wr_{\mathcal{X}}M is a monoid whose underlying set is

G𝒳M={(f,m)mM,fPT(𝒳,G),dom(f)=dom(m)}.G\wr_{\mathcal{X}}M=\{(f,m)\mid m\in M,\quad f\in\operatorname{PT}(\mathcal{X},G),\quad\operatorname{dom}(f)=\operatorname{dom}(m)\}.

The operation is given by

(f1,m1)(f2,m2)=((f1m2)f2,m1m2),(f_{1},m_{1})\cdot(f_{2},m_{2})=((f_{1}\ast m_{2})\cdot f_{2},m_{1}m_{2}),

where (f1m2)(x)=f1(m2x)(f_{1}\ast m_{2})(x)=f_{1}(m_{2}\bullet x) and the identity element is (𝟏𝒳,1M)({\bf 1}_{\mathcal{X}},1_{M}).

Remark 2.1.

Many authors adopt the convention of composing functions from left to right. Under this convention, the monoid MM acts on the right of 𝒳\mathcal{X} and on the left of PT(𝒳,G)\operatorname{PT}(\mathcal{X},G). Consequently, the multiplication in G𝒳MG\wr_{\mathcal{X}}M is often written in a different form in the literature.

The case where MM is a group is of great importance. If f:𝒳Gf:\mathcal{X}\to G is a (total) function, we denote by f1:𝒳Gf^{-1}:\mathcal{X}\to G the function defined by f1(x)=(f(x))1f^{-1}(x)=\left(f(x)\right)^{-1} for every x𝒳.x\in\mathcal{X}. If MM is a group, then G𝒳MG\wr_{\mathcal{X}}M is a group, and the inverse of (f,m)G𝒳M(f,m)\in G\wr_{\mathcal{X}}M is given by

(f,m)1=((fm1)1,m1).(f,m)^{-1}=(\left(f\ast m^{-1}\right)^{-1},m^{-1}).

There is a natural incomplete action of the monoid PT𝒳\operatorname{PT}_{\mathcal{X}} on the set 𝒳\mathcal{X}. Formally, the action is given by the identity function φ:PT𝒳PT𝒳\varphi:\operatorname{PT}_{\mathcal{X}}\to\operatorname{PT}_{\mathcal{X}}. In this case, we simply write GPT𝒳G\wr\operatorname{PT}_{\mathcal{X}} for G𝒳PT𝒳G\wr_{\mathcal{X}}\operatorname{PT}_{\mathcal{X}}. If 𝒳=[n]={1,,n}\mathcal{X}=[n]=\{1,\ldots,n\}, we denote the corresponding wreath product by GPTnG\wr\operatorname{PT}_{n}. In this special case, the wreath product has a natural description using matrices over G{0}G\cup\{0\}. For αPTn\alpha\in\operatorname{PT}_{n} and fPT([n],G)f\in\operatorname{PT}([n],G) with dom(f)=dom(α)\operatorname{dom}(f)=\operatorname{dom}(\alpha), we denote by [f,α][f,\alpha] an n×nn\times n matrix over G{0}G\cup\{0\} defined by

[f,α]i,j={f(j)α(j)=i,0otherwise.[f,\alpha]_{i,j}=\begin{cases}f(j)&\alpha(j)=i,\\ 0&\text{otherwise}.\end{cases}

Let \mathcal{M} denote the set of all such matrices. Note that each [f,α][f,\alpha]\in\mathcal{M} has at most one non-zero entry in each column, so matrix multiplication is well-defined. It is straightforward to verify that the function ψ:GPTn\psi:G\wr\operatorname{PT}_{n}\to\mathcal{M} defined by ψ((f,α))=[f,α]\psi((f,\alpha))=[f,\alpha] is a monoid isomorphism.

2.2 Ehresmann semigroups

Let SS be a semigroup and let ESE\subseteq S be a subset of idempotents. We define two equivalence relations ~E\widetilde{\mathcal{L}}_{E} and ~E\widetilde{\mathcal{R}}_{E} on SS.

a~Eb(eEbe=bae=a)a\widetilde{\mathcal{L}}_{E}b\iff(\forall e\in E\quad be=b\Leftrightarrow ae=a)
a~Eb(eEeb=bea=a).a\widetilde{\mathcal{R}}_{E}b\iff(\forall e\in E\quad eb=b\Leftrightarrow ea=a).

A subset ESE\subseteq S of idempotents is called a subsemilattice if it is a commutative subsemigroup. It is well known that any commutative semigroup of idempotents has the structure of a semilattice (i.e. a poset where every two elements have a meet) if one defines aba\leq b whenever ab=ba=aab=ba=a. A semigroup SS with a subsemilattice ESE\subseteq S is called right EE-Ehresmann if every ~E\widetilde{\mathcal{L}}_{E}-class contains a unique idempotent from EE and ~E\widetilde{\mathcal{L}}_{E} is a right congruence. We denote the unique idempotent in the ~E\widetilde{\mathcal{L}}_{E}-class of aa by aa^{\ast}. Note that aa^{\ast} is the unique minimal element eEe\in E such that ae=aae=a. It is well known that ~E\widetilde{\mathcal{L}}_{E} is a right congruence if and only if the identity (ab)=(ab)(ab)^{\ast}=(a^{\ast}b)^{\ast} holds for every a,bSa,b\in S.

Dually, we can consider semigroups for which every ~E\widetilde{\mathcal{R}}_{E} class contains a unique idempotent. We denote the unique idempotent in the ~E\widetilde{\mathcal{R}}_{E} class of aa by a+a^{+}. Such a semigroup is called left EE-Ehresmann if ~E\widetilde{\mathcal{R}}_{E} is a left congruence, or equivalently if (ab)+=(ab+)+(ab)^{+}=(ab^{+})^{+} for every a,bSa,b\in S. A semigroup SS with a subsemilattice ESE\subseteq S is called EE-Ehresmann if it is both left and right EE-Ehresmann. The semilattice EE is also called the set of projections of SS.

A right (left) Ehresmann semigroup SS is called right (respectively, left) restriction if the “right ample” (respectively, “left ample”) identity ea=a(ea)ea=a(ea)^{\ast} (respectively, ae=(ae)+aae=(ae)^{+}a) holds for every aSa\in S and eEe\in E.

For every Ehresmann semigroup SS, we can associate a category 𝐂(S){\bf C}(S) in the following way. The object set of 𝐂(S){\bf C}(S) is the set EE of projections and the morphisms of 𝐂(S){\bf C}(S) are in one-to-one correspondence with elements of SS. For every aSa\in S, we associate a morphism C(a)𝐂(S)1C(a)\in{\bf C}(S)^{1} with domain aa^{\ast} and range a+a^{+} and if the range of C(a)C(a) is the domain of C(b)C(b), the composition C(b)C(a)C(b)\cdot C(a) is defined to be C(ba)C(ba). For more facts and proofs on Ehresmann semigroups and Ehresmann categories, the reader is referred to [6, 7].

2.3 Algebras and modules

Let AA be an algebra. We will only discuss unital, finite-dimensional \mathbb{C}-algebras in this paper. Likewise, when we say that VV is a module over AA (or an AA-module or an AA-representation), we mean that VV is a finite-dimensional left module over AA. For aAa\in A and vVv\in V, we write ava\bullet v for the action of aa on the module element vv. An AA-module VV is simple (or irreducible) if 0 is its only proper submodule. The ordinary quiver QQ of a finite dimensional algebra AA is a directed graph defined in the following way: The vertices of QQ are in a one-to-one correspondence with the simple modules of AA (up to isomorphism). If ViV_{i} and VjV_{j} are simple modules of AA (identified with two vertices of the quiver), then the number of arrows from ViV_{i} to VjV_{j} is

dimExt1(Vi,Vj)\dim\operatorname{Ext}^{1}(V_{i},V_{j})

where Ext1(V,)\operatorname{Ext}^{1}(V,-) is the first right derived functor of Hom(V,)\operatorname{Hom}(V,-), see [20, Chapters 6-7]. More about modules of algebras and quivers can be found in [1].

In this paper, we discuss complex algebras of finite categories. Let 𝒜\mathcal{A} be a finite category. The category algebra 𝒜\mathbb{C}\mathcal{A} is a vector space over \mathbb{C} with the morphisms of 𝒜\mathcal{A} as its basis. It consists of all formal linear combinations:

{i=1nkimiki,mi𝒜1}.\left\{\sum_{i=1}^{n}k_{i}m_{i}\mid k_{i}\in\mathbb{C},\,m_{i}\in\mathcal{A}^{1}\right\}.

The multiplication in 𝒜\mathbb{C}\mathcal{A} is the linear extension of the following:

mm={mmif mm is defined in 𝒜,0otherwise.m^{\prime}\cdot m=\begin{cases}m^{\prime}m&\text{if }m^{\prime}m\text{ is defined in }\mathcal{A},\\ 0&\text{otherwise}.\end{cases}

The algebra 𝒜\mathbb{C}\mathcal{A} has a unit element given by the sum of the identity morphisms of all objects in 𝒜\mathcal{A}:

1𝒜=c𝒜0idc.1_{\mathbb{C}\mathcal{A}}=\sum_{c\in\mathcal{A}^{0}}\operatorname{id}_{c}.

Since a monoid is a category with a single object, this construction naturally specializes to the definition of a monoid algebra. In this case, the algebra M\mathbb{C}M consists of all formal linear combinations of elements of the monoid MM, with multiplication defined as the linear extension of the monoid operation.

2.4 Complex group representations

Let GG be a finite group. If VV is a \mathbb{C}G-module, we will usually simply say that VV is a GG-module (or a GG-representation). Equivalently, a GG-module is a pair (V,ρ)(V,\rho) of a \mathbb{C}-vector space VV and a group homomorphism ρ:GGL(V)\rho:G\to\operatorname{GL}(V). We denote the set of simple modules of GG (up to isomorphism) by IRepG\operatorname{IRep}G. It is well known that every GG-module is a finite direct sum of simple modules and that the number of different simple GG-modules (up to isomorphism) is the number of conjugacy classes of GG. We denote the trivial module of any group GG by trG\operatorname{tr}_{G}. Recall that if VV is a GG-module, then V=Hom(V,)V^{\ast}=\operatorname{Hom}(V,\mathbb{C}) is also a GG-module with operation (gφ)(v)=φ(g1v)(g\bullet\varphi)(v)=\varphi(g^{-1}\bullet v). Let UU and VV be GG-modules. The inner tensor product UVU\otimes V is again a GG-module with action defined by g(uv)=(gu)(gv)g\bullet(u\otimes v)=(g\bullet u)\otimes(g\bullet v) and extending linearly. Now, assume that U1U_{1} and U2U_{2} are modules of G1G_{1} and G2G_{2}, respectively. The outer tensor product U1U2U_{1}\otimes U_{2} of U1U_{1} and U2U_{2} is the (G1×G2G_{1}\times G_{2})-module where (g1,g2)(u1u2)=(g1u1)(g2u2)(g_{1},g_{2})\bullet(u_{1}\otimes u_{2})=(g_{1}\bullet u_{1})\otimes(g_{2}\bullet u_{2}). Although the two types of tensor product can be distinguished by context, we prefer to use a different notation for the outer tensor product, denoting it by \boxtimes. Similarly, the simple tensors of UVU\boxtimes V will be denoted by uvu\boxtimes v. It is well known that IRep(G1×G2)={UVUIRepG1,VIRepG2}\operatorname{IRep}(G_{1}\times G_{2})=\{U\boxtimes V\mid U\in\operatorname{IRep}G_{1},V\in\operatorname{IRep}G_{2}\}. The character χU\chi_{U} of the GG-module (U,ρ)(U,\rho) is the function χU:G\chi_{U}:G\to\mathbb{C} defined by χU(g)=trace(ρ(g))\chi_{U}(g)=\operatorname{trace}(\rho(g)). Recall that the multiplicity of UIRepGU\in\operatorname{IRep}G as a simple constituent in some GG-module VV is given by the inner product of characters

χU,χVG=1|G|gGχU(g)χV(g)¯.\langle\chi_{U},\chi_{V}\rangle_{G}=\frac{1}{|G|}\sum_{g\in G}\chi_{U}(g)\overline{\chi_{V}(g)}.

We may omit the subscript GG when the group is clear from the context. Recall also that χV(g)=χV(g)¯\chi_{V^{\ast}}(g)=\overline{\chi_{V}(g)}, χUV((g1,g2))=χU(g1)χV(g2)\chi_{U\boxtimes V}((g_{1},g_{2}))=\chi_{U}(g_{1})\chi_{V}(g_{2}) and χUV(g)=χU(g)χV(g)\chi_{U\otimes V}(g)=\chi_{U}(g)\chi_{V}(g). In order to simplify notation, we will usually omit χ\chi and write UU also for the character of UU. Hence the above inner product will be written as

U,V=1|G|gGU(g)V(g)¯.\langle U,V\rangle=\frac{1}{|G|}\sum_{g\in G}U(g)\overline{V(g)}.

Let (U,ρ)(U,\rho) be a GG-module and let HGH\leq G be a subgroup. The restriction of (U,ρ)(U,\rho) to HH is the HH-module (ResHGU,ResHGρ)(\operatorname{Res}_{H}^{G}U,\operatorname{Res}_{H}^{G}\rho) defined by

ResHGρ(h)(u)=ρ(h)(u)\operatorname{Res}_{H}^{G}\rho(h)(u)=\rho(h)(u)

that is, restricting the homomorphism to the subgroup HH. Note that dimResHGU=dimU\dim\operatorname{Res}_{H}^{G}U\allowbreak=\dim U and if UU is a simple GG-module, then ResHGU\operatorname{Res}_{H}^{G}U does not have to be a simple HH-module. Let (U,ρ)(U,\rho) be an HH-module, the induction to GG, denoted (IndHGU,IndHGρ)(\operatorname{Ind}_{H}^{G}U,\operatorname{Ind}_{H}^{G}\rho) is the tensor product

IndHGU=GHU\operatorname{Ind}_{H}^{G}U=\mathbb{C}G\underset{\mathbb{C}H}{\otimes}U

where the GG action is given by

g(su)=(gs)ug\bullet(s\otimes u)=(gs)\otimes u

where sGs\in\mathbb{C}G and uUu\in U. However, we will also use the following more concrete description. Choose S={s1,,sl}S=\{s_{1},\ldots,s_{l}\} to be representatives of the left cosets of HH in GG (where l=[G:H]l=[G:H]). Note that any element gGg\in G can be written in a unique way as g=sihg=s_{i}h where siSs_{i}\in S and hHh\in H. Every element of IndHGU\operatorname{Ind}_{H}^{G}U is a formal sum of the form

α1(s1,u1)++αl(sl,ul)\alpha_{1}(s_{1},u_{1})+\ldots+\alpha_{l}(s_{l},u_{l})

where uiUu_{i}\in U and αi\alpha_{i}\in\mathbb{C}. In other words, as a vector space IndHGU\operatorname{Ind}_{H}^{G}U is i=1lU{\displaystyle\bigoplus_{i=1}^{l}U}, that is, ll copies of UU. The action is defined on elements of the form (si,u)(s_{i},u) by

g(si,u)=(sj,hu)g\bullet(s_{i},u)=(s_{j},h\bullet u)

where sjs_{j} and hh are unique such that gsi=sjhgs_{i}=s_{j}h. The required action is given by extending linearly. Note that dimIndHGU=[G:H]dimU\dim\operatorname{Ind}_{H}^{G}U=[G:H]\dim U. It is important to mention that the modules IndHGU\operatorname{Ind}_{H}^{G}U and ResHGV\operatorname{Res}_{H}^{G}V depend not only on the groups GG and HH but also on the specific embedding of HH into GG. Hence, we will have to give the specific embeddings when discussing these modules. Both induction and restriction are transitive and additive, that is, if KHGK\leq H\leq G then

IndHGIndKHUIndKGU,IndHG(UV)IndHGUIndHGV\operatorname{Ind}_{H}^{G}\operatorname{Ind}_{K}^{H}U\cong\operatorname{Ind}_{K}^{G}U,\quad\operatorname{Ind}_{H}^{G}(U\oplus V)\cong\operatorname{Ind}_{H}^{G}U\oplus\operatorname{Ind}_{H}^{G}V

and

ResKHResHGUResKGU,ResHG(UV)ResHGUResHGV.\operatorname{Res}_{K}^{H}\operatorname{Res}_{H}^{G}U\cong\operatorname{Res}_{K}^{G}U,\quad\operatorname{Res}_{H}^{G}(U\oplus V)\cong\operatorname{Res}_{H}^{G}U\oplus\operatorname{Res}_{H}^{G}V.

For the restriction this is a trivial statement, and for the induction the proof is [3, Propositions 1.1.10 and 1.1.11]. An important fact that relates induction to restriction is the following one (for a proof, see [3, Corollary 1.1.20 ]).

Theorem 2.2 (Frobenius reciprocity).

Let HGH\leq G and let UU and VV be GG and HH-modules respectively. Then the multiplicity of VV in ResHGU\operatorname{Res}_{H}^{G}U equals the multiplicity of UU in IndHGV\operatorname{Ind}_{H}^{G}V.

Using characters, Frobenius reciprocity can be written as the following equality

IndHGV,UG=V,ResHGUH.\langle\operatorname{Ind}_{H}^{G}V,U\rangle_{G}=\langle V,\operatorname{Res}_{H}^{G}U\rangle_{H}.

Let UU be a GG-module. Consider the swap transformation S:UUUUS:U\otimes U\to U\otimes U defined on simple tensors by S(u1u2)=u2u1S(u_{1}\otimes u_{2})=u_{2}\otimes u_{1}. We define the symmetric square Sym2U\operatorname{Sym}^{2}U and the alternating square Alt2U\operatorname{Alt}^{2}U as the following submodules of the tensor product UUU\otimes U:

Sym2U\displaystyle\operatorname{Sym}^{2}U ={vUUS(v)=v},\displaystyle=\{v\in U\otimes U\mid S(v)=v\},
Alt2U\displaystyle\operatorname{Alt}^{2}U ={vUUS(v)=v}.\displaystyle=\{v\in U\otimes U\mid S(v)=-v\}.

As GG-modules, UUSym2UAlt2UU\otimes U\cong\operatorname{Sym}^{2}U\oplus\operatorname{Alt}^{2}U. The characters of these modules are given by:

(Sym2U)(g)=12(U(g)2+U(g2))and(Alt2U)(g)=12(U(g)2U(g2)).(\operatorname{Sym}^{2}U)(g)=\frac{1}{2}\left(U(g)^{2}+U(g^{2})\right)\quad\text{and}\quad(\operatorname{Alt}^{2}U)(g)=\frac{1}{2}\left(U(g)^{2}-U(g^{2})\right).

