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2021

[2]\fnmTracy \surWeyand

1]\orgdivDepartment of Mathematics, \orgnameBaylor University, \orgaddress\street1410 S. 4th Street, \cityWaco, \postcode76706, \stateTX, \countryUSA

[2]\orgdivDepartment of Mathematics, \orgnameRose-Hulman Institute of Technology, \orgaddress\street5500 Wabash Avenue, \cityTerre Haute, \postcode47803, \stateIN, \countryUSA

Can One Hear the Spanning Trees of a Quantum Graph?

\fnmJonathan \surHarrison jon_harrison@baylor.edu    weyand@rose-hulman.edu [ *
Abstract

Kirchhoff showed that the number of spanning trees of a graph is the spectral determinant of the combinatorial Laplacian divided by the number of vertices; we reframe this result in the quantum graph setting. We prove that the spectral determinant of the Laplace operator on a finite connected metric graph with standard (Neummann-Kirchhoff) vertex conditions determines the number of spanning trees when the lengths of the edges of the metric graph are sufficiently close together. To obtain this result, we analyze an equilateral quantum graph whose spectrum is closely related to spectra of discrete graph operators and then use the continuity of the spectral determinant under perturbations of the edge lengths.

keywords:
quantum graphs, spectral determinant, zeta functions, spanning trees
pacs:
[

MSC Classification]81Q10, 81Q35, 05C05, 34B45

1 Introduction

The question “Can one hear the shape of a quantum graph?” was answered in the affirmative by Gutkin and Smilansky GS01 for a quantum graph where the set of edge lengths are incommensurate. Their work was inspired by the famous question of Kac Kac66 which also sowed the seeds of results on isospectral billiards Cha95 ; GWW92 , graphs BPB09 and Riemannian manifolds Sun85 , along with many other related works. The connection between these questions is the extent to which properties of the spectrum can be used to recover information on the system’s geometry.

Isospectral domains were also studied in the context of discrete graphs Bro99 . In graph theory, a historic spectral geometric connection is provided by a theorem of Kirchhoff Kirchhoff . Kirchhoff’s matrix tree theorem expresses the number of spanning trees of a connected graph in terms of the spectral determinant of the combinatorial Laplacian of the graph which is the matrix 𝐋=𝐃𝐀\mathbf{L}=\mathbf{D}-\mathbf{A} where 𝐃\mathbf{D} is a diagonal matrix of the vertex degrees and 𝐀\mathbf{A} is the adjacency matrix, see section 2.

Theorem 1 (Kirchhoff’s Matrix Tree Theorem).

For a connected graph GG with VV vertices,

# spanning trees =1Vdet(𝐋)=det(𝐋[i])\#\mbox{ spanning trees }=\dfrac{1}{V}{\det}^{\prime}(\mathbf{L})=\det(\mathbf{L}[i]) (1)

for any i=1,2,,Vi=1,2,\ldots,V where 𝐋[i]\mathbf{L}[i] is the matrix 𝐋\mathbf{L} with row ii and column ii removed.

In this article we reframe Kirchhoff’s theorem in the setting of quantum graphs. Quantum graphs were introduced to model electrons in organic molecules Pau36 and are widely employed in mathematical physics as a model of quantum mechanics in systems with complex geometry, see BKbook ; Kuc03 for a review. In a quantum graph the edges of the graph consist of intervals connected at the vertices with a self-adjoint differential operator on the set of intervals. Here we consider the most widely studied case of the Laplace operator with Neumann-Kirchhoff (or standard) vertex conditions, denoted \mathcal{L}. For Neumann-Kirchhoff conditions, functions on the graph are continuous and outgoing derivatives at the vertices sum to zero. We obtain the following relationship between the spectral determinant of \mathcal{L} and the number of spanning trees of the graph.

Theorem 2.