2.5 Representation theory of SnS_{n} and GSnG\wr S_{n}

We will recall some elementary facts regarding the representation theory of the symmetric group. More details can be found in [9, 21]. Recall that an integer composition of nn is a tuple λ=[λ1,,λk]\lambda=[\lambda_{1},\ldots,\lambda_{k}] of non-negative integers such that λ1++λk=n\lambda_{1}+\cdots+\lambda_{k}=n while an integer partition of nn (denoted λn\lambda\vdash n) is an integer composition such that λ1λ2λk>0\lambda_{1}\geq\lambda_{2}\geq\cdots\geq\lambda_{k}>0. From now on, when dealing with a partition λ\lambda we will write its elements in superscript λ=[λ1,,λk]\lambda=[\lambda^{1},\ldots,\lambda^{k}] because we want to reserve the subscript for multipartitions. Note that 0 has one partition, namely the empty partition, denoted by \emptyset. We can associate to any partition λ\lambda a graphical description called a Young diagram, which is a table with λi\lambda^{i} boxes in its ii-th row. For instance, the Young diagram associated to the partition [3,3,2,1][3,3,2,1] of 99 is:

    

We will identify the two notions and regard integer partition and Young diagram as synonyms. It is well-known that simple modules of SnS_{n} are indexed by integer partitions of nn. We denote the simple module associated to the partition λ\lambda (also called its Specht module) by SλS^{\lambda}. An explicit description of SλS^{\lambda} can be found in [21, Section 2.3]. It will be often convenient to draw the diagram λ\lambda instead of writing SλS^{\lambda}. For instance we may write

 
 
\hbox{\vtop{\halign{&\opttoksa@YT={\font@YT}\getcolor@YT{\save@YT{\opttoksb@YT}}\nil@YT\getcolor@YT{\startbox@@YT\the\opttoksa@YT\the\opttoksb@YT}#\endbox@YT\cr\lower 0.39993pt\vbox{\kern 0.19997pt\hbox{\kern 0.39993pt\vbox to15.39995pt{\vss\hbox to15.00002pt{\hss$$\hss}\vss}\kern-15.39995pt\vrule height=15.39995pt,width=0.39993pt\kern 15.00002pt\vrule height=15.39995pt,width=0.39993pt}\kern-0.19997pt\kern-15.39995pt\hrule width=15.79988pt,height=0.39993pt\kern 15.00002pt\hrule width=15.79988pt,height=0.39993pt}&\lower 0.39993pt\vbox{\kern 0.19997pt\hbox{\kern 0.39993pt\vbox to15.39995pt{\vss\hbox to15.00002pt{\hss$$\hss}\vss}\kern-15.39995pt\vrule height=15.39995pt,width=0.39993pt\kern 15.00002pt\vrule height=15.39995pt,width=0.39993pt}\kern-0.19997pt\kern-15.39995pt\hrule width=15.79988pt,height=0.39993pt\kern 15.00002pt\hrule width=15.79988pt,height=0.39993pt}&\lower 0.39993pt\vbox{\kern 0.19997pt\hbox{\kern 0.39993pt\vbox to15.39995pt{\vss\hbox to15.00002pt{\hss$$\hss}\vss}\kern-15.39995pt\vrule height=15.39995pt,width=0.39993pt\kern 15.00002pt\vrule height=15.39995pt,width=0.39993pt}\kern-0.19997pt\kern-15.39995pt\hrule width=15.79988pt,height=0.39993pt\kern 15.00002pt\hrule width=15.79988pt,height=0.39993pt}\cr}}\kern 31.99976pt}\oplus\hbox{\vtop{\halign{&\opttoksa@YT={\font@YT}\getcolor@YT{\save@YT{\opttoksb@YT}}\nil@YT\getcolor@YT{\startbox@@YT\the\opttoksa@YT\the\opttoksb@YT}#\endbox@YT\cr\lower 0.39993pt\vbox{\kern 0.19997pt\hbox{\kern 0.39993pt\vbox to15.39995pt{\vss\hbox to15.00002pt{\hss$$\hss}\vss}\kern-15.39995pt\vrule height=15.39995pt,width=0.39993pt\kern 15.00002pt\vrule height=15.39995pt,width=0.39993pt}\kern-0.19997pt\kern-15.39995pt\hrule width=15.79988pt,height=0.39993pt\kern 15.00002pt\hrule width=15.79988pt,height=0.39993pt}&\lower 0.39993pt\vbox{\kern 0.19997pt\hbox{\kern 0.39993pt\vbox to15.39995pt{\vss\hbox to15.00002pt{\hss$$\hss}\vss}\kern-15.39995pt\vrule height=15.39995pt,width=0.39993pt\kern 15.00002pt\vrule height=15.39995pt,width=0.39993pt}\kern-0.19997pt\kern-15.39995pt\hrule width=15.79988pt,height=0.39993pt\kern 15.00002pt\hrule width=15.79988pt,height=0.39993pt}\cr\lower 0.39993pt\vbox{\kern 0.19997pt\hbox{\kern 0.39993pt\vbox to15.39995pt{\vss\hbox to15.00002pt{\hss$$\hss}\vss}\kern-15.39995pt\vrule height=15.39995pt,width=0.39993pt\kern 15.00002pt\vrule height=15.39995pt,width=0.39993pt}\kern-0.19997pt\kern-15.39995pt\hrule width=15.79988pt,height=0.39993pt\kern 15.00002pt\hrule width=15.79988pt,height=0.39993pt}\cr}}\kern 31.99976pt}

instead of: SλSδS^{\lambda}\oplus S^{\delta} for partitions λ=[3]\lambda=[3] and δ=[2,1]\delta=[2,1].

Let 𝐧=[n1,,nl]{\bf n}=[n_{1},\ldots,n_{l}] be an integer composition of nn. A tuple Λ=(λ1,,λl)\Lambda=(\lambda_{1},\ldots,\lambda_{l}) such that λini\lambda_{i}\vdash n_{i} for every ii is called a multipartition of nn with ll components. We also call it a multipartition of the composition 𝐧{\bf n} and denote this by Λ𝐧\Lambda\Vdash{\bf n}. We define a multi-Young diagram to be a tuple of Young diagrams. As we identify partitions with Young diagrams, we also identify multipartitions with multi-Young diagrams.

Let GG be a finite group with ll conjugacy classes. It is well-known ([3, Theorem 2.6.1]) that multi-Young diagrams with nn boxes and ll components index the simple modules of the wreath product GSnG\wr S_{n}. If Λ𝐧\Lambda\Vdash{\bf n} is a multi-Young diagram, then we denote by SΛS^{\Lambda} its associated GSnG\wr S_{n}-module.

3 Branching rules

Let GG be a finite group with ll conjugacy classes. Fix IRepG={U1,Ul}\operatorname{IRep}G=\{U_{1},\ldots U_{l}\} to be its set of simple modules. In this section we will describe several known branching rules for the group GSnG\wr S_{n} that we will need later on.

3.1 Restriction of GS2G\wr S_{2}

Let S2={id,s}S_{2}=\{\operatorname{id},s\} be the symmetric group of order 22 where ss will always be the swap permutation. We denote by tr2\operatorname{tr}_{2} the trivial module of S2S_{2} and by sgn2\operatorname{sgn}_{2} the sign module of S2S_{2}. The group G×S2G\times S_{2} can be embedded in GS2G\wr S_{2} by φ(g,σ)=((g,g),σ)\varphi(g,\sigma)=((g,g),\sigma). In this section, we study the restriction ResG×S2GS2\operatorname{Res}_{G\times S_{2}}^{G\wr S_{2}}. Every simple module of G×S2G\times S_{2} is of the form Urtr2U_{r}\boxtimes\operatorname{tr}_{2} or Ursgn2U_{r}\boxtimes\operatorname{sgn}_{2} where UrIRepGU_{r}\in\operatorname{IRep}G (r{1,l}r\in\{1,\ldots l\}). The description of simple modules of GS2G\wr S_{2} is more complicated, but well-known (see [3, Chapter 2] for the description of simple modules of GSnG\wr S_{n} in general). If Ui,UjIRepGU_{i},U_{j}\in\operatorname{IRep}G are two non-isomorphic simple modules of GG then UiUjU_{i}\boxtimes U_{j} is a G×GG\times G simple module. Clearly, G×GG\times G embeds in GS2G\wr S_{2} by φ(g1,g2)=((g1,g2),id)\varphi(g_{1},g_{2})=((g_{1},g_{2}),\operatorname{id}). One type of simple GS2G\wr S_{2} module is obtained by induction Wi,j=IndG×GGS2(UiUj)W_{i,j}=\operatorname{Ind}_{G\times G}^{G\wr S_{2}}(U_{i}\boxtimes U_{j}). This gives us (l2)\binom{l}{2} simple modules. Note that dimWi,j=2dimUidimUj\dim W_{i,j}=2\dim U_{i}\dim U_{j}. The module Wi,jW_{i,j} corresponds to the multipartition Λ\Lambda with λi=λj=[1]\lambda_{i}=\lambda_{j}=[1] and λk=\lambda_{k}=\emptyset for ki,jk\neq i,j. Given UiIRepGU_{i}\in\operatorname{IRep}G, another type of simple module is the tensor product UiUiU_{i}\boxtimes U_{i} where the action is

((g1,g2),σ)(u1u2)=(gσ(1)uσ(1))(gσ(2)uσ(2)).((g_{1},g_{2}),\sigma)\bullet(u_{1}\boxtimes u_{2})=(g_{\sigma(1)}\bullet u_{\sigma(1)})\boxtimes(g_{\sigma(2)}\bullet u_{\sigma(2)}).

We denote this simple module by Wi+W_{i}^{+}. This gives another ll simple modules. The module Wi+W_{i}^{+} corresponds to the multipartition Λ\Lambda with λi=[2]\lambda_{i}=[2] and λk=\lambda_{k}=\emptyset for kik\neq i. Finally, we denote by Inf(sgn2)\operatorname{Inf}(\operatorname{sgn}_{2}) the inflation of sgn2\operatorname{sgn}_{2} to a GS2G\wr S_{2} module. This means that ((g1,g2),σ)((g_{1},g_{2}),\sigma) acts like σ\sigma. The last ll simple modules of GS2G\wr S_{2} are obtained by the tensor product Wi+Inf(sgn2)W_{i}^{+}\otimes\operatorname{Inf}(\operatorname{sgn}_{2}) and we denote them by WiW_{i}^{-}. The module WiW_{i}^{-} corresponds to the multipartition Λ\Lambda with λi=[1,1]\lambda_{i}=[1,1] and λk=\lambda_{k}=\emptyset for kik\neq i. In total, we have l2+3l2\frac{l^{2}+3l}{2} simple modules for GS2G\wr S_{2}.

Remark 3.1.

In the literature, the module Wi+W_{i}^{+} is defined by the action

((g1,g2),σ)(u1u2)=(g1uσ(1))(g2uσ(2))((g_{1},g_{2}),\sigma)\bullet(u_{1}\boxtimes u_{2})=(g_{1}\bullet u_{\sigma(1)})\boxtimes(g_{2}\bullet u_{\sigma(2)})

(in fact, with σ1\sigma^{-1}, but σ1=σ\sigma^{-1}=\sigma in our case.) This variation arises because, in the context of groups, the composition in the wreath product GMG\wr M is defined by

(f2,m2)(f1,m1)=(f2(m2f1),m2m1)(f_{2},m_{2})\cdot(f_{1},m_{1})=(f_{2}\cdot(m_{2}\star f_{1}),m_{2}m_{1})

where (mf1)(x)=f1(m1x)(m\star f_{1})(x)=f_{1}(m^{-1}x). As shown in [27, Lemma 6.3], the two definitions are isomorphic under the map

T(f,m)=(mf,m)T(f,m)=(m\star f,m)

but it changes the concrete description of the module Wi+W_{i}^{+}. In any case, we are interested in the action of elements of the form ((g,g),σ)((g,g),\sigma). For such elements, the two actions coincide, ensuring there is no ambiguity in our context.

The characters of these modules are well-known and essential for computing the desired restriction. Recall that we use the same notation for a module and its character. If we take ((1G,1G),id)((1_{G},1_{G}),\operatorname{id}) and ((1G,1G),s)((1_{G},1_{G}),s) as representatives of the cosets of G×GG\times G in GS2G\wr S_{2}, it is easy to see that ((g,g),s)((g,g),s) swaps the cosets and ((g,g),id)((g,g),\operatorname{id}) fixes them. The character of the induction is summation of the base character over the fixed cosets (see [21, Section 1.12]). Therefore, the character Wi,jW_{i,j} for an element ((g,g),σ)GS2((g,g),\sigma)\in G\wr S_{2} is given by:

Wi,j((g,g),σ)={2Ui(g)Uj(g)if σ=id,0if σ=s.W_{i,j}((g,g),\sigma)=\begin{cases}2U_{i}(g)U_{j}(g)&\text{if }\sigma=\operatorname{id},\\ 0&\text{if }\sigma=s.\end{cases}

For the modules Wi+W_{i}^{+} and WiW_{i}^{-}, the character values on the elements ((g,g),σ)((g,g),\sigma) are given as follows (see [9, 4.3.10 (vi), p. 150]):

Wi+((g,g),σ)={Ui(g)2if σ=id,Ui(g2)if σ=s,W_{i}^{+}((g,g),\sigma)=\begin{cases}U_{i}(g)^{2}&\text{if }\sigma=\operatorname{id},\\ U_{i}(g^{2})&\text{if }\sigma=s,\end{cases}

and

Wi((g,g),σ)={Ui(g)2if σ=id,Ui(g2)if σ=s.W_{i}^{-}((g,g),\sigma)=\begin{cases}U_{i}(g)^{2}&\text{if }\sigma=\operatorname{id},\\ -U_{i}(g^{2})&\text{if }\sigma=s.\end{cases}
Lemma 3.2.

The multiplicities of Uktr2U_{k}\boxtimes\operatorname{tr}_{2} and Uksgn2U_{k}\boxtimes\operatorname{sgn}_{2} in ResG×S2GS2Wi,j\operatorname{Res}_{G\times S_{2}}^{G\wr S_{2}}W_{i,j} are both equal to the multiplicity of UkU_{k} in UiUjU_{i}\otimes U_{j}.

Proof.

Let VV be either the trivial module tr2\operatorname{tr}_{2} or the sign module sgn2\operatorname{sgn}_{2} of S2S_{2}. The multiplicity of UkVU_{k}\boxtimes V in the restriction is:

ResG×S2GS2Wi,j,UkVG×S2=12|G|gGσS2Wi,j((g,g),σ)Uk(g)V(σ)¯.\langle\operatorname{Res}_{G\times S_{2}}^{G\wr S_{2}}W_{i,j},U_{k}\boxtimes V\rangle_{G\times S_{2}}=\frac{1}{2|G|}\sum_{g\in G}\sum_{\sigma\in S_{2}}W_{i,j}((g,g),\sigma)\overline{U_{k}(g)V(\sigma)}.

As Wi,j((g,g),s)=0W_{i,j}((g,g),s)=0, the sum over σS2\sigma\in S_{2} only has a contribution from σ=id\sigma=\operatorname{id}. Since V(id)=1V(\operatorname{id})=1 for both the trivial and sign modules, the expression becomes:

12|G|gGWi,j((g,g),id)Uk(g)¯=12|G|gG2Ui(g)Uj(g)Uk(g)¯=UiUj,UkG,\frac{1}{2|G|}\sum_{g\in G}W_{i,j}((g,g),\operatorname{id})\overline{U_{k}(g)}=\frac{1}{2|G|}\sum_{g\in G}2U_{i}(g)U_{j}(g)\overline{U_{k}(g)}=\langle U_{i}\otimes U_{j},U_{k}\rangle_{G},

which completes the proof. ∎

Lemma 3.3.

The multiplicities of Uktr2U_{k}\boxtimes\operatorname{tr}_{2} and Uksgn2U_{k}\boxtimes\operatorname{sgn}_{2} in the restrictions ResG×S2GS2Wi+\operatorname{Res}_{G\times S_{2}}^{G\wr S_{2}}W_{i}^{+} and ResG×S2GS2Wi\operatorname{Res}_{G\times S_{2}}^{G\wr S_{2}}W_{i}^{-} are given by the multiplicities of UkU_{k} in Sym2Ui\operatorname{Sym}^{2}U_{i} and Alt2Ui\operatorname{Alt}^{2}U_{i} as follows:

  1. 1.

    ResG×S2GS2Wi+,Uktr2G×S2=Sym2Ui,UkG\langle\operatorname{Res}_{G\times S_{2}}^{G\wr S_{2}}W_{i}^{+},U_{k}\boxtimes\operatorname{tr}_{2}\rangle_{G\times S_{2}}=\langle\operatorname{Sym}^{2}U_{i},U_{k}\rangle_{G}

  2. 2.

    ResG×S2GS2Wi+,Uksgn2G×S2=Alt2Ui,UkG\langle\operatorname{Res}_{G\times S_{2}}^{G\wr S_{2}}W_{i}^{+},U_{k}\boxtimes\operatorname{sgn}_{2}\rangle_{G\times S_{2}}=\langle\operatorname{Alt}^{2}U_{i},U_{k}\rangle_{G}

  3. 3.

    ResG×S2GS2Wi,Uktr2G×S2=Alt2Ui,UkG\langle\operatorname{Res}_{G\times S_{2}}^{G\wr S_{2}}W_{i}^{-},U_{k}\boxtimes\operatorname{tr}_{2}\rangle_{G\times S_{2}}=\langle\operatorname{Alt}^{2}U_{i},U_{k}\rangle_{G}

  4. 4.

    ResG×S2GS2Wi,Uksgn2G×S2=Sym2Ui,UkG\langle\operatorname{Res}_{G\times S_{2}}^{G\wr S_{2}}W_{i}^{-},U_{k}\boxtimes\operatorname{sgn}_{2}\rangle_{G\times S_{2}}=\langle\operatorname{Sym}^{2}U_{i},U_{k}\rangle_{G}

Proof.

We prove the first case; the others follow by similar character computations. By the definition of the inner product of characters on G×S2G\times S_{2}, we have:

ResG×S2GS2Wi+,Uktr2G×S2=12|G|gG(Wi+((g,g),id)Uk(g)¯+Wi+((g,g),s)Uk(g)¯).\langle\operatorname{Res}_{G\times S_{2}}^{G\wr S_{2}}W_{i}^{+},U_{k}\boxtimes\operatorname{tr}_{2}\rangle_{G\times S_{2}}=\frac{1}{2|G|}\sum_{g\in G}\left(W_{i}^{+}((g,g),\operatorname{id})\overline{U_{k}(g)}+W_{i}^{+}((g,g),s)\overline{U_{k}(g)}\right).

Substituting the character values Wi+((g,g),id)=Ui(g)2W_{i}^{+}((g,g),\operatorname{id})=U_{i}(g)^{2} and Wi+((g,g),s)=Ui(g2)W_{i}^{+}((g,g),s)=U_{i}(g^{2}), we obtain:

1|G|gG(Ui(g)2+Ui(g2)2)Uk(g)¯.\frac{1}{|G|}\sum_{g\in G}\left(\frac{U_{i}(g)^{2}+U_{i}(g^{2})}{2}\right)\overline{U_{k}(g)}.

The term in parentheses is precisely the character of Sym2Ui\operatorname{Sym}^{2}U_{i}. Thus, the expression reduces to Sym2Ui,UkG\langle\operatorname{Sym}^{2}U_{i},U_{k}\rangle_{G}, which is the multiplicity of UkU_{k} in Sym2Ui\operatorname{Sym}^{2}U_{i}. ∎

3.2 Littlewood-Richardson rules for small additions

Let GG be a group with ll conjugacy classes. The group (GSk)×(GSr)(G\wr S_{k})\times(G\wr S_{r}) is naturally embedded in GSk+rG\wr S_{k+r}. If f1:{1,,k}Gf_{1}:\{1,\ldots,k\}\to G and f2:{1,,r}Gf_{2}:\{1,\ldots,r\}\to G we define f:{1,,k+r}Gf:\{1,\ldots,k+r\}\to G by

f(i)={f1(i)ikf2(ik)i>k.f(i)=\begin{cases}f_{1}(i)&i\leq k\\ f_{2}(i-k)&i>k\end{cases}.

Then, the natural embedding φ:GSk×GSrGSk+r\varphi:G\wr S_{k}\times G\wr S_{r}\to G\wr S_{k+r} is defined by φ((f1,σ1),(f2,σ2))=(f,σ1σ2)\varphi((f_{1},\sigma_{1}),(f_{2},\sigma_{2}))=(f,\sigma_{1}\sigma_{2}) where σ1\sigma_{1} (σ2\sigma_{2}) can be regarded as an element of Sk+rS_{k+r} that fixes {k+1,,k+r}\{k+1,\ldots,k+r\} ({1,,k}\{1,\ldots,k\}). The branching rules for describing the induction from GSk×GSrG\wr S_{k}\times G\wr S_{r} to GSk+rG\wr S_{k+r} are known (see [8, Theorem 4.7] or [27, Theorem 4.5]), but we will give here only the cases for r=1,2r=1,2 as this is what we need in this paper.

Let 𝐤=[k1,,kl]{\bf k}=[k_{1},\ldots,k_{l}] be a composition of kk and let Λ𝐤\Lambda\Vdash{\bf k} be a multi-Young diagram and let SΛS^{\Lambda} be the associated GSkG\wr S_{k}-module. Let UiU_{i} be a G=GS1G=G\wr S_{1}-module. We can think of it as a multi-Young diagram with one box in the ii-th component and all the other components are empty. Let Yi+(Λ)Y^{+}_{i}(\Lambda) be the set of multi-Young diagrams that can be obtained from Λ\Lambda by adding one box at the ii-th component. Conversely, let Yi(Λ)Y^{-}_{i}(\Lambda) be the set of multi-Young diagrams obtained from Λ\Lambda by removing one box from the ii-th component.

Proposition 3.4.

The induction and restriction rules are as follows:

  1. 1.

    Induction:

    Ind(GSk)×GGSk+1(SΛUi)=ΓYi+(Λ)SΓ\operatorname{Ind}_{(G\wr S_{k})\times G}^{G\wr S_{k+1}}(S^{\Lambda}\boxtimes U_{i})=\bigoplus_{\Gamma\in Y^{+}_{i}(\Lambda)}S^{\Gamma}
  2. 2.

    Restriction: By Frobenius reciprocity, the restriction of a GSk+1G\wr S_{k+1}-module SΓS^{\Gamma} to the subgroup (GSk)×G(G\wr S_{k})\times G is given by:

    Res(GSk)×GGSk+1(SΓ)=i=1lΛYi(Γ)SΛUi\operatorname{Res}^{G\wr S_{k+1}}_{(G\wr S_{k})\times G}(S^{\Gamma})=\bigoplus_{i=1}^{l}\bigoplus_{\Lambda\in Y^{-}_{i}(\Gamma)}S^{\Lambda}\boxtimes U_{i}

For the case r=2r=2, we define the sets of multi-Young diagrams obtained by adding exactly two boxes to Λ\Lambda:

  • Yi,j+(Λ)Y^{+}_{i,j}(\Lambda): one box added to component ii and one box added to component jj (iji\neq j).

  • Yi,H2+(Λ)Y^{+}_{i,H^{2}}(\Lambda): a horizontal strip of two boxes added to component ii. This means that we cannot add the two boxes in the same column.

  • Yi,V2+(Λ)Y^{+}_{i,V^{2}}(\Lambda): a vertical strip of two boxes added to component ii. This means that we cannot add the two boxes in the same row.

Proposition 3.5.

The induction from (GSk)×(GS2)(G\wr S_{k})\times(G\wr S_{2}) to GSk+2G\wr S_{k+2} for the various simple GS2G\wr S_{2}-modules is given by:

Ind(GSk)×(GS2)GSk+2(SΛWi,j)=ΓYi,j+(Λ)SΓ\operatorname{Ind}_{(G\wr S_{k})\times(G\wr S_{2})}^{G\wr S_{k+2}}(S^{\Lambda}\boxtimes W_{i,j})=\bigoplus_{\Gamma\in Y^{+}_{i,j}(\Lambda)}S^{\Gamma}
Ind(GSk)×(GS2)GSk+2(SΛWi+)=ΓYi,H2+(Λ)SΓ\operatorname{Ind}_{(G\wr S_{k})\times(G\wr S_{2})}^{G\wr S_{k+2}}(S^{\Lambda}\boxtimes W_{i}^{+})=\bigoplus_{\Gamma\in Y^{+}_{i,H^{2}}(\Lambda)}S^{\Gamma}
Ind(GSk)×(GS2)GSk+2(SΛWi)=ΓYi,V2+(Λ)SΓ\operatorname{Ind}_{(G\wr S_{k})\times(G\wr S_{2})}^{G\wr S_{k+2}}(S^{\Lambda}\boxtimes W_{i}^{-})=\bigoplus_{\Gamma\in Y^{+}_{i,V^{2}}(\Lambda)}S^{\Gamma}

4 The quiver of (GPTn)\mathbb{C}(G\wr\operatorname{PT}_{n})

4.1 Ehresmann structure

For every X[n]={1,n}X\subseteq[n]=\{1,\ldots n\} we define idX\operatorname{id}_{X} to be the partial identity of the set XX

idX(x)={xif xX,undefinedotherwise,\operatorname{id}_{X}(x)=\begin{cases}x&\text{if }x\in X,\\ \text{undefined}&\text{otherwise,}\end{cases}

and 𝟏X:[n]G{\bf 1}_{X}:[n]\to G to be the function

𝟏X(x)={1Gif xX,undefinedotherwise.{\bf 1}_{X}(x)=\begin{cases}1_{G}&\text{if }x\in X,\\ \text{undefined}&\text{otherwise.}\end{cases}

Set ={(𝟏X,idX)X[n]}\mathcal{E}=\{({\bf 1}_{X},\operatorname{id}_{X})\mid X\subseteq[n]\} and note that this is a subsemilattice of GPTnG\wr\operatorname{PT}_{n}. It is routine to verify that the idempotent (𝟏X,idX)(\mathbf{1}_{X},\operatorname{id}_{X}) is a left (right) identity of (f,α)GPTn(f,\alpha)\in G\wr\operatorname{PT}_{n} if and only if im(α)X\operatorname{im}(\alpha)\subseteq X (respectively, dom(α)X\operatorname{dom}(\alpha)\subseteq X). Therefore, we have that two elements (f,α)(f,\alpha) and (g,β)(g,\beta) of GPTnG\wr\operatorname{PT}_{n} are ~\widetilde{\mathcal{L}}_{\mathcal{E}}-related if and only if dom(α)=dom(β)\operatorname{dom}(\alpha)=\operatorname{dom}(\beta), and they are ~\widetilde{\mathcal{R}}_{\mathcal{E}}-related if and only if im(α)=im(β)\operatorname{im}(\alpha)=\operatorname{im}(\beta). In other words, if X=dom(α)X=\operatorname{dom}(\alpha) and Y=im(α)Y=\operatorname{im}(\alpha) then

(f,α)=(𝟏X,idX),(f,α)+=(𝟏Y,idY).(f,\alpha)^{\ast}=({\bf 1}_{X},\operatorname{id}_{X}),\quad(f,\alpha)^{+}=({\bf 1}_{Y},\operatorname{id}_{Y}).

In [2, Proposition 9.11], it was proved that GPTnG\wr\operatorname{PT}_{n} is a right \mathcal{E}-restriction monoid. It is also easy to prove that the left congruence condition holds.

Lemma 4.1.

The relation ~\widetilde{\mathcal{R}}_{\mathcal{E}} is a left congruence on GPTnG\wr\operatorname{PT}_{n}.

Proof.

Let (f1,α1),(f2,α2)GPTn(f_{1},\alpha_{1}),(f_{2},\alpha_{2})\in G\wr\operatorname{PT}_{n} such that (f1,α1)~(f2,α2)(f_{1},\alpha_{1})\widetilde{\mathcal{R}}_{\mathcal{E}}(f_{2},\alpha_{2}). This is equivalent to im(α1)=im(α2)\operatorname{im}(\alpha_{1})=\operatorname{im}(\alpha_{2}). Let (f3,α3)(f_{3},\alpha_{3}) be any element in GPTnG\wr\operatorname{PT}_{n}. Note that im(α3α1)=im(α3α2)\operatorname{im}(\alpha_{3}\alpha_{1})=\operatorname{im}(\alpha_{3}\alpha_{2}) so

(f3,α3)(f1,α1)=((f3α1)f1,α3α1)~((f3α2)f2,α3α2)=(f3,α3)(f2,α2).(f_{3},\alpha_{3})(f_{1},\alpha_{1})=((f_{3}\ast\alpha_{1})\cdot f_{1},\alpha_{3}\alpha_{1})\tilde{\mathcal{R}}_{\mathcal{E}}((f_{3}\ast\alpha_{2})\cdot f_{2},\alpha_{3}\alpha_{2})=(f_{3},\alpha_{3})(f_{2},\alpha_{2}).

Thus, ~\widetilde{\mathcal{R}}_{\mathcal{E}} is a left congruence. ∎

It follows that GPTnG\wr\operatorname{PT}_{n} is a \mathcal{E}-Ehresmann and right restriction monoid. This will be crucial in view of the following fact.

Theorem 4.2 ([28, Theorem 1.5]).

Let MM be a finite EE-Ehresmann and right restriction monoid and let 𝐂(M){\bf C}(M) be its associated Ehresmann category. Then, for every unital commutative ring 𝕜\Bbbk there is an isomorphism of algebras 𝕜M𝕜𝐂(M)\Bbbk M\simeq\Bbbk{\bf C}(M)

Therefore, we can switch to studying the representation theory of the associated category 𝐂(GPTn){\bf C}(G\wr\operatorname{PT}_{n}). We start by describing it. The objects of 𝐂(GPTn)\mathbf{C}(G\wr\operatorname{PT}_{n}) are in one-to-one correspondence with the elements of \mathcal{E}. Thus, the objects are of the form (𝟏X,idX)(\mathbf{1}_{X},\operatorname{id}_{X}) for X[n]X\subseteq[n]. For two subsets X,Y[n]X,Y\subseteq[n], the hom-set 𝐂(GPTn)((𝟏X,idX),(𝟏Y,idY))\mathbf{C}(G\wr\operatorname{PT}_{n})((\mathbf{1}_{X},\operatorname{id}_{X}),(\mathbf{1}_{Y},\operatorname{id}_{Y})) is identified with the elements (f,α)GPTn(f,\alpha)\in G\wr\operatorname{PT}_{n} such that

(f,α)=(𝟏X,idX)and(f,α)+=(𝟏Y,idY).(f,\alpha)^{*}=(\mathbf{1}_{X},\operatorname{id}_{X})\quad\text{and}\quad(f,\alpha)^{+}=(\mathbf{1}_{Y},\operatorname{id}_{Y}).

Note that in this case, X=dom(α)X=\operatorname{dom}(\alpha) and Y=im(α)Y=\operatorname{im}(\alpha). We denote by C(f,α)C(f,\alpha) the morphism associated with (f,α)(f,\alpha).

Let En\operatorname{E}_{n} be the category defined as follows. The objects of En\operatorname{E}_{n} are subsets X[n]X\subseteq[n]. For X,Y[n]X,Y\subseteq[n], the hom-set En(X,Y)\operatorname{E}_{n}(X,Y) contains all the onto (total) functions α:XY\alpha\colon X\to Y. Let GG be a group. We denote by GEnG\wr\operatorname{E}_{n} the wreath product GHEnG\wr_{H}\operatorname{E}_{n}, where H:En𝐒𝐞𝐭H\colon\operatorname{E}_{n}\to\operatorname{\bf{Set}} is the inclusion functor.

Proposition 4.3.

There is an isomorphism of categories 𝐂(GPTn)GEn\mathbf{C}(G\wr\operatorname{PT}_{n})\simeq G\wr\operatorname{E}_{n}.

Proof.

It follows immediately from the above discussion. Formally, an isomorphism

ψ:𝐂(GPTn)GEn\psi\colon\mathbf{C}(G\wr\operatorname{PT}_{n})\to G\wr\operatorname{E}_{n}

is defined by ψ((𝟏X,idX))=X\psi((\mathbf{1}_{X},\operatorname{id}_{X}))=X and ψ(C(f,α))=(f,α)\psi(C(f,\alpha))=(f,\alpha). Note that if C(f,α)C(f,\alpha) is a morphism in 𝐂(GPTn)((𝟏X,idX),(𝟏Y,idY))\mathbf{C}(G\wr\operatorname{PT}_{n})((\mathbf{1}_{X},\operatorname{id}_{X}),(\mathbf{1}_{Y},\operatorname{id}_{Y})), then dom(α)=X\operatorname{dom}(\alpha)=X and im(α)=Y\operatorname{im}(\alpha)=Y, so α\alpha is indeed a total onto function α:XY\alpha\colon X\to Y. Moreover, dom(f)=X\operatorname{dom}(f)=X, so fGXf\in G^{X} as required in the definition of GEnG\wr\operatorname{E}_{n}. It is easy to see now that ψ\psi is an isomorphism. ∎

4.2 The skeleton

If 𝒞\mathcal{C} and 𝒟\mathcal{D} are equivalent categories, then their algebras are Morita equivalent (see [33, Proposition 2.2]). Since the quiver of an algebra is an invariant of Morita equivalence, we can switch our attention to a simpler category which is equivalent to GEnG\wr\operatorname{E}_{n}.

We can take a full subcategory with one object from every isomorphism class in GEnG\wr\operatorname{E}_{n}. This category is called the skeleton of GEnG\wr\operatorname{E}_{n}. To describe it, we first have to characterize which objects in GEnG\wr\operatorname{E}_{n} are isomorphic.

Lemma 4.4.

Two objects X,YX,Y in GEnG\wr\operatorname{E}_{n} are isomorphic if and only if |X|=|Y||X|=|Y|.

Proof.

First, note that if |X|<|Y||X|<|Y|, then the hom-set (GEn)(X,Y)(G\wr\operatorname{E}_{n})(X,Y) is empty because there are no onto functions from XX to YY. If XX and YY are isomorphic, then both (GEn)(X,Y)(G\wr\operatorname{E}_{n})(X,Y) and (GEn)(Y,X)(G\wr\operatorname{E}_{n})(Y,X) are non-empty, which implies |X|=|Y||X|=|Y|.

Conversely, if |X|=|Y||X|=|Y|, we can take any invertible function α:XY\alpha\colon X\to Y, and we claim that (𝟏X,α)(\mathbf{1}_{X},\alpha) is an isomorphism with inverse (𝟏Y,α1)(\mathbf{1}_{Y},\alpha^{-1}). Indeed,

(𝟏Y,α1)(𝟏X,α)\displaystyle(\mathbf{1}_{Y},\alpha^{-1})\cdot(\mathbf{1}_{X},\alpha) =((𝟏Yα)𝟏X,α1α)\displaystyle=((\mathbf{1}_{Y}\ast\alpha)\cdot\mathbf{1}_{X},\alpha^{-1}\alpha)
=((𝟏Yα)𝟏X,idX).\displaystyle=((\mathbf{1}_{Y}\ast\alpha)\cdot\mathbf{1}_{X},\operatorname{id}_{X}).

Note that since im(α)=Y\operatorname{im}(\alpha)=Y, we have 𝟏Yα=𝟏X\mathbf{1}_{Y}\ast\alpha=\mathbf{1}_{X}. Therefore,

(𝟏Y,α1)(𝟏X,α)=(𝟏X𝟏X,idX)=(𝟏X,idX),(\mathbf{1}_{Y},\alpha^{-1})\cdot(\mathbf{1}_{X},\alpha)=(\mathbf{1}_{X}\cdot\mathbf{1}_{X},\operatorname{id}_{X})=(\mathbf{1}_{X},\operatorname{id}_{X}),

which is the identity morphism of the object XX. Likewise, since αα1=idY\alpha\alpha^{-1}=\operatorname{id}_{Y}, it follows that (𝟏X,α)(𝟏Y,α1)=(𝟏Y,idY)(\mathbf{1}_{X},\alpha)\cdot(\mathbf{1}_{Y},\alpha^{-1})=(\mathbf{1}_{Y},\operatorname{id}_{Y}). ∎

Denote by GSEnG\wr\operatorname{SE}_{n} the full subcategory of GEnG\wr\operatorname{E}_{n} whose objects are the sets [0]=[0]=\emptyset and [k]={1,,k}[k]=\{1,\dots,k\} for 1kn1\leq k\leq n. As the notation suggests, this category can be identified with the wreath product of GG with the category SEn\operatorname{SE}_{n}, where the set of objects is {[k]0kn}\{[k]\mid 0\leq k\leq n\} and the morphisms are total onto functions. Following the discussion above, to determine the quiver of the original algebra, it suffices to focus our attention on the quiver of the algebra (GSEn)\mathbb{C}(G\wr\operatorname{SE}_{n}).

It is also convenient to describe GSEnG\wr\operatorname{SE}_{n} using matrices. Let 𝒟n\mathcal{D}_{n} be the category defined as follows. The set of objects of 𝒟n\mathcal{D}_{n} is {[k]0kn}\{[k]\mid 0\leq k\leq n\}. For 0k,rn0\leq k,r\leq n, the hom-set 𝒟n([k],[r])\mathcal{D}_{n}([k],[r]) consists of all r×kr\times k matrices over G{0}G\cup\{0\} with exactly one non-zero element in every column and at least one non-zero element in every row. Composition of morphisms is given by standard matrix multiplication, which is well-defined because each column contains only one group element.

It is straightforward to see that there is an isomorphism of categories GSEn𝒟nG\wr\operatorname{SE}_{n}\simeq\mathcal{D}_{n}. To each morphism (f,α)(GSEn)([k],[r])(f,\alpha)\in(G\wr\operatorname{SE}_{n})([k],[r]), we associate an r×kr\times k matrix [f,α][f,\alpha] defined by:

[f,α]i,j={f(j)if α(j)=i,0otherwise.[f,\alpha]_{i,j}=\begin{cases}f(j)&\text{if }\alpha(j)=i,\\ 0&\text{otherwise.}\end{cases}

By construction, the jj-th column of [f,α][f,\alpha] contains a unique non-zero element in the α(j)\alpha(j)-th row. The condition that α\alpha is surjective implies that every row contains at least one non-zero element. It is routine to verify that this assignment respects composition and thus defines an isomorphism of categories.

4.3 The quiver of a skeletal EI-category algebra

A category is called an EI-category if its endomorphism monoids are groups. In other words, in an EI-category, every endomorphism is an isomorphism.

The category GSEnG\wr\operatorname{SE}_{n} is an EI-category because for any morphism (f,α):[k][k](f,\alpha)\colon[k]\to[k], the map α\alpha is a surjective map from a finite set to itself, which is necessarily a bijection. Therefore, the endomorphism monoid of an object [k][k] is the group GSkG\wr S_{k}.

The problem of finding the ordinary quiver of the complex algebra of a skeletal EI-category can be reduced to a problem in group representation theory. We define a few concepts below and then state the relevant theorem.

For any finite set XX, we denote by X\mathbb{C}X (or [X]\mathbb{C}[X]) the complex vector space consisting of all formal linear combinations of elements of XX. If a group GG acts on XX, then X\mathbb{C}X naturally becomes a G\mathbb{C}G-module called a permutation module.

Let 𝒜\mathcal{A} be a finite EI-category. A morphism m𝒜1m\in\mathcal{A}^{1} is called irreducible if it is not an isomorphism, and whenever m=m1m2m=m_{1}m_{2}, either m1m_{1} or m2m_{2} is an isomorphism. We denote the set of irreducible morphisms from object cc to object cc^{\prime} by Irr(𝒜)(c,c)\operatorname{Irr}(\mathcal{A})(c,c^{\prime}). Recall that we denote the set of simple modules of a group GG by IRep(G)\operatorname{IRep}(G).

Theorem 4.5 ([16, Theorem 6.13], [11, Theorem 4.7]).

Let 𝒜\mathcal{A} be a finite skeletal EI-category and let QQ be the quiver of 𝒜\mathbb{C}\mathcal{A}. Then:

  1. 1.

    The set of vertices of QQ is given by

    c𝒜0IRep(𝒜(c,c)).\bigsqcup_{c\in\mathcal{A}^{0}}\operatorname{IRep}(\mathcal{A}(c,c)).
  2. 2.

    The vector space [Irr(𝒜)(c,c)]\mathbb{C}[\operatorname{Irr}(\mathcal{A})(c,c^{\prime})] can be viewed as an (𝒜(c,c)×𝒜(c,c))(\mathcal{A}(c^{\prime},c^{\prime})\times\mathcal{A}(c,c))-module with the action given by (h,g)f=hfg1(h,g)\bullet f=hfg^{-1}. For VIRep(𝒜(c,c))V\in\operatorname{IRep}(\mathcal{A}(c,c)) and UIRep(𝒜(c,c))U\in\operatorname{IRep}(\mathcal{A}(c^{\prime},c^{\prime})), the number of arrows from VV to UU is the multiplicity of UVU\otimes V^{*} as a simple constituent in [Irr(𝒜)(c,c)]\mathbb{C}[\operatorname{Irr}(\mathcal{A})(c,c^{\prime})].

In view of the theorem above, the vertices of the quiver QQ of (GSEn)\mathbb{C}(G\wr\operatorname{SE}_{n}) are indexed by the simple modules of the automorphism groups GSkG\wr S_{k} for each object [k][k] in GSEnG\wr\operatorname{SE}_{n}. Since GG has ll conjugacy classes, these modules are indexed by multipartitions (or equivalently, multi-Young diagrams) Λ\Lambda with kk boxes and ll components, where kk varies from 0 to nn.

4.4 Irreducible morphisms

The next step for using Theorem 4.5 is identifying the irreducible morphisms of GSEnG\wr\operatorname{SE}_{n}.

Lemma 4.6.

The irreducible morphisms of GSEnG\wr\operatorname{SE}_{n} are precisely the morphisms from [k+1][k+1] to [k][k] for 0k<n0\leq k<n. In other words,

Irr(GSEn)([p],[k])={GSEn([p],[k])if p=k+1,otherwise.\operatorname{Irr}(G\wr\operatorname{SE}_{n})([p],[k])=\begin{cases}G\wr\operatorname{SE}_{n}([p],[k])&\text{if }p=k+1,\\ \emptyset&\text{otherwise.}\end{cases}
Proof.