Let Γ\mathit{\Gamma} be a connected metric graph with edge lengths in the interval [,+δ)[\ell,\ell+\delta) and \mathcal{L} the Laplacian with Neumann-Kirchoff vertex conditions. If

δ<VV 2E+V2EV,\delta<\frac{\ell}{V^{V}\,2^{E+V}\sqrt{2EV}}\ , (2)

then the number of spanning trees is the closest integer to

TΓ=v𝒱dvE 2Eβ+1det(),T_{\mathit{\Gamma}}=\dfrac{\prod_{v\in\mathcal{V}}d_{v}}{E\,2^{E}\,\ell^{\beta+1}}{\det}^{\prime}(\mathcal{L})\ , (3)

where 𝒱\mathcal{V} is the set of vertices, dvd_{v} is the degree of vertex vv, EE is the number of edges and β\beta is the first Betti number of Γ\mathit{\Gamma}.

If we have an equilateral quantum graph Γ~\widetilde{\mathit{\Gamma}} where all the edge lengths are \ell, then TΓ~T_{\widetilde{\mathit{\Gamma}}} is precisely the number of spanning trees. We use ~\widetilde{\mathcal{L}} to denote the Laplace operator of an equilateral quantum graph.

Theorem 3.

Let Γ~\widetilde{\mathit{\Gamma}} be a connected equilateral metric graph with edge length \ell and ~\widetilde{\mathcal{L}} the Laplacian with Neumann-Kirchoff vertex conditions. Then,

# spanning trees =v𝒱dvE 2Eβ+1det(~),\#\mbox{ spanning trees }=\dfrac{\prod_{v\in\mathcal{V}}d_{v}}{E\,2^{E}\,\ell^{\beta+1}}{\det}^{\prime}(\widetilde{\mathcal{L}}), (4)

where 𝒱\mathcal{V} is the set of vertices, dvd_{v} is the degree of vertex vv, EE is the number of edges and β\beta is the first Betti number of Γ~\widetilde{\mathit{\Gamma}}.

In the formula for TΓT_{\Gamma} (3), the number of edges EE can be determined from the spectrum of \mathcal{L} via the Weyl law, where the mean spacing of the eigenvalues is given by π1ele\pi^{-1}\sum_{e\in\mathcal{E}}l_{e}, see BKbook , as the edge lengths are tightly constrained to [,+δ)[\ell,\ell+\delta). For a connected graph Γ\Gamma, the first Betti number is determined by the number of edges and vertices, β=EV+1\beta=E-V+1. Hence, it would be interesting to know if there are also spectral interpretations of the number of vertices and the product of the degrees in (3).

The article is organised as follows. In section 2 we introduce discrete graph and metric graph notation and operators. We relate the spectral determinants of equilateral quantum graphs and discrete graph operators in section 3. In section 4 we use Kirchoff’s matrix tree theorem and the relationship between spectral determinants to prove theorem 3. In section 5 we compare spectral determinants of equilateral and non-equilateral quantum graphs and in section 6 we prove theorem 2. Finally we summarize the results in section 7.

2 Background

A discrete graph GG is comprised of a set of vertices 𝒱\mathcal{V} and a set of edges \mathcal{E} such that each edge connects a pair of vertices; see for example Figure 1. Two vertices u,v𝒱u,v\in\mathcal{V} are adjacent if (u,v)(u,v)\in\mathcal{E} and we write uvu\sim v. We will denote the number of vertices by V=|𝒱|V=\lvert\mathcal{V}\rvert and the number of edges by E=||E=\lvert\mathcal{E}\rvert. The degree of a vertex vv, denoted dvd_{v}, is the number of vertices that are adjacent to vv. We let v\mathcal{E}_{v} denote the set of edges containing the vertex vv so dv=|v|d_{v}=\lvert\mathcal{E}_{v}\rvert. If dv=dd_{v}=d for all v𝒱v\in\mathcal{V}, the graph is regular. In this paper, we only consider simple graphs where there are no loops or multiple edges and the number of edges and vertices are finite. We also assume that GG is connected, so there is a path between every pair of vertices. The distance between a pair of vertices u,v𝒱u,v\in\mathcal{V} on a connected discrete graph is the number of edges in a shortest path joining uu and vv. The diameter DD of the graph is the maximum distance between a pair of vertices. The first Betti number of GG is β=EV+1\beta=E-V+1, the number of independent cycles on GG. A tree is a connected graph with no cycles, β=0\beta=0. A spanning tree of GG is a subgraph of GG that is a tree and contains all the vertices of GG.

Figure 1: The complete bipartite graph K2,4K_{2,4}.

A function on a discrete graph GG takes values at the vertices and therefore can be viewed as a vector fVf\in\mathbb{C}^{V}. The combinatorial Laplace operator, 𝐋\mathbf{L}, is defined by

(𝐋f)(v)=dvf(v)uvf(u).(\mathbf{L}f)(v)=d_{v}f(v)-\sum_{u\sim v}f(u). (5)

This means that we can define the self-adjoint V×VV\times V matrix 𝐋\mathbf{L} where

𝐋uv={duif u=v1if uv0otherwise.\mathbf{L}_{uv}=\begin{cases}d_{u}&\text{if }u=v\\ -1&\text{if }u\sim v\\ 0&\text{otherwise}\end{cases}\ . (6)

We note that 𝐋\mathbf{L} has zero as an eigenvalue (with multiplicity one for a connected graph), and we will index the eigenvalues of 𝐋\mathbf{L} in increasing order,

0=μ1<μ2μ3μV.0=\mu_{1}<\mu_{2}\leq\mu_{3}\leq\ldots\leq\mu_{V}. (7)

The harmonic Laplacian is

𝚫=𝐃1𝐋\mathbf{\Delta}=\mathbf{D}^{-1}\mathbf{L} (8)

where 𝐃\mathbf{D} is a diagonal matrix of the degrees, 𝐃uv=dvδuv\mathbf{D}_{uv}=d_{v}\delta_{uv}. We denote the eigenvalues of 𝚫\mathbf{\Delta} with λj\lambda_{j} for j=1,,Vj=1,\dots,V.

A metric graph Γ\mathit{\Gamma} is a discrete graph where every edge ee\in\mathcal{E} is assigned a length e>0\ell_{e}>0. We associate the edge ee with the interval [0,e][0,\ell_{e}]. For e=(u,v)e=(u,v), we set xe=0x_{e}=0 at uu and xe=ex_{e}=\ell_{e} at vv; the choice of orientation of the coordinate is arbitrary and will not affect the results. The total length of a metric graph is the sum of the lengths of each edge, tot=ee\ell_{\mathrm{tot}}=\sum_{e\in\mathcal{E}}\ell_{e}. An equilateral metric graph Γ~\widetilde{\mathit{\Gamma}} is a metric graph where all the edge lengths are equal. We will use the term generic metric graph to distinguish a non-equilateral graph. A function ff on Γ\mathit{\Gamma} is a collection of functions {fe}e\{f_{e}\}_{e\in\mathcal{E}} where fef_{e} is a function on the interval [0,e][0,\ell_{e}].

A quantum graph is a metric graph Γ\mathit{\Gamma} along with a self-adjoint differential operator. In this paper, we consider the Laplace operator, denoted by \mathcal{L}, which acts as d2dxe2-\frac{\mathrm{d}^{2}}{\mathrm{d}x_{e}^{2}} on functions defined on [0,e][0,\ell_{e}]. We will use the notation ~\widetilde{\mathcal{L}} if Γ~\widetilde{\mathit{\Gamma}} is an equilateral metric graph. At the vertices, functions will satisfy the Neumann-Kirchhoff (or standard) vertex conditions,

{f(x) is continuous on Γ and evdfedxe(v)=0 at each vertex v.\left\{\begin{array}[]{l}f(x)\mbox{ is continuous on }\mathit{\Gamma}\mbox{ and }\\ \displaystyle\sum_{e\in\mathcal{E}_{v}}\dfrac{\mathrm{d}f_{e}}{\mathrm{d}x_{e}}(v)=0\mbox{ at each vertex }v\end{array}\right.\ . (9)

By convention, dfedxe(v)\dfrac{\mathrm{d}f_{e}}{\mathrm{d}x_{e}}(v) is taken to be the outgoing derivative at the end of the interval [0,e][0,\ell_{e}] corresponding to vv. The second Sobolev space on Γ\mathit{\Gamma} is the direct sum of the second Sobolev spaces on the set of intervals,

H2(Γ)=eH2([0,e]).H^{2}(\mathit{\Gamma})=\bigoplus_{e\in\mathcal{E}}H^{2}([0,\ell_{e}]). (10)

The domain of \mathcal{L} is the set of functions fH2(Γ)f\in H^{2}(\mathit{\Gamma}) that satisfy (9). With these vertex conditions, \mathcal{L} has an infinite number of non-negative eigenvalues BKbook which we will denote as

0k12k220\leq k_{1}^{2}\leq k_{2}^{2}\leq\ldots (11)

with kjk_{j}\in\mathbb{R}.