It is clear that every morphism (f,α)(f,\alpha) from [k+1][k+1] to [k][k] is irreducible. Indeed, if one decomposes (f,α)=(f1,α1)(f2,α2)(f,\alpha)=(f_{1},\alpha_{1})\cdot(f_{2},\alpha_{2}), the size of the sets implies that one of the factors must be an endomorphism and hence an isomorphism.

Now, if (f,α)GSEn([p],[k])(f,\alpha)\in G\wr\operatorname{SE}_{n}([p],[k]) where p>k+1p>k+1, then it is known that we can write α=α1α2\alpha=\alpha_{1}\alpha_{2} for some onto functions α2:[p][k+1]\alpha_{2}\colon[p]\to[k+1] and α1:[k+1][k]\alpha_{1}\colon[k+1]\to[k] (see [26, Lemma 3.3]). In this case, (𝟏[k+1],α1)(\mathbf{1}_{[k+1]},\alpha_{1}) and (f,α2)(f,\alpha_{2}) are both well-defined morphisms which are not endomorphisms and therefore are not invertible. Finally,

(𝟏[k+1],α1)(f,α2)=(𝟏[k+1]α2f,α1α2)=(𝟏[p]f,α1α2)=(f,α),(\mathbf{1}_{[k+1]},\alpha_{1})\cdot(f,\alpha_{2})=(\mathbf{1}_{[k+1]}\ast\alpha_{2}\cdot f,\alpha_{1}\alpha_{2})=(\mathbf{1}_{[p]}\cdot f,\alpha_{1}\alpha_{2})=(f,\alpha),

so (f,α)(f,\alpha) is not irreducible. ∎

Let VIRep(GSp)V\in\operatorname{IRep}(G\wr S_{p}) and UIRep(GSk)U\in\operatorname{IRep}(G\wr S_{k}). If pk+1p\neq k+1, there are no arrows in the quiver of (GSEn)\mathbb{C}(G\wr\operatorname{SE}_{n}) from VV to UU because Irr(GSEn)([p],[k])\operatorname{Irr}(G\wr\operatorname{SE}_{n})([p],[k]) is empty. Consequently, we focus on the case p=k+1p=k+1 and examine the module [Irr(GSEn)([k+1],[k])]\mathbb{C}[\operatorname{Irr}(G\wr\operatorname{SE}_{n})([k+1],[k])] under the action of GSk×GSk+1G\wr S_{k}\times G\wr S_{k+1} as described in Theorem 4.5.

For convenience, we denote the set of irreducible morphisms by

X=Irr(GSEn)([k+1],[k])={(f,α)α:[k+1][k] is onto,f:[k+1]G}.X=\operatorname{Irr}(G\wr\operatorname{SE}_{n})([k+1],[k])=\{(f,\alpha)\mid\alpha\colon[k+1]\to[k]\text{ is onto},\,f\colon[k+1]\to G\}.

The group GSk×GSk+1G\wr S_{k}\times G\wr S_{k+1} acts on XX via

((f1,σ1),(f2,σ2))(f,α)=(f1,σ1)(f,α)(f2,σ2)1,((f_{1},\sigma_{1}),(f_{2},\sigma_{2}))\bullet(f,\alpha)=(f_{1},\sigma_{1})\cdot(f,\alpha)\cdot(f_{2},\sigma_{2})^{-1},

where f1:[k]Gf_{1}\colon[k]\to G, f2:[k+1]Gf_{2}\colon[k+1]\to G, σ1Sk\sigma_{1}\in S_{k}, and σ2Sk+1\sigma_{2}\in S_{k+1}. The module of interest is the linearization X\mathbb{C}X, which is a permutation module for this action.

4.5 Description of the action and stabilizer

Lemma 4.7.

The action of GSk×GSk+1G\wr S_{k}\times G\wr S_{k+1} on XX is transitive.

Proof.

We show that every element of XX lies in the orbit of (𝟏[k+1],dec)(\mathbf{1}_{[k+1]},\operatorname{dec}), where dec:[k+1][k]\operatorname{dec}\colon[k+1]\to[k] is defined by

dec(i)={iif ik,kif i=k+1.\operatorname{dec}(i)=\begin{cases}i&\text{if }i\leq k,\\ k&\text{if }i=k+1.\end{cases}

Let (f,α)X(f,\alpha)\in X. It is easy to verify (also mentioned in [26, Section 3]) that the action of Sk×Sk+1S_{k}\times S_{k+1} on the set of surjective maps from [k+1][k+1] to [k][k] is transitive. Thus, there exist σ1Sk\sigma_{1}\in S_{k} and σ2Sk+1\sigma_{2}\in S_{k+1} such that σ1decσ2=α\sigma_{1}\operatorname{dec}\sigma_{2}=\alpha.

Taking (𝟏[k],σ1)GSk(\mathbf{1}_{[k]},\sigma_{1})\in G\wr S_{k} and (f,σ2)1GSk+1(f,\sigma_{2})^{-1}\in G\wr S_{k+1}, we observe that:

(𝟏[k],σ1)(𝟏[k+1],dec)((f,σ2)1)1\displaystyle(\mathbf{1}_{[k]},\sigma_{1})\cdot(\mathbf{1}_{[k+1]},\operatorname{dec})\cdot\left((f,\sigma_{2})^{-1}\right)^{-1} =(𝟏[k]dec𝟏[k+1],σ1dec)(f,σ2)\displaystyle=(\mathbf{1}_{[k]}\ast\operatorname{dec}\cdot\mathbf{1}_{[k+1]},\sigma_{1}\operatorname{dec})\cdot(f,\sigma_{2})
=(𝟏[k+1],σ1dec)(f,σ2)\displaystyle=(\mathbf{1}_{[k+1]},\sigma_{1}\operatorname{dec})\cdot(f,\sigma_{2})
=(𝟏[k+1]σ2f,σ1decσ2)\displaystyle=(\mathbf{1}_{[k+1]}\ast\sigma_{2}\cdot f,\sigma_{1}\operatorname{dec}\sigma_{2})
=(𝟏[k+1]f,σ1decσ2)\displaystyle=(\mathbf{1}_{[k+1]}\cdot f,\sigma_{1}\operatorname{dec}\sigma_{2})
=(f,α).\displaystyle=(f,\alpha).

Thus, the action is indeed transitive. ∎

Let KK be the stabilizer of (𝟏[k+1],dec)(\mathbf{1}_{[k+1]},\operatorname{dec}) under the action of GSk×GSk+1G\wr S_{k}\times G\wr S_{k+1} described above, and let trK\operatorname{tr}_{K} denote the trivial module of KK. Since X\mathbb{C}X is a permutation module arising from a transitive group action, it follows that

XIndKGSk×GSk+1(trK).\mathbb{C}X\simeq\operatorname{Ind}_{K}^{G\wr S_{k}\times G\wr S_{k+1}}(\operatorname{tr}_{K}).

To proceed, we must characterize the stabilizer KK more explicitly.

For the action of Sk×Sk+1S_{k}\times S_{k+1} on the set of surjective maps from [k+1][k+1] to [k][k], it is known that the stabilizer of dec\operatorname{dec} is the subgroup

{(σ,στ)σSk1,τS{k,k+1}}\{(\sigma,\sigma\tau)\mid\sigma\in S_{k-1},\,\tau\in S_{\{k,k+1\}}\}

(see [26, Lemma 3.5]). For any function fG[k]f\in G^{[k]}, let f^G[k+1]\hat{f}\in G^{[k+1]} be the function defined by

f^(i)={f(i)if ik,f(k)if i=k+1.\hat{f}(i)=\begin{cases}f(i)&\text{if }i\leq k,\\ f(k)&\text{if }i=k+1.\end{cases}

Note, in particular, that f^(k+1)=f^(k)\hat{f}(k+1)=\hat{f}(k).

Recall that we can view any element σSk1\sigma\in S_{k-1} as an element of SkS_{k} that fixes kk.

Lemma 4.8.

The stabilizer KK of (𝟏[k+1],dec)(\mathbf{1}_{[k+1]},\operatorname{dec}) under the action of GSk×GSk+1G\wr S_{k}\times G\wr S_{k+1} is given explicitly by

K={((f,σ),(f^,στ))σSk1,τS{k,k+1},fG[k]}.K=\{((f,\sigma),(\hat{f},\sigma\tau))\mid\sigma\in S_{k-1},\,\tau\in S_{\{k,k+1\}},\,f\in G^{[k]}\}.
Proof.

An element ((f,σ),(h,ϵ))((f,\sigma),(h,\epsilon)) is in KK if and only if

(f,σ)(𝟏[k+1],dec)(h,ϵ)1=(𝟏[k+1],dec),(f,\sigma)\cdot(\mathbf{1}_{[k+1]},\operatorname{dec})\cdot(h,\epsilon)^{-1}=(\mathbf{1}_{[k+1]},\operatorname{dec}),

or equivalently,

(f,σ)(𝟏[k+1],dec)=(𝟏[k+1],dec)(h,ϵ).(f,\sigma)\cdot(\mathbf{1}_{[k+1]},\operatorname{dec})=(\mathbf{1}_{[k+1]},\operatorname{dec})\cdot(h,\epsilon).

Applying the product rule for the wreath product on both sides, we obtain

(fdec𝟏[k+1],σdec)=(𝟏[k+1]ϵh,decϵ).(f\ast\operatorname{dec}\cdot\mathbf{1}_{[k+1]},\sigma\operatorname{dec})=(\mathbf{1}_{[k+1]}\ast\epsilon\cdot h,\operatorname{dec}\epsilon).

Since 𝟏[k+1]\mathbf{1}_{[k+1]} is the identity for the pointwise product, this simplifies to the condition

(fdec,σdec)=(h,decϵ).(f\ast\operatorname{dec},\sigma\operatorname{dec})=(h,\operatorname{dec}\epsilon).

The map equality σdec=decϵ\sigma\operatorname{dec}=\operatorname{dec}\epsilon implies that (σ,ϵ)(\sigma,\epsilon) is in the stabilizer of dec\operatorname{dec} under the action of Sk×Sk+1S_{k}\times S_{k+1}. It follows that σSk1\sigma\in S_{k-1} and ϵ=στ\epsilon=\sigma\tau for some τS{k,k+1}\tau\in S_{\{k,k+1\}}.

Finally, the function equality fdec=hf\ast\operatorname{dec}=h is equivalent to h=f^h=\hat{f}. Indeed, for iki\leq k, we have h(i)=f(dec(i))=f(i)h(i)=f(\operatorname{dec}(i))=f(i), and for i=k+1i=k+1, we have h(k+1)=f(dec(k+1))=f(k)h(k+1)=f(\operatorname{dec}(k+1))=f(k). This completes the proof. ∎

For any fG[k1]f\in G^{[k-1]} and gGg\in G, we define a function fgG[k]f^{g}\in G^{[k]} by

fg(i)={f(i)ik1gi=k.f^{g}(i)=\begin{cases}f(i)&i\leq k-1\\ g&i=k\end{cases}.

Note that every hG[k]h\in G^{[k]} can be uniquely written as h=fgh=f^{g} for some fG[k1]f\in G^{[k-1]} and gGg\in G.

In what follows, it will be useful to understand how elements of KK correspond to matrices over G{0}G\cup\{0\}. Given an element (fg,σ)(f^{g},\sigma) with σSk1\sigma\in S_{k-1}, its associated matrix consists of an (k1)×(k1)(k-1)\times(k-1) block AA associated with (f,σ)(f,\sigma) and a 1×11\times 1 block containing gg. Thus, (fg,σ)(f^{g},\sigma) corresponds to a block-diagonal matrix:

A(g)=(A00g).A\oplus(g)=\begin{pmatrix}\text{\Large$A$}&0\\ 0&g\end{pmatrix}.

For the element (fg^,στ)(\widehat{f^{g}},\sigma\tau), the associated matrix similarly decomposes into two blocks of sizes (k1)×(k1)(k-1)\times(k-1) and 2×22\times 2. The first block is AA, and the second is the 2×22\times 2 block gPτgP_{\tau}, where PτP_{\tau} is the permutation matrix associated with τ\tau:

(A𝟎𝟎gPτ).\begin{pmatrix}\text{\Large$A$}&\mathbf{0}\\ \mathbf{0}&gP_{\tau}\end{pmatrix}.
Lemma 4.9.

There is an isomorphism of groups

K(GSk1)×G×S2.K\simeq(G\wr S_{k-1})\times G\times S_{2}.
Proof.

Identify S2S_{2} with S{k,k+1}S_{\{k,k+1\}}. We define a map ψ:(GSk1)×G×S2K\psi:(G\wr S_{k-1})\times G\times S_{2}\to K by

ψ((f,σ),g,τ)=((fg,σ),(fg^,στ)).\psi((f,\sigma),g,\tau)=\left((f^{g},\sigma),(\widehat{f^{g}},\sigma\tau)\right).

By Lemma 4.8, it is clear that ψ\psi is a bijection. It remains to show that ψ\psi is a group homomorphism. Indeed,

ψ(((f1,σ1),g1,τ1)((f2,σ2),g2,τ2))\displaystyle\psi(((f_{1},\sigma_{1}),g_{1},\tau_{1})\cdot((f_{2},\sigma_{2}),g_{2},\tau_{2})) =ψ(((f1,σ1)(f2,σ2)),g1g2,τ1τ2)\displaystyle=\psi(((f_{1},\sigma_{1})\cdot(f_{2},\sigma_{2})),g_{1}g_{2},\tau_{1}\tau_{2})
=ψ((f1σ2f2,σ1σ2),g1g2,τ1τ2)\displaystyle=\psi((f_{1}\ast\sigma_{2}\cdot f_{2},\sigma_{1}\sigma_{2}),g_{1}g_{2},\tau_{1}\tau_{2})
=(((f1σ2f2)g1g2,σ1σ2),((f1σ2f2)g1g2^,σ1σ2τ1τ2))\displaystyle=(((f_{1}\ast\sigma_{2}\cdot f_{2})^{g_{1}g_{2}},\sigma_{1}\sigma_{2}),(\widehat{(f_{1}\ast\sigma_{2}\cdot f_{2})^{g_{1}g_{2}}},\sigma_{1}\sigma_{2}\tau_{1}\tau_{2}))

On the other hand

ψ((f1,σ1),g1,τ1)ψ((f2,σ2),g2,τ2)\displaystyle\psi((f_{1},\sigma_{1}),g_{1},\tau_{1})\cdot\psi((f_{2},\sigma_{2}),g_{2},\tau_{2}) =((f1g1,σ1),(f1g1^,σ1τ1))((f2g2,σ2),(f2g2^,σ2τ2))\displaystyle=((f_{1}^{g_{1}},\sigma_{1}),(\widehat{f_{1}^{g_{1}}},\sigma_{1}\tau_{1}))\cdot((f_{2}^{g_{2}},\sigma_{2}),(\widehat{f_{2}^{g_{2}}},\sigma_{2}\tau_{2}))
=((f1g1σ2f2g2,σ1σ2),(f1g1^σ2τ2f2g2^,σ1τ1σ2τ2)).\displaystyle=((f_{1}^{g_{1}}\ast\sigma_{2}\cdot f_{2}^{g_{2}},\sigma_{1}\sigma_{2}),(\widehat{f_{1}^{g_{1}}}\ast\sigma_{2}\tau_{2}\cdot\widehat{f_{2}^{g_{2}}},\sigma_{1}\tau_{1}\sigma_{2}\tau_{2})).

First note that

σ1σ2τ1τ2=σ1τ1σ2τ2\sigma_{1}\sigma_{2}\tau_{1}\tau_{2}=\sigma_{1}\tau_{1}\sigma_{2}\tau_{2}

because τ1\tau_{1} and σ2\sigma_{2} have disjoint supports and thus commute as elements of Sk+1S_{k+1}. Next, for ik1i\leq k-1, we have

(f1σ2f2)g1g2(i)=f1(σ2(i))f2(i)=f1g1(σ2(i))f2g2(i)(f_{1}\ast\sigma_{2}\cdot f_{2})^{g_{1}g_{2}}(i)=f_{1}(\sigma_{2}(i))\cdot f_{2}(i)=f_{1}^{g_{1}}(\sigma_{2}(i))\cdot f_{2}^{g_{2}}(i)

because σ2(i)k1\sigma_{2}(i)\leq k-1 as well. For i=ki=k, we have

(f1σ2f2)g1g2(k)=g1g2=f1g1(k)f2g2(k)=f1g1(σ2(k))f2g2(k)(f_{1}\ast\sigma_{2}\cdot f_{2})^{g_{1}g_{2}}(k)=g_{1}g_{2}=f_{1}^{g_{1}}(k)\cdot f_{2}^{g_{2}}(k)=f_{1}^{g_{1}}(\sigma_{2}(k))\cdot f_{2}^{g_{2}}(k)

since σ2\sigma_{2} fixes kk. This establishes that

(f1σ2f2)g1g2=f1g1σ2f2g2.(f_{1}\ast\sigma_{2}\cdot f_{2})^{g_{1}g_{2}}=f_{1}^{g_{1}}\ast\sigma_{2}\cdot f_{2}^{g_{2}}.

Proving the last equality is similar. For ik1i\leq k-1, we have again

(f1σ2f2)g1g2^(i)=f1(σ2(i))f2(i)\widehat{(f_{1}\ast\sigma_{2}\cdot f_{2})^{g_{1}g_{2}}}(i)=f_{1}(\sigma_{2}(i))\cdot f_{2}(i)

and

(f1g1^σ2τ2f2g2^)(i)\displaystyle\left(\widehat{f_{1}^{g_{1}}}\ast\sigma_{2}\tau_{2}\cdot\widehat{f_{2}^{g_{2}}}\right)(i) =f1g1^(σ2τ2(i))f2g2^(i)\displaystyle=\widehat{f_{1}^{g_{1}}}(\sigma_{2}\tau_{2}(i))\cdot\widehat{f_{2}^{g_{2}}}(i)
=f1(σ2(i))f2(i)\displaystyle=f_{1}(\sigma_{2}(i))\cdot f_{2}(i)

because τ2(i)=i\tau_{2}(i)=i for all ik1i\leq k-1. Finally, for kik+1k\leq i\leq k+1, we have

(f1σ2f2)g1g2^(i)=(f1σ2f2)g1g2(k)=g1g2\widehat{(f_{1}\ast\sigma_{2}\cdot f_{2})^{g_{1}g_{2}}}(i)=(f_{1}\ast\sigma_{2}\cdot f_{2})^{g_{1}g_{2}}(k)=g_{1}g_{2}

and

(f1g1^σ2τ2f2g2^)(i)=f1g1^(σ2τ2(i))f2g2^(i)=g1g2,\left(\widehat{f_{1}^{g_{1}}}\ast\sigma_{2}\tau_{2}\cdot\widehat{f_{2}^{g_{2}}}\right)(i)=\widehat{f_{1}^{g_{1}}}(\sigma_{2}\tau_{2}(i))\cdot\widehat{f_{2}^{g_{2}}}(i)=g_{1}g_{2},

where the last equality follows because σ2\sigma_{2} fixes {k,k+1}\{k,k+1\} and fjgj^\widehat{f_{j}^{g_{j}}} takes the value gjg_{j} on both kk and k+1k+1. This completes the proof. ∎

4.6 The quiver computation

Let UIRepGSkU\in\operatorname{IRep}G\wr S_{k} and VIRepGSk+1V\in\operatorname{IRep}G\wr S_{k+1}. To simplify the notation, we shall use the same notation for a module and its character. For example, we write UU and VV in place of χU\chi_{U} and χV\chi_{V}.

The number of arrows in the quiver of (GSEn)\mathbb{C}(G\wr\operatorname{SE}_{n}) from VV to UU is the multiplicity of UVU\otimes V^{\ast} as a simple module in the (GSk×GSk+1)(G\wr S_{k}\times G\wr S_{k+1})-module

X=IndKGSk×GSk+1trK.\mathbb{C}X=\operatorname{Ind}_{K}^{G\wr S_{k}\times G\wr S_{k+1}}\operatorname{tr}_{K}.

This multiplicity can be expressed as the inner product of characters:

UV,IndKGSk×GSk+1trK.\langle U\otimes V^{\ast},\operatorname{Ind}_{K}^{G\wr S_{k}\times G\wr S_{k+1}}\operatorname{tr}_{K}\rangle.