Some of these eigenvalues may correspond to eigenfunctions where fe(0)=fe(e)=0f_{e}(0)=f_{e}(\ell_{e})=0 for all ee\in\mathcal{E}. In this case the eigenfunction is also an eigenfunction of the Laplacian with Dirichlet vertex conditions. The spectrum of the graph with Dirichlet vertex conditions is just the union of the spectra of the Laplacian on EE disconnected intervals [0,e][0,\ell_{e}] with Dirichlet boundary conditions. We call this the Dirichlet spectrum of Γ\mathit{\Gamma}.

3 Spectral determinants of equilateral graphs

In this section we relate the spectral determinants of 𝚫\mathbf{\Delta} and ~\widetilde{\mathcal{L}}. This is used in section 4 to prove theorem 3. The spectral determinant of the harmonic Laplacian 𝚫\mathbf{\Delta} is the product of its nonzero eigenvalues,

det(𝚫)=j=1Vλj.{\det}^{\prime}(\mathbf{\Delta})={\prod_{j=1}^{V}}^{\prime}\lambda_{j}\ . (12)

The prime shows that eigenvalues of zero are omitted from the product. Correspondingly, the spectral determinant of the Laplace operator ~\widetilde{\mathcal{L}} on an equilateral metric graph is, formally,

det(~)=j=1kj2.{\det}^{\prime}(\widetilde{\mathcal{L}})={\prod_{j=1}^{\infty}}^{\prime}k^{2}_{j}\,. (13)

The spectral determinant of quantum graphs has been studied in a number of situations Des00 ; Des01 ; Fri06 ; HarKir11 ; HarKirTex12 . Here we use a zeta function regularization of the product. The spectral zeta function, 𝒵(s)\mathcal{Z}(s), is a generalization of the Riemann zeta function where the nonzero eigenvalues take the place of the integers. The spectral zeta function corresponding to ~\widetilde{\mathcal{L}} is

𝒵(s)=j=1kj2s,\mathcal{Z}(s)=\sum_{j=1}^{\infty}k_{j}^{-2s}, (14)

which converges for Re(s)>1\operatorname{Re}(s)>1. Making an analytic continuation to the left of Re(s)=1\operatorname{Re}(s)=1, the regularized spectral determinant is defined as

det(~)=exp(𝒵(0)).{\det}^{\prime}(\widetilde{\mathcal{L}})=\mbox{exp}(-\mathcal{Z}^{\prime}(0)). (15)

There is a correspondence between the eigenvalues of 𝚫\mathbf{\Delta} and ~\widetilde{\mathcal{L}} Below85 (see also Kuc03 ; Pank06 ; BKbook ).

Proposition 1.

Suppose GG is a discrete graph and Γ~\widetilde{\mathit{\Gamma}} is the corresponding equilateral metric graph with edge length \ell. If k2k^{2} is not in the Dirichlet spectrum of ~\widetilde{\mathcal{L}}, then

k2σ(~)1cos(k)σ(𝚫)k^{2}\in\sigma(\widetilde{\mathcal{L}})\iff 1-\cos(k\ell)\in\sigma(\mathbf{\Delta}) (16)

where σ()\sigma(\cdot) denotes the spectrum of the operator.

By proposition 1, every eigenvalue of 𝚫\mathbf{\Delta} can be written as 1cos(t)1-\cos(t\ell) for some t[0,π]t\in\left[0,\frac{\pi}{\ell}\right]. Let T={tj}j=1VT=\{t_{j}\}_{j=1}^{V} be the set 0=t1<t2tVπ0=t_{1}<t_{2}\leq\ldots\leq t_{V}\leq\frac{\pi}{\ell} such that 1cos(tj)σ(𝚫)1-\cos(t_{j}\ell)\in\sigma(\mathbf{\Delta}) (including multiplicity). We know 0=t1<t20=t_{1}<t_{2} as zero is an eigenvalue of 𝚫\mathbf{\Delta} with multiplicity one when GG is connected. This allows us to write the spectral zeta function of ~\widetilde{\mathcal{L}} in terms of the finite set TT. The following lemma is a combination of equations (20) and (24) from HarWey18 .

Lemma 1.

Suppose GG is a discrete graph and Γ~\widetilde{\mathit{\Gamma}} is the corresponding equilateral metric graph with edge length \ell. For Re(s)12\operatorname{Re}(s)\neq\frac{1}{2}, the spectral zeta function of ~\widetilde{\mathcal{L}} is

𝒵(s)\displaystyle\mathcal{Z}(s) =(4s(β1)+2)(2π)2sζR(2s)\displaystyle=\left(4^{s}(\beta-1)+2\right)\left(\frac{\ell}{2\pi}\right)^{2s}\zeta_{R}(2s)
+(2π)2sj=2V(ζH(2s,tj2π)+ζH(2s,1tj2π))\displaystyle+\left(\dfrac{\ell}{2\pi}\right)^{2s}\sum_{j=2}^{V}\left(\zeta_{H}\left(2s,\frac{t_{j}\ell}{2\pi}\right)+\zeta_{H}\left(2s,1-\frac{t_{j}\ell}{2\pi}\right)\right) (17)

where ζR(z)\zeta_{R}(z) is the Riemann zeta function, ζH(z,a)\zeta_{H}(z,a) is the Hurwitz zeta function, and tjTt_{j}\in T.

Using lemma 1 we can obtain a relationship between the spectral determinants of the harmonic Laplacian of a discrete graph and the Laplacian of the corresponding equilateral quantum graph.

Proposition 2.

Suppose GG is a connected discrete graph and Γ~\widetilde{\mathit{\Gamma}} is the corresponding equilateral metric graph with edge length \ell. Then

det(~)=2E1β+1det(𝚫).{\det}^{\prime}(\widetilde{\mathcal{L}})=2^{E-1}\ell^{\beta+1}{\det}^{\prime}(\mathbf{\Delta})\ . (18)

Proof:

Since ζH(0,a)=12a\zeta_{H}(0,a)=\frac{1}{2}-a NITS , it follows that,

ζH(0,a)+ζH(0,1a)=0.\zeta_{H}(0,a)+\zeta_{H}(0,1-a)=0\ . (19)

Using lemma 1,

𝒵(0)=ln(2β1)ln(β+1)+2j=2V[ln(Γ(tj2π)Γ(1tj2π))ln2π]\mathcal{Z}^{\prime}(0)=-\ln\left(2^{\beta-1}\right)-\ln(\ell^{\beta+1})+2\sum_{j=2}^{V}\left[\ln\left(\Gamma\left(\frac{t_{j}\ell}{2\pi}\right)\Gamma\left(1-\frac{t_{j}\ell}{2\pi}\right)\right)-\ln{2\pi}\right]\\ (20)

since ζR(0)=1/2\zeta_{R}(0)=-1/2, ζR(0)=ln(2π)/2\zeta^{\prime}_{R}(0)=-\ln(2\pi)/2, and ζH(0,a)=ln(Γ(a))12ln(2π)\zeta^{\prime}_{H}(0,a)=\ln(\Gamma(a))-\frac{1}{2}\ln(2\pi) NITS . Additionally Γ(z)Γ(1z)=π/sin(πz)\Gamma(z)\Gamma(1-z)=\pi/\sin(\pi z) NITS and 4sin2(tj2)=2(1cos(tj))=2λj4\sin^{2}\left(\frac{t_{j}\ell}{2}\right)=2(1-\cos(t_{j}\ell))=2\lambda_{j}, so

𝒵(0)\displaystyle-\mathcal{Z}^{\prime}(0) =ln(2β1)+ln(β+1)+j=2Vln(4sin2(tj2))\displaystyle=\ln\left(2^{\beta-1}\right)+\ln(\ell^{\beta+1})+\sum_{j=2}^{V}\ln\left(4\sin^{2}\left(\frac{t_{j}\ell}{2}\right)\right) (21)
=ln(2V+β2β+1j=2Vλj).\displaystyle=\ln\left(2^{V+\beta-2}\ell^{\beta+1}\prod_{j=2}^{V}\lambda_{j}\right). (22)

Taking the exponential of this expression yields the result.