Using Frobenius reciprocity, this equals

ResKGSk×GSk+1(UV),trK.\displaystyle\langle\operatorname{Res}_{K}^{G\wr S_{k}\times G\wr S_{k+1}}(U\otimes V^{\ast}),\operatorname{tr}_{K}\rangle.

According to Lemma 4.8, a general element of KK is of the form

((fg,σ),(fg^,στ))((f^{g},\sigma),(\hat{f^{g}},\sigma\tau))

where σSk1,τS{k,k+1},fG[k1],gG\sigma\in S_{k-1},\,\tau\in S_{\{k,k+1\}},\,f\in G^{[k-1]},\,g\in G. Therefore,

ResKGSk×GSk+1(UV),trK\displaystyle\langle\operatorname{Res}_{K}^{G\wr S_{k}\times G\wr S_{k+1}}(U\otimes V^{\ast}),\operatorname{tr}_{K}\rangle
=1|K|fG[k1],gGσSk1,τS2UV(((fg,σ),(fg^,στ)))trK(((fg,σ),(fg^,στ)))\displaystyle=\frac{1}{|K|}\sum_{\begin{subarray}{c}f\in G^{[k-1]},g\in G\\ \sigma\in S_{k-1},\tau\in S_{2}\end{subarray}}U\otimes V^{\ast}(((f^{g},\sigma),(\hat{f^{g}},\sigma\tau)))\operatorname{tr}_{K}(((f^{g},\sigma),(\hat{f^{g}},\sigma\tau)))
=1|K|fG[k1],gGσSk1,τS2U((fg,σ))V((fg^,στ))\displaystyle=\frac{1}{|K|}\sum_{\begin{subarray}{c}f\in G^{[k-1]},g\in G\\ \sigma\in S_{k-1},\tau\in S_{2}\end{subarray}}U((f^{g},\sigma))\cdot V^{\ast}((\hat{f^{g}},\sigma\tau))
=1|K|fG[k1],gGσSk1,τS2U((fg,σ))V((fg^,στ))¯.\displaystyle=\frac{1}{|K|}\sum_{\begin{subarray}{c}f\in G^{[k-1]},g\in G\\ \sigma\in S_{k-1},\tau\in S_{2}\end{subarray}}U((f^{g},\sigma))\cdot\overline{V((\hat{f^{g}},\sigma\tau))}.

Now, if we think of (fg^,στ)(\hat{f^{g}},\sigma\tau) as a (k1)×(k1)(k-1)\times(k-1) and 2×22\times 2 block matrix, it is just a general element of GSk1×G×S2G\wr S_{k-1}\times G\times S_{2} so we can write

V((fg^,στ))=ResGSk1×(G×S2)GSk+1V((fg^,στ))V((\hat{f^{g}},\sigma\tau))=\operatorname{Res}^{G\wr S_{k+1}}_{G\wr S_{k-1}\times(G\times S_{2})}V((\hat{f^{g}},\sigma\tau))

Likewise, if we view (fg,σ)(f^{g},\sigma) as a (k1)×(k1)(k-1)\times(k-1) and 1×11\times 1 block matrix, it is a general element of GSk1×GG\wr S_{k-1}\times G so

U((fg,σ))=ResGSk1×GGSkU((fg,σ)).U((f^{g},\sigma))=\operatorname{Res}^{G\wr S_{k}}_{G\wr S_{k-1}\times G}U((f^{g},\sigma)).

In order to view this also as a K=(GSk1×(G×S2))K=(G\wr S_{k-1}\times(G\times S_{2})) module we will write this as

ResGSk1×GGSkU((fg,σ))tr2(τ).\operatorname{Res}^{G\wr S_{k}}_{G\wr S_{k-1}\times G}U((f^{g},\sigma))\cdot\operatorname{tr}_{2}(\tau).

where tr2\operatorname{tr}_{2} is the trivial module of S2S_{2}. Therefore, we obtain

ResKGSk×GSk+1(UV),trK\displaystyle\langle\operatorname{Res}_{K}^{G\wr S_{k}\times G\wr S_{k+1}}(U\otimes V^{\ast}),\operatorname{tr}_{K}\rangle
=1|K|fG[k1],gGσSk1,τS2U((fg,σ))V((fg^,στ))¯\displaystyle=\frac{1}{|K|}\sum_{\begin{subarray}{c}f\in G^{[k-1]},g\in G\\ \sigma\in S_{k-1},\tau\in S_{2}\end{subarray}}U((f^{g},\sigma))\cdot\overline{V((\hat{f^{g}},\sigma\tau))}
=1|K|fG[k1],gGσSk1,τS2(ResGSk1×GGSkU((fg,σ))tr2(τ))ResGSk1×(G×S2)GSk+1V((fg^,στ))¯\displaystyle=\frac{1}{|K|}\sum_{\begin{subarray}{c}f\in G^{[k-1]},g\in G\\ \sigma\in S_{k-1},\tau\in S_{2}\end{subarray}}\left(\operatorname{Res}^{G\wr S_{k}}_{G\wr S_{k-1}\times G}U((f^{g},\sigma))\cdot\operatorname{tr}_{2}(\tau)\right)\cdot\overline{\operatorname{Res}^{G\wr S_{k+1}}_{G\wr S_{k-1}\times(G\times S_{2})}V((\hat{f^{g}},\sigma\tau))}
=1|K|((f,σ),(g,τ))(GSk1)×(G×S2)((ResGSk1×GGSkU)tr2)((fg,σ,τ))ResGSk1×(G×S2)GSk+1V((fg^,στ))¯\displaystyle=\frac{1}{|K|}\sum_{\begin{subarray}{c}((f,\sigma),(g,\tau))\\ \in(G\wr S_{k-1})\times(G\times S_{2})\end{subarray}}((\operatorname{Res}^{G\wr S_{k}}_{G\wr S_{k-1}\times G}U)\boxtimes\operatorname{tr}_{2})((f^{g},\sigma,\tau))\cdot\overline{\operatorname{Res}^{G\wr S_{k+1}}_{G\wr S_{k-1}\times(G\times S_{2})}V((\hat{f^{g}},\sigma\tau))}
=(ResGSk1×GGSkU)tr2,ResGSk1×(G×S2)GSk+1V.\displaystyle=\langle(\operatorname{Res}^{G\wr S_{k}}_{G\wr S_{k-1}\times G}U)\boxtimes\operatorname{tr}_{2},\operatorname{Res}^{G\wr S_{k+1}}_{G\wr S_{k-1}\times(G\times S_{2})}V\rangle.

By Frobenius reciprocity, this equals

IndGSk1×(G×S2)GSk+1((ResGSk1×GGSkU)tr2),V.\langle\operatorname{Ind}^{G\wr S_{k+1}}_{G\wr S_{k-1}\times(G\times S_{2})}((\operatorname{Res}^{G\wr S_{k}}_{G\wr S_{k-1}\times G}U)\boxtimes\operatorname{tr}_{2}),V\rangle.

By transitivity of induction we obtain

IndGSk1×(GS2)GSk+1IndGSk1×(G×S2)GSk1×(GS2)((ResGSk1×GGSkU)tr2),V.\langle\operatorname{Ind}^{G\wr S_{k+1}}_{G\wr S_{k-1}\times(G\wr S_{2})}\operatorname{Ind}^{G\wr S_{k-1}\times(G\wr S_{2})}_{G\wr S_{k-1}\times(G\times S_{2})}((\operatorname{Res}^{G\wr S_{k}}_{G\wr S_{k-1}\times G}U)\boxtimes\operatorname{tr}_{2}),V\rangle.

Now we analyze this expression using the branching rules described in Section 3. Let UU be a simple module of GSkG\wr S_{k} corresponding to a multipartition Λ\Lambda.

By Proposition 3.4, we have

Res(GSk)×GGSk+1(SΛ)=r=1lΓYr(Λ)SΓUr,\operatorname{Res}^{G\wr S_{k+1}}_{(G\wr S_{k})\times G}(S^{\Lambda})=\bigoplus_{r=1}^{l}\bigoplus_{\Gamma\in Y^{-}_{r}(\Lambda)}S^{\Gamma}\boxtimes U_{r},

where ΓYr(Λ)\Gamma\in Y^{-}_{r}(\Lambda) means that Γ\Gamma is obtained by removing one box from the rr-th component of Λ\Lambda. Let SΓUrS^{\Gamma}\boxtimes U_{r} be one component in this summation. The next step is to compute the induction

IndGSk1×(G×S2)GSk1×(GS2)(SΓUrtr2)\operatorname{Ind}^{G\wr S_{k-1}\times(G\wr S_{2})}_{G\wr S_{k-1}\times(G\times S_{2})}(S^{\Gamma}\boxtimes U_{r}\boxtimes\operatorname{tr}_{2})

For this we need to compute the induction

Ind(G×S2)GS2(Urtr2).\operatorname{Ind}^{G\wr S_{2}}_{(G\times S_{2})}(U_{r}\boxtimes\operatorname{tr}_{2}).

Let mi,jrm^{r}_{i,j} be the multiplicity of UrU_{r} in UiUjU_{i}\otimes U_{j}, let mi+,rm^{+,r}_{i} be the multiplicity of UrU_{r} in Sym2Ui\operatorname{Sym}^{2}U_{i}, and let mi,rm^{-,r}_{i} be the multiplicity of UrU_{r} in Alt2Ui\operatorname{Alt}^{2}U_{i}. According to Lemma 3.2 and Lemma 3.3 we have that

Ind(G×S2)GS2(Urtr2)=1i<jl(mi,jrWi,j)i=1l(mi+,rWi+mi,rWi)\operatorname{Ind}^{G\wr S_{2}}_{(G\times S_{2})}(U_{r}\boxtimes\operatorname{tr}_{2})=\bigoplus_{1\leq i<j\leq l}\left(m^{r}_{i,j}W_{i,j}\right)\oplus\bigoplus_{i=1}^{l}\left(m^{+,r}_{i}W^{+}_{i}\oplus m^{-,r}_{i}W^{-}_{i}\right)

so

IndGSk1×(G×S2)GSk1×(GS2)(SΓUrtr2)=1i<jl(mi,jr(SΓWi,j))i=1l(mi+,r(SΓWi+)mi,r(SΓWi)).\operatorname{Ind}^{G\wr S_{k-1}\times(G\wr S_{2})}_{G\wr S_{k-1}\times(G\times S_{2})}\left(S^{\Gamma}\boxtimes U_{r}\boxtimes\operatorname{tr}_{2}\right)=\bigoplus_{1\leq i<j\leq l}\left(m^{r}_{i,j}(S^{\Gamma}\boxtimes W_{i,j})\right)\oplus\bigoplus_{i=1}^{l}\left(m^{+,r}_{i}(S^{\Gamma}\boxtimes W^{+}_{i})\oplus m^{-,r}_{i}(S^{\Gamma}\boxtimes W^{-}_{i})\right).

Finally, by Proposition 3.5 we have that

IndGSk1×(GS2)GSk+1(1i<jlmi,jr(SΓWi,j)i=1l(mi+,r(SΓWi+)mi,r(SΓWi)))=\operatorname{Ind}^{G\wr S_{k+1}}_{G\wr S_{k-1}\times(G\wr S_{2})}\left(\bigoplus_{1\leq i<j\leq l}m^{r}_{i,j}(S^{\Gamma}\boxtimes W_{i,j})\oplus\bigoplus_{i=1}^{l}\left(m^{+,r}_{i}(S^{\Gamma}\boxtimes W^{+}_{i})\oplus m^{-,r}_{i}(S^{\Gamma}\boxtimes W^{-}_{i})\right)\right)=
1i<jl(mi,jrΔYi,j+(Γ)SΔ)i=1l(mi+,rΔYi,H2+(Γ)SΔmi,rΔYi,V2+(Γ)SΔ.)\bigoplus_{1\leq i<j\leq l}\left(m^{r}_{i,j}\bigoplus_{\Delta\in Y^{+}_{i,j}(\Gamma)}S^{\Delta}\right)\oplus\bigoplus_{i=1}^{l}\left(m_{i}^{+,r}\bigoplus_{\Delta\in Y^{+}_{i,H^{2}}(\Gamma)}S^{\Delta}\oplus m_{i}^{-,r}\bigoplus_{\Delta\in Y^{+}_{i,V^{2}}(\Gamma)}S^{\Delta}.\right)

From this we can conclude:

Theorem 4.10.

Let GG be a group with ll conjugacy classes and let IRepG={U1,,Ul}\operatorname{IRep}G=\{U_{1},\ldots,U_{l}\}. Define mi,jr,mi+,r,mi,rm^{r}_{i,j},m^{+,r}_{i},m^{-,r}_{i} as above. The quiver QQ of the monoid GPTnG\wr\operatorname{PT}_{n} is described as follows. The vertices correspond to multi-Young diagrams with ll components and kk boxes, where kk varies from 0 to nn. Let UU be a multi-Young diagram with kk boxes, and VV be a multi-Young diagram with pp boxes. If pk+1p\neq k+1, then there are no arrows from VV to UU. If p=k+1p=k+1, then the number of arrows depends on the ways that VV can be constructed from UU by removing one box and adding two. For each way that VV can be constructed from UU by removing one box from the rr-th component and adding one box in components ii and jj (iji\neq j) we add mi,jrm^{r}_{i,j} arrows. In each way that VV can be constructed from UU by removing one box from the rr-th component and adding two boxes on the ii-th component but not on the same column we add mi+,rm^{+,r}_{i} arrows. In each way that VV can be constructed from UU by removing one box from the rr-th component and adding two boxes on the ii-th component but not on the same row we add mi,rm^{-,r}_{i} arrows.

4.7 Examples

4.7.1 The quiver of PTn\mathbb{C}\operatorname{PT}_{n}

If GG is the trivial group then GPTnPTnG\wr\operatorname{PT}_{n}\simeq\operatorname{PT}_{n}. In this case, IRepG\operatorname{IRep}G contains only the trivial module U1=trGU_{1}=\operatorname{tr}_{G}. Clearly Sym2trG=trG\operatorname{Sym}^{2}\operatorname{tr}_{G}=\operatorname{tr}_{G} and Alt2trG=0\operatorname{Alt}^{2}\operatorname{tr}_{G}=0. Therefore, m1+,1=1m^{+,1}_{1}=1 and m1,1=0m^{-,1}_{1}=0. Therefore, we retrieve [26, Theorem 3.8]:

Theorem 4.11.

The vertices of the quiver QQ of the monoid algebra PTn\mathbb{C}\operatorname{PT}_{n} correspond to Young diagrams with kk boxes where kk varies from 0 to nn. Let UU be a Young diagram with kk boxes and VV be a Young diagram with pp boxes. If pk+1p\neq k+1, then there are no arrows from VV to UU. If p=k+1p=k+1, then the number of arrows from VV to UU is the number of ways that VV can be constructed from UU by removing one box and adding two, but not in the same column.

4.7.2 Generalized monoid of partial functions

Let G=ClG=C_{l} be the cyclic group with ll elements, say G={1G,g,g2,,gl1}G=\{1_{G},g,g^{2},\dots,g^{l-1}\} where gl=1Gg^{l}=1_{G}. All simple modules ρIRep G\rho\in\text{IRep }G are one-dimensional. There are ll such modules, ρr\rho_{r} for r=0,,l1r=0,\dots,l-1, defined by:

ρr(gn)=ωrn\rho_{r}(g^{n})=\omega^{rn}

where ω=e2πi/l\omega=e^{2\pi i/l} is a primitive ll-th root of unity. These modules satisfy ρiρj=ρi+j\rho_{i}\otimes\rho_{j}=\rho_{i+j}, where the sum is taken modulo ll. Since each ρr\rho_{r} is one-dimensional, its symmetric square and alternating square satisfy:

Sym2ρr=ρrρr=ρ2randAlt2ρr=0\text{Sym}^{2}\rho_{r}=\rho_{r}\otimes\rho_{r}=\rho_{2r}\quad\text{and}\quad\text{Alt}^{2}\rho_{r}=0

Therefore, the decomposition coefficients mi,jrm_{i,j}^{r} for the tensor product are given by mi,jr=1m_{i,j}^{r}=1 if i+jr(modl)i+j\equiv r\pmod{l} and zero otherwise. For the symmetric and alternating squares, the coefficients are mi+,r=1m^{+,r}_{i}=1 if 2ir(modl)2i\equiv r\pmod{l} and zero otherwise, while mi,r=0m^{-,r}_{i}=0 for all r{0,,l1}r\in\{0,\dots,l-1\}. We end with the following result:

Theorem 4.12.

The vertices of the quiver QQ of the monoid algebra (ClPTn)\mathbb{C}(C_{l}\wr\operatorname{PT}_{n}) correspond to mutli-Young diagrams with ll components, indexed {0,l1}\{0,\ldots l-1\}, and kk boxes, where kk varies from 0 to nn. Let UU be a multi-Young diagram with kk boxes and VV be a multi-Young diagram with pp boxes. If pk+1p\neq k+1, then there are no arrows from VV to UU. If p=k+1p=k+1, then the number of arrows depends on the ways that VV can be constructed from UU by removing one box and adding two. For each way that VV can be constructed from UU by removing one box from the rr-th component and adding one box in components iiand jj we add an arrow if i+jr(modl)i+j\equiv r\pmod{l}. In each way that VV can be constructed from UU by removing one box from the rr-th component and adding two boxes on the ii-th component but not on the same column we add an arrow if 2ir(modl)2i\equiv r\pmod{l}.

Example 4.13.

Consider the case G=C2G=C_{2}. The quiver of the algebra (C2PT3)\mathbb{C}(C_{2}\wr\operatorname{PT}_{3}) is given by the following figure:

(,)\left(\emptyset,\emptyset\right)(,)\left(\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular},\emptyset\right)(,)\left(\emptyset,\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular}\right)(,)\left(\begin{tabular}[]{|c|c|}\hline\cr\phantom{.}&\phantom{.}\\ \hline\cr\end{tabular},\emptyset\right)(,)\left(\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\phantom{.}\\ \hline\cr\end{tabular},\emptyset\right)(,)\left(\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular},\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular}\right)(,)\left(\emptyset,\begin{tabular}[]{|c|c|}\hline\cr\phantom{.}&\phantom{.}\\ \hline\cr\end{tabular}\right)(,)\left(\emptyset,\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\phantom{.}\\ \hline\cr\end{tabular}\right)(,)\left(\begin{tabular}[]{|c|c|c|}\hline\cr\phantom{.}&\phantom{.}&\phantom{.}\\ \hline\cr\end{tabular},\emptyset\right)(,)\left(\begin{tabular}[]{|c|c|}\hline\cr\phantom{.}&\phantom{.}\\ \hline\cr\phantom{.}&\lx@intercol\hfil\hfil\lx@intercol \\ \cline{1-1}\cr\end{tabular},\emptyset\right)( ,)\left(\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\phantom{.}\\ \hline\cr\phantom{.}\\ \hline\cr\end{tabular},\emptyset\right)(,)\left(\begin{tabular}[]{|c|c|}\hline\cr\phantom{.}&\phantom{.}\\ \hline\cr\end{tabular},\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular}\right)(,)\left(\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\phantom{.}\\ \hline\cr\end{tabular},\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular}\right)(,)\left(\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular},\begin{tabular}[]{|c|c|}\hline\cr\phantom{.}&\phantom{.}\\ \hline\cr\end{tabular}\right)(,)\left(\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular},\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\phantom{.}\\ \hline\cr\end{tabular}\right)(,)\left(\emptyset,\begin{tabular}[]{|c|c|c|}\hline\cr\phantom{.}&\phantom{.}&\phantom{.}\\ \hline\cr\end{tabular}\right)(,)\left(\emptyset,\begin{tabular}[]{|c|c|}\hline\cr\phantom{.}&\phantom{.}\\ \hline\cr\phantom{.}&\lx@intercol\hfil\hfil\lx@intercol \\ \cline{1-1}\cr\end{tabular}\right)(, )\left(\emptyset,\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\phantom{.}\\ \hline\cr\phantom{.}\\ \hline\cr\end{tabular}\right)

The first component of each multi-Young diagram corresponds to the trivial module ρ0\rho_{0}, while the second component corresponds to the alternating module ρ1\rho_{1}.

Notably, there are two arrows from (,)\left(\begin{tabular}[]{|c|c|}\hline\cr\phantom{.}&\phantom{.}\\ \hline\cr\end{tabular}\,,\,\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular}\right) to (,)\left(\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular}\,,\,\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular}\right) . This multiplicity arises because the branching construction can be satisfied in two distinct ways:

  • First, by removing one box from the first component (r=0r=0) and adding two boxes in the same row, which is valid since 0+00(mod2)0+0\equiv 0\pmod{2}.

  • Second, by removing one box from the second component (r=1r=1) and adding one box to each component, which is valid since 0+11(mod2)0+1\equiv 1\pmod{2}.

4.7.3 The quiver of (S3PTn)\mathbb{C}(S_{3}\wr\operatorname{PT}_{n})

We now consider the case of the smallest non-abelian group G=S3G=S_{3}. The set IRep(G)\operatorname{IRep}(G) contains three simple modules: The trivial module U1U_{1}, the sign module U2U_{2}, and the standard module U3U_{3}. It is well-known and easily verified by character considerations that the symmetric and alternating squares satisfy:

Sym2U1\displaystyle\operatorname{Sym}^{2}U_{1} =Sym2U2=U1,\displaystyle=\operatorname{Sym}^{2}U_{2}=U_{1}, Sym2U3\displaystyle\operatorname{Sym}^{2}U_{3} =U3U1,\displaystyle=U_{3}\oplus U_{1},
Alt2U1\displaystyle\operatorname{Alt}^{2}U_{1} =Alt2U2=0,\displaystyle=\operatorname{Alt}^{2}U_{2}=0, Alt2U3\displaystyle\operatorname{Alt}^{2}U_{3} =U2.\displaystyle=U_{2}.

Furthermore, the tensor products are given by:

U1U2=U2,U1U3=U3,U2U3=U3.U_{1}\otimes U_{2}=U_{2},\quad U_{1}\otimes U_{3}=U_{3},\quad U_{2}\otimes U_{3}=U_{3}.

Therefore, the coefficients mi,jrm_{i,j}^{r} are given by:

m1,2r={1if r=2,0otherwise,andm1,3r=m2,3r={1if r=3,0otherwise.m_{1,2}^{r}=\begin{cases}1&\text{if }r=2,\\ 0&\text{otherwise,}\end{cases}\quad\text{and}\quad m_{1,3}^{r}=m_{2,3}^{r}=\begin{cases}1&\text{if }r=3,\\ 0&\text{otherwise.}\end{cases}

The coefficients m1q,r,m2q,rm_{1}^{q,r},m_{2}^{q,r}, where q{+,}q\in\{+,-\}, satisfy:

m1q,r=m2q,r={1if q=+ and r=1,0otherwise.m_{1}^{q,r}=m_{2}^{q,r}=\begin{cases}1&\text{if }q=+\text{ and }r=1,\\ 0&\text{otherwise.}\end{cases}

Finally, for the coefficients m3q,rm_{3}^{q,r}, where q{+,}q\in\{+,-\}, we have:

m3+,r={1if r{1,3},0otherwise,andm3,r={1if r=2,0otherwise.m_{3}^{+,r}=\begin{cases}1&\text{if }r\in\{1,3\},\\ 0&\text{otherwise,}\end{cases}\quad\text{and}\quad m_{3}^{-,r}=\begin{cases}1&\text{if }r=2,\\ 0&\text{otherwise.}\end{cases}

Therefore, we obtain:

Theorem 4.14.

The vertices of the quiver QQ of the monoid algebra (S3PTn)\mathbb{C}(S_{3}\wr\operatorname{PT}_{n}) correspond to multi-Young diagrams 𝚲=(λ1,λ2,λ3)\boldsymbol{\Lambda}=(\lambda_{1},\lambda_{2},\lambda_{3}) with kk total boxes, where 0kn0\leq k\leq n. Let UU be a multi-Young diagram with kk boxes and VV be a multi-Young diagram with pp boxes.

If pk+1p\neq k+1, there are no arrows from VV to UU. If p=k+1p=k+1, the number of arrows from VV to UU is the number of ways VV can be constructed from UU by removing one box and adding two boxes according to the following rules:

  • Remove one box from λ1\lambda_{1} and add two boxes to any one component, provided they are not in the same column.

  • Remove one box from λ2\lambda_{2} and add one box to λ1\lambda_{1} and one box to λ2\lambda_{2}.

  • Remove one box from λ2\lambda_{2} and add two boxes to λ3\lambda_{3}, provided they are not in the same row.

  • Remove one box from λ3\lambda_{3} and add one box to λ1\lambda_{1} or λ2\lambda_{2} and another box to λ3\lambda_{3}.

  • Remove one box from λ3\lambda_{3} and add two boxes to λ3\lambda_{3}, provided they are not in the same column.

Example 4.15.

The quiver of the algebra (S3PT2)\mathbb{C}(S_{3}\wr\operatorname{PT}_{2}) is given by the following figure:

(,,)(\emptyset,\emptyset,\emptyset)(,,)(\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular},\emptyset,\emptyset)(,,)(\emptyset,\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular},\emptyset)(,,)(\emptyset,\emptyset,\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular})(,,)(\begin{tabular}[]{|c|c|}\hline\cr\phantom{.}&\phantom{.}\\ \hline\cr\end{tabular},\emptyset,\emptyset)(,,)(\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\phantom{.}\\ \hline\cr\end{tabular},\emptyset,\emptyset)(,,)(\emptyset,\begin{tabular}[]{|c|c|}\hline\cr\phantom{.}&\phantom{.}\\ \hline\cr\end{tabular},\emptyset)(,,)(\emptyset,\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\phantom{.}\\ \hline\cr\end{tabular},\emptyset)(,,)(\emptyset,\emptyset,\begin{tabular}[]{|c|c|}\hline\cr\phantom{.}&\phantom{.}\\ \hline\cr\end{tabular})(,,)(\emptyset,\emptyset,\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\phantom{.}\\ \hline\cr\end{tabular})(,,)(\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular},\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular},\emptyset)(,,)(\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular},\emptyset,\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular})(,,)(\emptyset,\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular},\begin{tabular}[]{|c|}\hline\cr\phantom{.}\\ \hline\cr\end{tabular})

5 Global dimension of (GPTn)\mathbb{C}(G\wr\operatorname{PT}_{n})

In this section, we prove that the global dimension of the algebra (GPTn)\mathbb{C}(G\wr\operatorname{PT}_{n}) is n1n-1 based on the results established for the algebra PTn\mathbb{C}\operatorname{PT}_{n} in [29]. We show that every projective module of PTn\mathbb{C}\operatorname{PT}_{n} can be lifted to a corresponding projective module of (GPTn)\mathbb{C}(G\wr\operatorname{PT}_{n}), allowing us to transfer the known homological properties to the wreath product case.

5.1 The global dimension of an algebra

Let AA be a finite-dimensional \mathbb{C}-algebra. An AA-module PP is projective if the functor HomA(P,)\text{Hom}_{A}(P,-) is exact, or equivalently, if PP is a direct summand of a free module. A module is indecomposable if it cannot be written as a direct sum of two non-zero submodules. Every projective AA-module decomposes into a direct sum of indecomposable projective modules.

These modules are classified by the idempotents of the algebra. Two idempotents e,fe,f are orthogonal if ef=fe=0ef=fe=0. An idempotent is primitive if it cannot be written as a sum of two non-zero orthogonal idempotents. A set {e1,,en}\{e_{1},\dots,e_{n}\} is a complete set of orthogonal primitive idempotents if the elements are pairwise orthogonal, each eie_{i} is primitive, and ei=1A\sum e_{i}=1_{A}. Every indecomposable projective AA-module is isomorphic to AeAe for some primitive idempotent ee, and a complete set of primitive orthogonal idempotents yields all indecomposable projectives up to isomorphism.

Let AA be a finite-dimensional \mathbb{C}-algebra. The Jacobson radical of AA, denoted Rad(A)\operatorname{Rad}(A), is defined as the intersection of all maximal left ideals of AA. Equivalently, Rad(A)\operatorname{Rad}(A) is the unique maximal nilpotent two-sided ideal of AA. For any finite-dimensional AA-module MM, we define its radical, Rad(M)\operatorname{Rad}(M), as the intersection of all maximal submodules of MM. A fundamental property of the radical is that it can be computed via the action of the algebra’s radical. Specifically, we have the identity Rad(M)=Rad(A)M\operatorname{Rad}(M)=\operatorname{Rad}(A)M.

Let AA be a finite-dimensional \mathbb{C}-algebra and MM an AA-module. A projective cover of MM is a pair (P,π)(P,\pi), where PP is a projective AA-module and π:PM\pi:P\to M is a surjection such that ker(π)Rad(P)\ker(\pi)\subseteq\operatorname{Rad}(P).

For the algebras considered here, every finite-dimensional module MM admits a projective cover, which is unique up to isomorphism.

Let AA be a finite-dimensional \mathbb{C}-algebra and MM an AA-module. A projective resolution of MM is an exact sequence of the form

𝐏:PndnPn1P1d1P0ϵM0\mathbf{P}_{\bullet}:\dots\to P_{n}\xrightarrow{d_{n}}P_{n-1}\to\dots\to P_{1}\xrightarrow{d_{1}}P_{0}\xrightarrow{\epsilon}M\to 0

where each PiP_{i} is a projective AA-module. Such a resolution is called minimal if P0P_{0} is the projective cover of MM, and for each i1i\geq 1, PiP_{i} is the projective cover of ker(di1)\ker(d_{i-1}).

Every finite-dimensional module MM possesses a minimal projective resolution, which is unique up to isomorphism of complexes. The projective dimension of MM, denoted pd(M)\operatorname{pd}(M), is the length of its minimal projective resolution, that is, the largest integer nn such that Pn0P_{n}\neq 0 (or infinity if the resolution does not terminate). For a finite-dimensional algebra AA, the global dimension of AA, denoted glDim(A)\operatorname{glDim}(A), is the supremum of the projective dimensions of all simple AA-modules:

glDim(A)=sup{pd(S)S is a simple A-module}\operatorname{glDim}(A)=\sup\{\operatorname{pd}(S)\mid S\text{ is a simple }A\text{-module}\}

The global dimension is an invariant of the Morita equivalence class of the algebra AA. If two algebras are Morita equivalent, their global dimensions are equal. Moreover, it is a known fact for finite-dimensional algebras that the global dimension is bounded above by the length of the longest path in the quiver of the algebra.

5.2 Lifting projective resolutions of EI-categories

Let E\operatorname{E} be a category and GG be a finite group. For simplicity, assume that E\operatorname{E} is a subcategory of 𝐒𝐞𝐭\operatorname{\bf{Set}} so that there is a natural wreath product GEG\wr\operatorname{E}. Clearly, every E\mathbb{C}\operatorname{E}-module MM can be inflated to a (GE)\mathbb{C}(G\wr\operatorname{E})-module via the action (f,m)v=mv(f,m)\bullet v=m\bullet v. We denote the inflation of MM to (GE)\mathbb{C}(G\wr\operatorname{E}) by Inf(M)\operatorname{Inf}(M). In fact, we consider Inf\operatorname{Inf} as a functor between the category of E\mathbb{C}\operatorname{E}-modules and (GE)\mathbb{C}(G\wr\operatorname{E})-modules. In this subsection, we show that if E\operatorname{E} is an EI-category the inflation functor lifts the minimal projective resolution of MM to the minimal projective resolution of Inf(M)\operatorname{Inf}(M).

Let E\operatorname{E} be an EI-category. For every object eE0e\in\operatorname{E}^{0}, we denote by HeH_{e} the associated endomorphism group, and let PeP_{e} be a complete set of orthogonal primitive idempotents of He\mathbb{C}H_{e}. It is known (see [12, Lemma 9.31] or [33, Corollary 4.5]) that we can obtain a complete set of orthogonal primitive idempotents PP of E\mathbb{C}\operatorname{E} by taking the union of all complete sets of orthogonal primitive idempotents of the endomorphism groups:

P=eE0Pe.P=\bigcup_{e\in\operatorname{E}^{0}}P_{e}.

Therefore, if VV is a simple He\mathbb{C}H_{e}-module isomorphic to Hep\mathbb{C}H_{e}p for some pPep\in P_{e}, then

EpEeHeHepEeHeV\mathbb{C}\operatorname{E}p\cong\mathbb{C}\operatorname{E}e\otimes_{\mathbb{C}H_{e}}\mathbb{C}H_{e}p\cong\mathbb{C}\operatorname{E}e\otimes_{\mathbb{C}H_{e}}V

is an indecomposable projective module of E\mathbb{C}\operatorname{E}. Moreover, every indecomposable projective module is isomorphic to EeHeV\mathbb{C}\operatorname{E}e\otimes_{\mathbb{C}H_{e}}V for some eE0e\in\operatorname{E}^{0} and VIRep(He)V\in\operatorname{IRep}(\mathbb{C}H_{e}).

It is straightforward to verify that GEG\wr\operatorname{E} is also an EI-category with the same set of objects E0\operatorname{E}^{0}. For any object eE0e\in\operatorname{E}^{0}, the associated endomorphism group in the wreath product category is GHeG\wr H_{e}. Given a simple module VIRep(He)V\in\operatorname{IRep}(\mathbb{C}H_{e}), its inflation Inf(V)\operatorname{Inf}(V) is a module over (GHe)\mathbb{C}(G\wr H_{e}), which remains simple under the action defined previously. The relationship between the inflation functor and the indecomposable projectives is captured by the following lemma.

Lemma 5.1.

Let eE0e\in\operatorname{E}^{0} and VIRep(He)V\in\operatorname{IRep}(\mathbb{C}H_{e}). Then there is an isomorphism of (GE)\mathbb{C}(G\wr\operatorname{E})-modules:

Inf(EeHeV)(GE)e(GHe)Inf(V).\operatorname{Inf}(\mathbb{C}\operatorname{E}e\otimes_{\mathbb{C}H_{e}}V)\simeq\mathbb{C}(G\wr\operatorname{E})e\otimes_{\mathbb{C}(G\wr H_{e})}\operatorname{Inf}(V).
Proof.

We denote by 𝟏e\mathbf{1}_{e} the function in GeG^{e} that maps every element of the set ee to the identity 1G1_{G} and by ide\operatorname{id}_{e} we denote the identity function of ee. To establish the isomorphism

Inf(EeHeV)(GE)e(GHe)Inf(V),\operatorname{Inf}(\mathbb{C}\operatorname{E}e\otimes_{\mathbb{C}H_{e}}V)\cong\mathbb{C}(G\wr\operatorname{E})e\otimes_{\mathbb{C}(G\wr H_{e})}\operatorname{Inf}(V),

we first observe that for every (f,m)(GE)e(f,m)\in(G\wr\operatorname{E})e and vVv\in V we have

(f,m)v=((𝟏e,m)(f,ide))v=(𝟏e,m)(f,ide)v=(𝟏e,m)(idev)=(𝟏e,m)v,\begin{split}(f,m)\otimes v&=((\mathbf{1}_{e},m)\cdot(f,\operatorname{id}_{e}))\otimes v\\ &=(\mathbf{1}_{e},m)\otimes(f,\operatorname{id}_{e})\bullet v\\ &=(\mathbf{1}_{e},m)\otimes(\operatorname{id}_{e}\bullet v)\\ &=(\mathbf{1}_{e},m)\otimes v,\end{split}

Next, define a linear map

Ψ:Inf(EeHeV)(GE)e(GHe)Inf(V).\Psi:\operatorname{Inf}(\mathbb{C}\operatorname{E}e\otimes_{\mathbb{C}H_{e}}V)\to\mathbb{C}(G\wr\operatorname{E})e\otimes_{\mathbb{C}(G\wr H_{e})}\operatorname{Inf}(V).

on simple tensors by

Ψ(mv)=(𝟏e,m)v,\Psi(m\otimes v)=(\mathbf{1}_{e},m)\otimes v,

where mEem\in\mathbb{C}\operatorname{E}e and vVv\in V. To see that Ψ\Psi is well-defined, note that for any hHeh\in H_{e}, the inflation action on VV satisfies (𝟏e,h)v=hv(\mathbf{1}_{e},h)\bullet v=h\bullet v. Thus,

Ψ(mhv)=(𝟏e,mh)v=(𝟏e,m)(𝟏e,h)v=(𝟏e,m)(𝟏e,h)v=(𝟏e,m)hv=Ψ(mhv),\begin{split}\Psi(mh\otimes v)&=(\mathbf{1}_{e},mh)\otimes v\\ &=(\mathbf{1}_{e},m)(\mathbf{1}_{e},h)\otimes v\\ &=(\mathbf{1}_{e},m)\otimes(\mathbf{1}_{e},h)\bullet v\\ &=(\mathbf{1}_{e},m)\otimes h\bullet v\\ &=\Psi(m\otimes h\bullet v),\end{split}

which confirms Ψ\Psi respects the tensor relation over He\mathbb{C}H_{e}.

To verify that Ψ\Psi is a (GE)\mathbb{C}(G\wr\operatorname{E})-module homomorphism, let (f,m)GE(f,m^{\prime})\in G\wr\operatorname{E} where mE(e,e′′)m^{\prime}\in\operatorname{E}(e^{\prime},e^{\prime\prime}) and let mvEeHeVm\otimes v\in\mathbb{C}\operatorname{E}e\otimes_{\mathbb{C}H_{e}}V where mE(e,e)m\in\operatorname{E}(e,e^{\prime}). By the definition of the inflation action, we have:

Ψ((f,m)(mv))=Ψ(mmv)=(𝟏e,mm)v.\Psi((f,m^{\prime})\bullet(m\otimes v))=\Psi(m^{\prime}m\otimes v)=(\mathbf{1}_{e},m^{\prime}m)\otimes v.

On the other hand, acting on the image gives:

(f,m)Ψ(mv)=(f,m)((𝟏e,m)v)=((f,m)(𝟏e,m))v=(fm𝟏e,mm)v=(fm,mm)v=(𝟏e,mm)v.\begin{split}(f,m^{\prime})\bullet\Psi(m\otimes v)&=(f,m^{\prime})\bullet((\mathbf{1}_{e},m)\otimes v)\\ &=((f,m^{\prime})\cdot(\mathbf{1}_{e},m))\otimes v\\ &=(f\ast m\cdot\mathbf{1}_{e},m^{\prime}m)\otimes v\\ &=(f\ast m,m^{\prime}m)\otimes v\\ &=(\mathbf{1}_{e},m^{\prime}m)\otimes v.\end{split}

To prove that Ψ\Psi is an isomorphism, we construct its inverse

Φ:(GE)e(GHe)Inf(V)Inf(EeHeV).\Phi:\mathbb{C}(G\wr\operatorname{E})e\otimes_{\mathbb{C}(G\wr H_{e})}\operatorname{Inf}(V)\to\operatorname{Inf}(\mathbb{C}\operatorname{E}e\otimes_{\mathbb{C}H_{e}}V).

Define Φ\Phi on spanning elements by Φ((f,m)v)=mv\Phi((f,m)\otimes v)=m\otimes v. To show that Φ\Phi is well-defined, let (g,h)GHe(g,h)\in G\wr H_{e}; then:

Φ((f,m)(g,h)v)=Φ((fhg,mh)v)=mhv.\begin{split}\Phi((f,m)\cdot(g,h)\otimes v)&=\Phi((f\ast h\cdot g,mh)\otimes v)\\ &=mh\otimes v.\end{split}

On the other hand:

Φ((f,m)(g,h)v)=Φ((f,m)hv)=mhv=mhv.\begin{split}\Phi((f,m)\otimes(g,h)\bullet v)&=\Phi((f,m)\otimes h\bullet v)\\ &=m\otimes h\bullet v\\ &=mh\otimes v.\end{split}

Thus Φ\Phi is well-defined.

To show that Φ\Phi is a (GE)\mathbb{C}(G\wr\operatorname{E})-module homomorphism, let (g,m)GE(g,m^{\prime})\in G\wr\operatorname{E} and (f,m)v(f,m)\otimes v be a spanning element of the domain. We have:

Φ((g,m)((f,m)v))=Φ(((g,m)(f,m))v)=Φ((gmf,mm)v)=mmv.\begin{split}\Phi((g,m^{\prime})\bullet((f,m)\otimes v))&=\Phi(((g,m^{\prime})\cdot(f,m))\otimes v)\\ &=\Phi((g\ast m\cdot f,m^{\prime}m)\otimes v)\\ &=m^{\prime}m\otimes v.\end{split}

On the other hand, acting after applying Φ\Phi gives:

(g,m)Φ((f,m)v)=(g,m)(mv)=mmv,\begin{split}(g,m^{\prime})\bullet\Phi((f,m)\otimes v)&=(g,m^{\prime})\bullet(m\otimes v)\\ &=m^{\prime}m\otimes v,\end{split}

so Φ\Phi is a (GE)\mathbb{C}(G\wr\operatorname{E})-module homomorphism.