3.1 Example: complete bipartite graphs

Proposition 2 simplifies for complete bipartite graphs. The complete bipartite graph, Km,pK_{m,p}, consists of m+pm+p vertices and mpmp edges. The vertices can be divided into two disjoint sets, \mathcal{M} of size mm and 𝒫\mathcal{P} of size pp, such that every vertex in \mathcal{M} is connected to every vertex in 𝒫\mathcal{P} and no vertex is connected to another vertex from the same set; see for example Figure 1. A star graph is a complete bipartite graph with m=1m=1 and p=V1=Ep=V-1=E.

Corollary 1.

For an equilateral complete bipartite graph Km,pK_{m,p} with edge length \ell,

det(~)=2mpmpmp+2.{\det}^{\prime}(\widetilde{\mathcal{L}})=2^{mp}\ell^{mp-m-p+2}. (23)

In particular, for a star graph,

det(~)=2E.{\det}^{\prime}(\widetilde{\mathcal{L}})=2^{E}\ell. (24)

Proof: The eigenvalues of a discrete complete bipartite graph Km,pK_{m,p} are 0 with multiplicity one, 11 with multiplicity m+p2m+p-2, and 22 with multiplicity one Chungbook , and therefore

det(𝚫)=2.{\det}^{\prime}(\mathbf{\Delta})=2. (25)

The complete bipartite graph Km,pK_{m,p} has β=EV+1=mp(m+p)+1\beta=E-V+1=mp-(m+p)+1. Substituting into proposition 2 produces the result. The case of a star graph is obtained by setting m=1m=1 and p=V1=Ep=V-1=E.

Corollary 1 agrees with HarWey18 where the spectral determinant was obtained from the quantum spectral zeta function directly. The star graph formula (24) agrees with HarKir11 where the spectral zeta functions of quantum star graphs were calculated using a contour integral approach.

4 Spanning trees of equilateral graphs

Kirchhoff’s matrix tree theorem Kirchhoff gives the number of spanning trees of a discrete graph in terms of the spectral determinant of the combinatorial Laplacian. In this section we prove theorem 3 which reframes this result in terms of the spectral determinant of an equilateral quantum graph.

4.1 Regular equilateral graphs

We start by proving theorem 3 for a dd-regular graph where the proof is straightforward.

Proposition 3.

Suppose Γ~\widetilde{\mathit{\Gamma}} is a connected dd-regular equilateral metric graph with edge length \ell. Then

# spanning trees =dV12E1β+1Vdet(~).\#\mbox{ spanning trees }=\dfrac{d^{V-1}}{2^{E-1}\ell^{\beta+1}V}{\det}^{\prime}(\widetilde{\mathcal{L}}). (26)

Proof: Since Γ~\widetilde{\mathit{\Gamma}} is a dd-regular graph,

𝚫=𝐃1𝐋=1d𝐋.\mathbf{\Delta}=\mathbf{D}^{-1}\mathbf{L}=\dfrac{1}{d}\mathbf{L}. (27)

If μ\mu is an eigenvalue of 𝐋\mathbf{L}, then μ/d\mu/d is an eigenvalue of 𝚫\mathbf{\Delta} so

det(𝚫)=i=2Vμid=d1Vdet(𝐋).{\det}^{\prime}(\mathbf{\Delta})=\prod_{i=2}^{V}\dfrac{\mu_{i}}{d}=d^{1-V}{\det}^{\prime}(\mathbf{L}). (28)

By Kirchhoff’s matrix tree theorem,

# spanning trees =dV1Vdet(𝚫).\#\mbox{ spanning trees }=\dfrac{d^{V-1}}{V}\mbox{det}^{\prime}(\mathbf{\Delta}). (29)

Combining equation (29) with proposition 2 produces the result.