From the definitions it follows immediately that ΦΨ\Phi\circ\Psi is the identity on Inf(EeHeV)\operatorname{Inf}(\mathbb{C}\operatorname{E}e\otimes_{\mathbb{C}H_{e}}V), as:

Φ(Ψ(mv))=Φ((𝟏e,m)v)=mv.\Phi(\Psi(m\otimes v))=\Phi((\mathbf{1}_{e},m)\otimes v)=m\otimes v.

Conversely, for any (f,m)v(f,m)\otimes v in the target, we previously established the identity (f,m)v=(𝟏e,m)v(f,m)\otimes v=(\mathbf{1}_{e},m)\otimes v. Therefore:

Ψ(Φ((f,m)v))=Ψ(mv)=(𝟏e,m)v=(f,m)v,\Psi(\Phi((f,m)\otimes v))=\Psi(m\otimes v)=(\mathbf{1}_{e},m)\otimes v=(f,m)\otimes v,

which shows ΨΦ\Psi\circ\Phi is the identity. Thus, Ψ\Psi is an isomorphism of (GE)\mathbb{C}(G\wr\operatorname{E})-modules. ∎

As a consequence of the fact that inflation preserves the structure of indecomposable projective modules, we obtain the following result regarding general projective modules.

Corollary 5.2.

If PP is a projective E\mathbb{C}\operatorname{E}-module, then its inflation Inf(P)\operatorname{Inf}(P) is a projective (GE)\mathbb{C}(G\wr\operatorname{E})-module.

Proof.

Each projective E\mathbb{C}\operatorname{E}-module PP can be decomposed into a direct sum of indecomposable projectives, each isomorphic to EeHeV\mathbb{C}\operatorname{E}e\otimes_{\mathbb{C}H_{e}}V for some eE0e\in\operatorname{E}^{0} and VIRep(He)V\in\operatorname{IRep}(\mathbb{C}H_{e}). According to Lemma 5.1, the inflation of each such indecomposable projective is an indecomposable projective (GE)\mathbb{C}(G\wr\operatorname{E})-module. Since the inflation functor Inf\operatorname{Inf} preserves direct sums, it follows that Inf(P)\operatorname{Inf}(P) is a direct sum of projective modules and is, therefore, projective. ∎

The next step is to characterize the radical of an EI-category algebra.

Proposition 5.3 ([11, Proposition 4.6]).

Let E\operatorname{E} be a finite EI-category. The radical Rad(E)\operatorname{Rad}(\mathbb{C}\operatorname{E}) is the subspace spanned by all non-invertible morphisms in E\operatorname{E}.

In an EI-category, a morphism mE(e,e)m\in\operatorname{E}(e,e^{\prime}) is non-invertible if and only if its domain and codomain are not isomorphic (e≄ee\not\simeq e^{\prime}).

Lemma 5.4.

Let PP be a projective E\mathbb{C}\operatorname{E}-module. Then Inf(RadP)=Rad(InfP)\operatorname{Inf}(\operatorname{Rad}P)=\operatorname{Rad}(\operatorname{Inf}P).

Proof.

First, assume PP is an indecomposable projective module. Then PEeHeVP\simeq\mathbb{C}\operatorname{E}e\otimes_{\mathbb{C}H_{e}}V for some eE0e\in\operatorname{E}^{0} and VIRep(He)V\in\operatorname{IRep}(\mathbb{C}H_{e}). The radical of PP is given by RadP=Rad(E)P=Rad(E)eHeV\operatorname{Rad}P=\operatorname{Rad}(\mathbb{C}\operatorname{E})P=\operatorname{Rad}(\mathbb{C}\operatorname{E})e\otimes_{\mathbb{C}H_{e}}V. Using the characterization of the radical for EI-category algebras, RadP\operatorname{Rad}P and Inf(RadP)\operatorname{Inf}(\operatorname{Rad}P) are spanned by the set

S={mvmE(e,e),e≄e,vV}.S=\{m\otimes v\mid m\in\operatorname{E}(e,e^{\prime}),\ e^{\prime}\not\simeq e,\ v\in V\}.

On the other hand, by Lemma 5.1, Inf(P)(GE)e(GHe)InfV\operatorname{Inf}(P)\simeq\mathbb{C}(G\wr\operatorname{E})e\otimes_{\mathbb{C}(G\wr H_{e})}\operatorname{Inf}V. The radical of the latter is Rad((GE))e(GHe)InfV\operatorname{Rad}(\mathbb{C}(G\wr\operatorname{E}))e\otimes_{\mathbb{C}(G\wr H_{e})}\operatorname{Inf}V, which is spanned by simple tensors of the form (f,m)v(f,m)\otimes v where mE(e,e)m\in\operatorname{E}(e,e^{\prime}) and e≄ee^{\prime}\not\simeq e. As shown in the proof of Lemma 5.1, (f,m)v=(𝟏e,m)v(f,m)\otimes v=(\mathbf{1}_{e},m)\otimes v.

Under the isomorphism Φ:(GE)e(GHe)InfVInfP\Phi:\mathbb{C}(G\wr\operatorname{E})e\otimes_{\mathbb{C}(G\wr H_{e})}\operatorname{Inf}V\to\operatorname{Inf}P, the image of the spanning set

{(𝟏e,m)vmE(e,e),e≄e,vV}\{(\mathbf{1}_{e},m)\otimes v\mid m\in\operatorname{E}(e,e^{\prime}),\ e\not\simeq e^{\prime},\ v\in V\}

is exactly the set SS defined above. Therefore, SS also spans Rad(InfP)\operatorname{Rad}(\operatorname{Inf}P). Since both Inf(RadP)\operatorname{Inf}(\operatorname{Rad}P) and Rad(InfP)\operatorname{Rad}(\operatorname{Inf}P) are spanned by the same set of elements within InfP\operatorname{Inf}P, we have Rad(InfP)=Inf(RadP)\operatorname{Rad}(\operatorname{Inf}P)=\operatorname{Inf}(\operatorname{Rad}P).

The result for a general projective module PP follows immediately from the fact that PP is a direct sum of indecomposable projectives and both the radical and the inflation functor preserve direct sums. ∎

Lemma 5.5.

Let MM be a E\mathbb{C}\operatorname{E}-module and let P𝜋MP\xrightarrow{\pi}M be its projective cover. Then Inf(P)Inf(π)Inf(M)\operatorname{Inf}(P)\xrightarrow{\operatorname{Inf}(\pi)}\operatorname{Inf}(M) is the projective cover of the (GE)\mathbb{C}(G\wr\operatorname{E})-module Inf(M)\operatorname{Inf}(M).

Proof.

Recall that a surjective homomorphism π:PM\pi:P\to M is a projective cover if and only if PP is a projective module and ker(π)Rad(P)\ker(\pi)\subseteq\operatorname{Rad}(P).

Applying Inf\operatorname{Inf} yields

Inf(P)Inf(π)Inf(M),\operatorname{Inf}(P)\xrightarrow{\operatorname{Inf}(\pi)}\operatorname{Inf}(M),

and it is clear that Inf(π)\operatorname{Inf}(\pi) is surjective and ker(Inf(π))Inf(ker(π))\ker(\operatorname{Inf}(\pi))\simeq\operatorname{Inf}(\ker(\pi)).

Next, we know from Lemma 5.1 that Inf(P)\operatorname{Inf}(P) is a projective (GE)\mathbb{C}(G\wr\operatorname{E})-module. Finally, applying the result of our previous lemma, we have:

ker(Inf(π))Inf(ker(π))Inf(RadP)=Rad(InfP).\ker(\operatorname{Inf}(\pi))\simeq\operatorname{Inf}(\ker(\pi))\subseteq\operatorname{Inf}(\operatorname{Rad}P)=\operatorname{Rad}(\operatorname{Inf}P).

Since Inf(P)\operatorname{Inf}(P) is projective and the kernel of the surjection is contained in its radical, Inf(P)Inf(π)Inf(M)\operatorname{Inf}(P)\xrightarrow{\operatorname{Inf}(\pi)}\operatorname{Inf}(M) is the projective cover of Inf(M)\operatorname{Inf}(M). ∎

Corollary 5.6.

Let 𝐏M\mathbf{P}_{\bullet}\to M be a minimal projective resolution of a E\mathbb{C}\operatorname{E}-module MM. Then the inflated sequence Inf(𝐏)Inf(M)\operatorname{Inf}(\mathbf{P}_{\bullet})\to\operatorname{Inf}(M) is a minimal projective resolution of the (GE)\mathbb{C}(G\wr\operatorname{E})-module Inf(M)\operatorname{Inf}(M).

Proof.

Let 𝐏\mathbf{P}_{\bullet} be the resolution P1d1P0ϵM0\dots\to P_{1}\xrightarrow{d_{1}}P_{0}\xrightarrow{\epsilon}M\to 0. It is easy to verify that Inf\operatorname{Inf} is an exact functor. Therefore, the sequence

Inf(P1)Inf(d1)Inf(P0)Inf(ϵ)Inf(M)0\dots\to\operatorname{Inf}(P_{1})\xrightarrow{\operatorname{Inf}(d_{1})}\operatorname{Inf}(P_{0})\xrightarrow{\operatorname{Inf}(\epsilon)}\operatorname{Inf}(M)\to 0

is exact. By Lemma 5.1, each Inf(Pi)\operatorname{Inf}(P_{i}) is a projective (GE)\mathbb{C}(G\wr\operatorname{E})-module.

By definition, the resolution 𝐏\mathbf{P}_{\bullet} is minimal if ϵ\epsilon is a projective cover and each dnd_{n} induces a projective cover Pnker(dn1)P_{n}\to\ker(d_{n-1}). By Lemma 5.5, inflation preserves the projective cover property. Thus, Inf(ϵ)\operatorname{Inf}(\epsilon) is the projective cover of Inf(M)\operatorname{Inf}(M) and each Inf(dn)\operatorname{Inf}(d_{n}) induces the projective cover of Inf(ker(dn1))ker(Inf(dn1))\operatorname{Inf}(\ker(d_{n-1}))\simeq\ker(\operatorname{Inf}(d_{n-1})). It follows that Inf(𝐏)\operatorname{Inf}(\mathbf{P}_{\bullet}) is a minimal projective resolution. ∎

Corollary 5.7.

The inflation functor preserves the projective dimension of modules. That is, for any E\mathbb{C}\operatorname{E}-module MM, we have

pdE(M)=pd(GE)(InfM).\operatorname{pd}_{\mathbb{C}\operatorname{E}}(M)=\operatorname{pd}_{\mathbb{C}(G\wr\operatorname{E})}(\operatorname{Inf}M).

5.3 The Global Dimension

Finally, we apply the preceding results to compute the global dimension of (GPTn)\mathbb{C}(G\wr\operatorname{PT}_{n}). Recall that En\operatorname{E}_{n} is the EI-category whose objects are the subsets of [n]={1,,n}[n]=\{1,\ldots,n\} and whose morphisms are onto functions. Since (GPTn)\mathbb{C}(G\wr\operatorname{PT}_{n}) is Morita equivalent to the category algebra (GEn)\mathbb{C}(G\wr\operatorname{E}_{n}), we may instead determine the global dimension of the latter.

Theorem 5.8.

The global dimension of the category algebra (GEn)\mathbb{C}(G\wr\operatorname{E}_{n}) is n1n-1.

Proof.

We first establish n1n-1 as an upper bound. The global dimension is bounded above by the length of the longest path in the quiver of the algebra. In Theorem 4.10, we characterized the vertices of the quiver as multi-Young diagrams. Specifically, we showed that if UU is a multi-Young diagram with kk boxes and VV is one with pp boxes, an arrow VUV\to U can only exist if p=k+1p=k+1. Furthermore, there are no arrows directed toward the vertex corresponding to a multipartition with 0 boxes (the ”bottom” element). Consequently, the longest directed path in the quiver has length n1n-1, which provides the required upper bound: glDim((GEn))n1\operatorname{glDim}(\mathbb{C}(G\wr\operatorname{E}_{n}))\leq n-1.

For the lower bound, we consider the En\mathbb{C}\operatorname{E}_{n}-simple module MM corresponding to the partition [2,1n2][2,1^{n-2}]. It was shown in [29, Corollary 6.9] that pdEn(M)=n1\operatorname{pd}_{\mathbb{C}\operatorname{E}_{n}}(M)=n-1. By Corollary 5.7, the inflation functor Inf\operatorname{Inf} preserves projective dimension, implying:

pd(GEn)(InfM)=pdEn(M)=n1.\operatorname{pd}_{\mathbb{C}(G\wr\operatorname{E}_{n})}(\operatorname{Inf}M)=\operatorname{pd}_{\mathbb{C}\operatorname{E}_{n}}(M)=n-1.

Since the global dimension of an algebra is the supremum of the projective dimensions of its simple modules, it follows that glDim((GEn))n1\operatorname{glDim}(\mathbb{C}(G\wr\operatorname{E}_{n}))\geq n-1. Combining these bounds, we conclude that the global dimension is exactly n1n-1. ∎

Corollary 5.9.

For every finite group GG, the global dimension of the monoid algebra (GPTn)\mathbb{C}(G\wr\operatorname{PT}_{n}) is n1n-1.

6 The quiver of the wreath product of a group with the monoid of all order-preserving partial functions

A partial function α:[n][n]\alpha\colon[n]\to[n] is called order-preserving if xyα(x)α(y)x\leq y\implies\alpha(x)\leq\alpha(y) for every x,yx,y in the domain of α\alpha. Let POn\operatorname{PO}_{n} be the submonoid of PTn\operatorname{PT}_{n} consisting of all order-preserving partial functions. In this section, we describe the quiver of the complex algebra (GPOn)\mathbb{C}(G\wr\operatorname{PO}_{n}).

In this case, the wreath product is

GPOn={(f,α)fPT([n],G),αPOn, and dom(α)=dom(f)}.G\wr\operatorname{PO}_{n}=\{(f,\alpha)\mid f\in\operatorname{PT}([n],G),\,\alpha\in\operatorname{PO}_{n},\text{ and }\operatorname{dom}(\alpha)=\operatorname{dom}(f)\}.

Recall the set of idempotents ={(1X,idX)X[n]}\mathcal{E}=\{(1_{X},\text{id}_{X})\mid X\subseteq[n]\}, which forms a subsemilattice of GPOnG\wr\operatorname{PO}_{n}. It is a straightforward consequence that GPOnG\wr\operatorname{PO}_{n} is an \mathcal{E}-Ehresmann and a right restriction monoid.

Let EOn\operatorname{EO}_{n} be the subcategory of the category En\operatorname{E}_{n}, defined in Section 4.1, which has the same set of objects but whose morphisms consist of surjective, total order-preserving functions. It follows that GEOnG\wr\operatorname{EO}_{n} is the Ehresmann category associated with GPOnG\wr\operatorname{PO}_{n}. Thus, by Theorem 4.2, we obtain an isomorphism of algebras

(GPOn)(GEOn).\mathbb{C}(G\wr\operatorname{PO}_{n})\simeq\mathbb{C}(G\wr\operatorname{EO}_{n}).

Following the approach in Section 4.2, we now consider the skeleton of GEOnG\wr\operatorname{EO}_{n}. If α:XY\alpha\colon X\to Y is an order-preserving bijection, then its inverse α1\alpha^{-1} is also order-preserving. Consequently, Lemma 4.4 implies that two objects XX and YY of GEOnG\wr\operatorname{EO}_{n} are isomorphic if and only if |X|=|Y||X|=|Y|. Let SEOn\operatorname{SEO}_{n} denote the category whose objects are [k][k] for 0kn0\leq k\leq n, and whose morphisms are surjective, total order-preserving functions. The skeleton of GEOnG\wr\operatorname{EO}_{n} is then the wreath product GSEOnG\wr\operatorname{SEO}_{n}. Our goal now is to describe the quiver of the algebra (GSEOn)\mathbb{C}(G\wr\operatorname{SEO}_{n}).

The endomorphism groups in GSEOnG\wr\operatorname{SEO}_{n} have a straightforward structure. Since the only order-preserving bijection from [k][k] to itself is the identity map, the endomorphism group of any object [k][k] in GSEOnG\wr\operatorname{SEO}_{n} is simply the direct product GkG^{k}.

By applying Theorem 4.5 to the skeletal category GSEOnG\wr\operatorname{SEO}_{n}, the set of vertices of QQ is the disjoint union of the simple modules of the endomorphism groups of the objects in the skeleton. Since the endomorphism group of the object [k][k] is isomorphic to GkG^{k}, the vertex set is:

k=0nIRep(Gk).\bigsqcup_{k=0}^{n}\operatorname{IRep}(G^{k}).

Any simple module of GkG^{k} is an outer tensor product of kk simple modules of GG. Thus, the vertices of the quiver are naturally indexed by sequences (V1,,Vk)(V_{1},\dots,V_{k}) of length 0kn0\leq k\leq n, where each ViIRep(G)V_{i}\in\operatorname{IRep}(G). So the vertex set is:

k=0n{V1VkViIRep(G)}.\bigsqcup_{k=0}^{n}\{V_{1}\boxtimes\dots\boxtimes V_{k}\mid V_{i}\in\operatorname{IRep}(G)\}.

For k=0k=0, the unique vertex is the trivial module of the trivial group G0G^{0}.

Our next step is to identify the irreducible morphisms in the category GSEOnG\wr\operatorname{SEO}_{n}.

Lemma 6.1.

The irreducible morphisms of GSEOnG\wr\operatorname{SEO}_{n} are precisely the morphisms from [k+1][k+1] to [k][k] for 0k<n0\leq k<n. That is,

Irr(GSEOn)([r],[k])={GSEOn([r],[k])if r=k+1,otherwise.\operatorname{Irr}(G\wr\operatorname{SEO}_{n})([r],[k])=\begin{cases}G\wr\operatorname{SEO}_{n}([r],[k])&\text{if }r=k+1,\\ \emptyset&\text{otherwise.}\end{cases}
Proof.

As in the proof of Lemma 4.6, any morphism from [k+1][k+1] to [k][k] is clearly irreducible because any factorization would force one of the factors to be an isomorphism. Conversely, suppose (f,α)GSEOn([r],[k])(f,\alpha)\in G\wr\operatorname{SEO}_{n}([r],[k]) with r>k+1r>k+1. Since α\alpha is a surjective order-preserving function, it is known that α\alpha factors as α=α1α2\alpha=\alpha_{1}\alpha_{2}, where α2:[r][k+1]\alpha_{2}\colon[r]\to[k+1] and α1:[k+1][k]\alpha_{1}\colon[k+1]\to[k] are both surjective order-preserving functions (see [26, Lemma 5.1]). We may then define the morphisms (𝟏[k+1],α1)(\mathbf{1}_{[k+1]},\alpha_{1}) and (f,α2)(f,\alpha_{2}). Since neither α1\alpha_{1} nor α2\alpha_{2} is a bijection, these factors are not invertible in GSEOnG\wr\operatorname{SEO}_{n}. Their product is

(𝟏[k+1],α1)(f,α2)=(𝟏[k+1]α2f,α1α2)=(f,α),(\mathbf{1}_{[k+1]},\alpha_{1})\cdot(f,\alpha_{2})=(\mathbf{1}_{[k+1]}\ast\alpha_{2}\cdot f,\alpha_{1}\alpha_{2})=(f,\alpha),

which shows that (f,α)(f,\alpha) is not irreducible. ∎

Let VIRep(Gp)V\in\operatorname{IRep}(G^{p}) and UIRep(Gk)U\in\operatorname{IRep}(G^{k}) be vertices of the quiver. If pk+1p\neq k+1, there are no arrows in the quiver of (GSEOn)\mathbb{C}(G\wr\operatorname{SEO}_{n}) from VV to UU because Irr(GSEOn)([p],[k])\operatorname{Irr}(G\wr\operatorname{SEO}_{n})([p],[k]) is empty. Consequently, we focus on the case p=k+1p=k+1 and examine the structure of [Irr(GSEOn)([k+1],[k])]\mathbb{C}[\operatorname{Irr}(G\wr\operatorname{SEO}_{n})([k+1],[k])] as a (Gk×Gk+1)(G^{k}\times G^{k+1})-module, with the action defined in Theorem 4.5.

A morphism in Irr(GSEOn)([k+1],[k])\operatorname{Irr}(G\wr\operatorname{SEO}_{n})([k+1],[k]) is a pair (f,α)(f,\alpha), where α:[k+1][k]\alpha\colon[k+1]\to[k] is a surjective order-preserving function and f:[k+1]Gf\colon[k+1]\to G. It is easy to see that there are exactly kk surjective order-preserving maps from [k+1][k+1] to [k][k], denoted σ1,,σk\sigma_{1},\dots,\sigma_{k}. The map σi\sigma_{i} is defined by:

σi(j)={jif ji,j1if j>i.\sigma_{i}(j)=\begin{cases}j&\text{if }j\leq i,\\ j-1&\text{if }j>i.\end{cases}

so α=σi\alpha=\sigma_{i} for some ii. Set M=[Irr(GSEOn)([k+1],[k])]M=\mathbb{C}[\operatorname{Irr}(G\wr\operatorname{SEO}_{n})([k+1],[k])] and define

Mi=span{(f,σi)fG[k+1]}.M_{i}=\text{span}\{(f,\sigma_{i})\mid f\in G^{[k+1]}\}.

We naturally identify G[k]G^{[k]} with GkG^{k}.

Lemma 6.2.

The (Gk×Gk+1)(G^{k}\times G^{k+1})-module MM decomposes as a direct sum of kk submodules:

Mi=1kMi,M\cong\bigoplus_{i=1}^{k}M_{i},
Proof.

Since the set of all such pairs (f,α)(f,\alpha) forms a basis for MM, and since the MiM_{i} are disjoint except for the zero vector and their union spans MM, we can write MM as a direct sum of vector spaces

Mi=1kMi.M\cong\bigoplus_{i=1}^{k}M_{i}.

To show this is a decomposition of (Gk×Gk+1)(G^{k}\times G^{k+1})-modules, we examine the action defined in Theorem 4.5. For hGkh\in G^{k} and gGk+1g\in G^{k+1}, the action on a basis element (f,σi)(f,\sigma_{i}) is:

(h,g)(f,σi)=(h,id[k])(f,σi)(g,id[k+1])1.(h,g)\bullet(f,\sigma_{i})=(h,\text{id}_{[k]})\cdot(f,\sigma_{i})\cdot(g,\text{id}_{[k+1]})^{-1}.

Since (g,id[k+1])1=(g1,id[k+1])(g,\text{id}_{[k+1]})^{-1}=(g^{-1},\text{id}_{[k+1]}) and by calculating the product in the wreath product category:

(h,id[k])(f,σi)(g1,id[k+1])=((hσi)fg1,σi).(h,\text{id}_{[k]})\cdot(f,\sigma_{i})\cdot(g^{-1},\text{id}_{[k+1]})=((h\ast\sigma_{i})\cdot f\cdot g^{-1},\sigma_{i}).

Crucially, the underlying order-preserving map σi\sigma_{i} remains unchanged by the action of the endomorphism groups so each subspace MiM_{i} is a submodule of MM. ∎

For each 1ik1\leq i\leq k, let Xi={(f,σi)fG[k+1]}X_{i}=\{(f,\sigma_{i})\mid f\in G^{[k+1]}\} denote the natural basis for the subspace MiM_{i}. By Lemma 6.2, the action of Gk×Gk+1G^{k}\times G^{k+1} preserves MiM_{i} and maps basis elements to basis elements. Consequently, we can view MiM_{i} as the permutation module Xi\mathbb{C}X_{i} arising from the action of Gk×Gk+1G^{k}\times G^{k+1} on the set XiX_{i}. To analyze the structure of this permutation module, we first establish that this action is transitive.

Lemma 6.3.

For each 1ik1\leq i\leq k, the action of Gk×Gk+1G^{k}\times G^{k+1} on the set XiX_{i} is transitive.

Proof.

Let (𝟏[k+1],σi)(\mathbf{1}_{[k+1]},\sigma_{i}) be the element of XiX_{i} where 𝟏[k+1]\mathbf{1}_{[k+1]} is the constant function mapping every element of [k+1][k+1] to 1G1_{G}. For any arbitrary (f,σi)Xi(f,\sigma_{i})\in X_{i}, we choose (𝟏[k],f1)Gk×Gk+1(\mathbf{1}_{[k]},f^{-1})\in G^{k}\times G^{k+1}. Applying the action, we have:

(𝟏[k],f1)(𝟏[k+1],σi)\displaystyle(\mathbf{1}_{[k]},f^{-1})\bullet(\mathbf{1}_{[k+1]},\sigma_{i}) =(𝟏[k],id[k])(𝟏[k+1],σi)(f1,id[k+1])1\displaystyle=(\mathbf{1}_{[k]},\text{id}_{[k]})\cdot(\mathbf{1}_{[k+1]},\sigma_{i})\cdot(f^{-1},\text{id}_{[k+1]})^{-1}
=(𝟏[k],id[k])(𝟏[k+1],σi)(f,id[k+1])\displaystyle=(\mathbf{1}_{[k]},\text{id}_{[k]})\cdot(\mathbf{1}_{[k+1]},\sigma_{i})\cdot(f,\text{id}_{[k+1]})
=((𝟏[k]σi)𝟏[k+1]f,σi)\displaystyle=((\mathbf{1}_{[k]}\ast\sigma_{i})\cdot\mathbf{1}_{[k+1]}\cdot f,\sigma_{i})
=(𝟏[k+1]𝟏[k+1]f,σi)\displaystyle=(\mathbf{1}_{[k+1]}\cdot\mathbf{1}_{[k+1]}\cdot f,\sigma_{i})
=(f,σi).\displaystyle=(f,\sigma_{i}).

This shows that any element of XiX_{i} can be reached from (𝟏[k+1],σi)(\mathbf{1}_{[k+1]},\sigma_{i}), and thus the action is transitive. ∎

The transitivity of the action allows us to identify each MiM_{i} as a permutation module induced by the stabilizer of our chosen base point. Let KiK_{i} denote the stabilizer of (𝟏[k+1],σi)(\mathbf{1}_{[k+1]},\sigma_{i}) in Gk×Gk+1G^{k}\times G^{k+1}.

Lemma 6.4.

For each 1ik1\leq i\leq k, the stabilizer KiK_{i} of the element (𝟏[k+1],σi)(\mathbf{1}_{[k+1]},\sigma_{i}) is given by

Ki={(h,hσi)hGk}.K_{i}=\{(h,h\ast\sigma_{i})\mid h\in G^{k}\}.
Proof.

An element (h,g)Gk×Gk+1(h,g)\in G^{k}\times G^{k+1} belongs to KiK_{i} if and only if (h,g)(𝟏[k+1],σi)=(𝟏[k+1],σi)(h,g)\bullet(\mathbf{1}_{[k+1]},\sigma_{i})=(\mathbf{1}_{[k+1]},\sigma_{i}). This condition is satisfied if and only if:

((hσi)𝟏[k+1]g1,σi)=(𝟏[k+1],σi).((h\ast\sigma_{i})\cdot\mathbf{1}_{[k+1]}\cdot g^{-1},\sigma_{i})=(\mathbf{1}_{[k+1]},\sigma_{i}).

Equating the first components, we obtain the equation (hσi)g1=𝟏[k+1](h\ast\sigma_{i})\cdot g^{-1}=\mathbf{1}_{[k+1]}, which implies g=hσig=h\ast\sigma_{i}. ∎

In particular, the elements of KiK_{i} are in one-to-one correspondence with GkG^{k}. Note that if we write hGkh\in G^{k} as h=(h1,,hk)h=(h_{1},\dots,h_{k}), then

hσi=(h1,,hi,hi,hi+1,,hk)h\ast\sigma_{i}=(h_{1},\dots,h_{i},h_{i},h_{i+1},\dots,h_{k})

.

Since MiM_{i} is a transitive permutation module, we have the following isomorphism of (Gk×Gk+1)(G^{k}\times G^{k+1})-modules:

MiIndKiGk×Gk+1(trKi).M_{i}\cong\text{Ind}_{K_{i}}^{G^{k}\times G^{k+1}}(\operatorname{tr}_{K_{i}}).

For each 1ik1\leq i\leq k, we define a group monomorphism φi:GkGk+1\varphi_{i}\colon G^{k}\to G^{k+1} by φi(h)=hσi\varphi_{i}(h)=h\ast\sigma_{i}. Explicitly, for h=(h1,,hk)Gkh=(h_{1},\dots,h_{k})\in G^{k}, we have

φi(h1,,hk)=(h1,,hi,hi,hi+1,,hk).\varphi_{i}(h_{1},\dots,h_{k})=(h_{1},\dots,h_{i},h_{i},h_{i+1},\dots,h_{k}).

It is easy to verify that this is indeed a group monomorphism.

Proposition 6.5.

Let UIRep(Gk)U\in\operatorname{IRep}(G^{k}) and VIRep(Gk+1)V\in\operatorname{IRep}(G^{k+1}). For each 1ik1\leq i\leq k, the multiplicity of the simple (Gk×Gk+1)(G^{k}\times G^{k+1})-module UVU\boxtimes V^{*} in MiM_{i} is equal to the multiplicity of VV in the induced module IndGkGk+1(U)\text{Ind}_{G^{k}}^{G^{k+1}}(U), where the induction is taken along the group homomorphism φi:GkGk+1\varphi_{i}\colon G^{k}\to G^{k+1}. In terms of characters, this is expressed as:

UV,MiGk×Gk+1=V,IndGkGk+1UGk+1.\langle U\boxtimes V^{*},M_{i}\rangle_{G^{k}\times G^{k+1}}=\langle V,\operatorname{Ind}_{G^{k}}^{G^{k+1}}U\rangle_{G^{k+1}}.
Proof.

Using the character of the permutation module MiM_{i} as identified in Lemma 6.4:

UV,MiGk×Gk+1=UV,IndKiGk×Gk+1trKiGk×Gk+1.\langle U\boxtimes V^{*},M_{i}\rangle_{G^{k}\times G^{k+1}}=\langle U\boxtimes V^{*},\text{Ind}_{K_{i}}^{G^{k}\times G^{k+1}}\operatorname{tr}_{K_{i}}\rangle_{G^{k}\times G^{k+1}}.

Applying Frobenius reciprocity:

UV,IndKiGk×Gk+1trKiGk×Gk+1=ResKiGk×Gk+1(UV),trKiKi.\langle U\boxtimes V^{*},\text{Ind}_{K_{i}}^{G^{k}\times G^{k+1}}\operatorname{tr}_{K_{i}}\rangle_{G^{k}\times G^{k+1}}=\langle\text{Res}_{K_{i}}^{G^{k}\times G^{k+1}}(U\boxtimes V^{*}),\operatorname{tr}_{K_{i}}\rangle_{K_{i}}.

As a summation, we have:

ResKiGk×Gk+1(UV),trKiKi\displaystyle\langle\text{Res}_{K_{i}}^{G^{k}\times G^{k+1}}(U\boxtimes V^{*}),\operatorname{tr}_{K_{i}}\rangle_{K_{i}} =1|Gk|hGk(UV)(h,hσi)1\displaystyle=\frac{1}{|G^{k}|}\sum_{h\in G^{k}}(U\boxtimes V^{*})(h,h\ast\sigma_{i})\cdot 1
=1|Gk|hGk(U(h)V(hσi))\displaystyle=\frac{1}{|G^{k}|}\sum_{h\in G^{k}}(U(h)\cdot V^{*}(h\ast\sigma_{i}))
=1|Gk|hGk(U(h)V(hσi)¯)\displaystyle=\frac{1}{|G^{k}|}\sum_{h\in G^{k}}(U(h)\cdot\overline{V(h\ast\sigma_{i})})

Note that V(hσi)=ResGkGk+1V(h)V(h\ast\sigma_{i})=\operatorname{Res}_{G^{k}}^{G^{k+1}}V(h) where the restriction is taken along the homomorphism φi\varphi_{i}.

Therefore, the final expression becomes:

1|Gk|hGkU(h)ResGkGk+1V(h)¯=U,ResGkGk+1VGk.\frac{1}{|G^{k}|}\sum_{h\in G^{k}}U(h)\cdot\overline{\operatorname{Res}_{G^{k}}^{G^{k+1}}V(h)}=\langle U,\operatorname{Res}_{G^{k}}^{G^{k+1}}V\rangle_{G^{k}}.

Finally, applying Frobenius reciprocity again, we obtain:

U,ResGkGk+1VGk=IndGkGk+1U,VGk+1.\langle U,\operatorname{Res}_{G^{k}}^{G^{k+1}}V\rangle_{G^{k}}=\langle\operatorname{Ind}_{G^{k}}^{G^{k+1}}U,V\rangle_{G^{k+1}}.

This completes the proof. ∎

Clearly, since φi\varphi_{i} acts as the identity on all coordinates jij\neq i, investigating the induction from GkG^{k} to Gk+1G^{k+1} along φi\varphi_{i} reduces to understanding the induction from GG to G×GG\times G along the diagonal homomorphism d(g)=(g,g)d(g)=(g,g).

Lemma 6.6.

Let U1,U2,U3IRep(G)U_{1},U_{2},U_{3}\in\operatorname{IRep}(G). The multiplicity of U1U2U_{1}\boxtimes U_{2} in the induced module IndGG×GU3\operatorname{Ind}_{G}^{G\times G}U_{3} is equal to the multiplicity of U3U_{3} in the tensor product U1U2U_{1}\otimes U_{2} as a GG-module.

Proof.

By Frobenius reciprocity for the group pair (G,G×G)(G,G\times G), we have:

IndGG×GU3,U1U2G×G=U3,ResGG×G(U1U2)G.\langle\operatorname{Ind}_{G}^{G\times G}U_{3},U_{1}\boxtimes U_{2}\rangle_{G\times G}=\langle U_{3},\operatorname{Res}_{G}^{G\times G}(U_{1}\boxtimes U_{2})\rangle_{G}.

The restriction of the external tensor product U1U2U_{1}\boxtimes U_{2} to the diagonal subgroup is the internal tensor product U1U2U_{1}\otimes U_{2}. Substituting this into the inner product, we obtain:

U3,ResGG×G(U1U2)G=U3,U1U2G.\langle U_{3},\text{Res}_{G}^{G\times G}(U_{1}\boxtimes U_{2})\rangle_{G}=\langle U_{3},U_{1}\otimes U_{2}\rangle_{G}.

Lemma 6.7.

Let U=U1UkIRep(Gk)U=U_{1}\boxtimes\dots\boxtimes U_{k}\in\text{IRep}(G^{k}) and V=V1Vk+1IRep(Gk+1)V=V_{1}\boxtimes\dots\boxtimes V_{k+1}\in\text{IRep}(G^{k+1}). The multiplicity of UVU\boxtimes V^{*} in MiM_{i} is non-zero only if:

  • VrUrV_{r}\cong U_{r} for all r<ir<i,

  • VrUr1V_{r}\cong U_{r-1} for all r>i+1r>i+1.

In this case, the multiplicity is given by the multiplicity of UiU_{i} in the tensor product ViVi+1V_{i}\otimes V_{i+1}.

Proof.

From Proposition 6.5, we have:

Mi,UV=IndGkGk+1U,VGk+1.\langle M_{i},U\boxtimes V^{*}\rangle=\langle\operatorname{Ind}_{G^{k}}^{G^{k+1}}U,V\rangle_{G^{k+1}}.

Since the induction along φi\varphi_{i} is the identity on all components except the ii-th one, where it is the diagonal induction, we have:

IndGkGk+1UU1Ui1IndGG×G(Ui)Ui+1Uk.\operatorname{Ind}_{G^{k}}^{G^{k+1}}U\cong U_{1}\boxtimes\dots\boxtimes U_{i-1}\boxtimes\operatorname{Ind}_{G}^{G\times G}(U_{i})\boxtimes U_{i+1}\boxtimes\dots\boxtimes U_{k}.

Comparing this with V=V1Vk+1V=V_{1}\boxtimes\dots\boxtimes V_{k+1}, the result follows from Lemma 6.6. ∎

If we use the Kronecker delta notation:

δU,V={1if UV0otherwise\delta_{U,V}=\begin{cases}1&\text{if }U\cong V\\ 0&\text{otherwise}\end{cases}

then the multiplicity formula can be expressed compactly as:

Mi,UV=(r=1i1δUr,Vr)(r=i+1kδUr,Vr+1)Ui,ViVi+1G.\langle M_{i},U\boxtimes V^{*}\rangle=\left(\prod_{r=1}^{i-1}\delta_{U_{r},V_{r}}\right)\left(\prod_{r=i+1}^{k}\delta_{U_{r},V_{r+1}}\right)\langle U_{i},V_{i}\otimes V_{i+1}\rangle_{G}.

In order to obtain the number of arrows from VV to UU all is left is to sum this number over ii from 11 to kk. We can conclude:

Theorem 6.8.

The quiver QQ of the algebra (GSEOn)\mathbb{C}(G\wr\operatorname{SEO}_{n}) or, equivalently, (GPOn)\mathbb{C}(G\wr\operatorname{PO}_{n}) is constructed as follows:

  • Vertices: The set of vertices is the disjoint union k=0nIRep(Gk)\displaystyle\bigsqcup_{k=0}^{n}\operatorname{IRep}(G^{k}), where each vertex is a simple module of the form U=U1UkU=U_{1}\boxtimes\dots\boxtimes U_{k} with UrIRep(G)U_{r}\in\operatorname{IRep}(G).

  • Arrows: For any V=V1Vk+1IRep(Gk+1)V=V_{1}\boxtimes\dots\boxtimes V_{k+1}\in\operatorname{IRep}(G^{k+1}) and U=U1UkIRep(Gk)U=U_{1}\boxtimes\dots\boxtimes U_{k}\in\operatorname{IRep}(G^{k}), the number of arrows from VV to UU is given by the sum:

    i=1k(r=1i1δUr,Vr)(r=i+1kδUr,Vr+1)Ui,ViVi+1G,\sum_{i=1}^{k}\left(\prod_{r=1}^{i-1}\delta_{U_{r},V_{r}}\right)\left(\prod_{r=i+1}^{k}\delta_{U_{r},V_{r+1}}\right)\langle U_{i},V_{i}\otimes V_{i+1}\rangle_{G},

    where Ui,ViVi+1G\langle U_{i},V_{i}\otimes V_{i+1}\rangle_{G} is the multiplicity of UiU_{i} in the tensor product ViVi+1V_{i}\otimes V_{i+1} as a GG-module.

Example 6.9.

We illustrate Theorem 6.8 by constructing the quiver QQ of the algebra (C2PO3)\mathbb{C}(C_{2}\wr\operatorname{PO}_{3}). The group G=C2G=C_{2} has two simple modules: the trivial module tr\operatorname{tr} and the sign module sgn\operatorname{sgn}.

The tensor product rules for these modules are straightforward:

\otimes tr\operatorname{tr} sgn\operatorname{sgn}
tr\operatorname{tr} tr\operatorname{tr} sgn\operatorname{sgn}
sgn\operatorname{sgn} sgn\operatorname{sgn} tr\operatorname{tr}

The quiver is a bit crowded, and given by:

(sgn,tr,tr)(\operatorname{sgn},\operatorname{tr},\operatorname{tr})(sgn,tr,sgn)(\operatorname{sgn},\operatorname{tr},\operatorname{sgn})(sgn,sgn,tr)(\operatorname{sgn},\operatorname{sgn},\operatorname{tr})(sgn,sgn,sgn)(\operatorname{sgn},\operatorname{sgn},\operatorname{sgn})(tr,tr,tr)(\operatorname{tr},\operatorname{tr},\operatorname{tr})(tr,tr,sgn)(\operatorname{tr},\operatorname{tr},\operatorname{sgn})(tr,sgn,tr)(\operatorname{tr},\operatorname{sgn},\operatorname{tr})(tr,sgn,sgn)(\operatorname{tr},\operatorname{sgn},\operatorname{sgn})(tr,tr)(\operatorname{tr},\operatorname{tr})(tr,sgn)(\operatorname{tr},\operatorname{sgn})(sgn,tr)(\operatorname{sgn},\operatorname{tr})(sgn,sgn)(\operatorname{sgn},\operatorname{sgn})(tr)(\operatorname{tr})(sgn)(\operatorname{sgn})\emptyset

Note that a multiplicity of two between vertices is denoted by a double-lined arrow.

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