4.2 General equilateral graphs

Theorem 3 follows from proposition 2 and the next lemma, which is an adaptation of a theorem by Chung and Yau ChYa and generalizes equation (29).

Lemma 2.

For a connected discrete graph GG,

# spanning trees =v𝒱dv2Edet(𝚫).\#\mbox{ spanning trees }=\dfrac{\prod_{v\in\mathcal{V}}d_{v}}{2E}{\det}^{\prime}(\mathbf{\Delta}). (30)

Proof: Since 𝚫\mathbf{\Delta} has one eigenvalue of zero, its characteristic polynomial is

p(x)=det(𝚫x𝐈)=xi=2V(λix).p(x)=\det(\mathbf{\Delta}-x\mathbf{I})=-x\prod_{i=2}^{V}(\lambda_{i}-x)\ . (31)

Therefore the coefficient of the linear term in p(x)p(x) is

i=2Vλi=det(𝚫).-\prod_{i=2}^{V}\lambda_{i}=-{\det}^{\prime}(\mathbf{\Delta}). (32)

On the other hand, since 𝚫=𝐃1𝐋\mathbf{\Delta}=\mathbf{D}^{-1}{\mathbf{L}},

𝚫x𝐈=𝐃1(𝐋x𝐃),\mathbf{\Delta}-x\mathbf{I}=\mathbf{D}^{-1}(\mathbf{L}-x\mathbf{D}), (33)

and the characteristic polynomial can also be written as

p(x)=(v𝒱dv)1det(𝐋x𝐃).p(x)=\left(\prod_{v\in\mathcal{V}}d_{v}\right)^{-1}\det(\mathbf{L}-x\mathbf{D}). (34)

Determinants are linear along the rows of a matrix so

det(𝐀+𝐁)=S[n]det𝐁S\det(\mathbf{A}+\mathbf{B})=\sum_{S\subseteq[n]}\det\mathbf{B}_{S} (35)

where 𝐀\mathbf{A} and 𝐁\mathbf{B} are square matrices of size nn, [n]={1,2,,n}[n]=\{1,2,\ldots,n\}, and 𝐁S\mathbf{B}_{S} is the matrix 𝐁\mathbf{B} whose rows that are indexed by SS are replaced with the corresponding rows from 𝐀\mathbf{A}. Hence,

det(𝐋x𝐃)\displaystyle\det(\mathbf{L}-x\mathbf{D}) =det(𝐋)+S[V]|S|=V1det(x𝐃S)+S[V]|S|=V2det(x𝐃S)++det(x𝐃)\displaystyle=\det(\mathbf{L})+\sum_{\begin{subarray}{c}S\subset[V]\\ \lvert S\rvert=V-1\\ \end{subarray}}\det(x\mathbf{D}_{S})+\sum_{\begin{subarray}{c}S\subset[V]\\ \lvert S\rvert=V-2\end{subarray}}\det(x\mathbf{D}_{S})+\ldots+\det(x\mathbf{D}) (36)
=det(𝐋)xi=1Vdidet(𝐋[i])+c2x2++cnxn\displaystyle=\det(\mathbf{L})-x\sum_{i=1}^{V}d_{i}\det(\mathbf{L}[i])+c_{2}x^{2}+\ldots+c_{n}x^{n} (37)

where 𝐋[i]\mathbf{L}[i] is the matrix 𝐋\mathbf{L} with both row ii and column ii removed. By theorem 1, det(𝐋[i])\det(\mathbf{L}[i]) is the number of spanning trees of GG. Therefore, we can see that

det(𝚫)=v𝒱dvv𝒱dv×# spanning trees ,{\det}^{\prime}(\mathbf{\Delta})=\dfrac{\sum_{v\in\mathcal{V}}d_{v}}{\prod_{v\in\mathcal{V}}d_{v}}\times\#\mbox{ spanning trees }\,, (38)

which proves the lemma as v𝒱dv=2E\sum_{v\in\mathcal{V}}d_{v}=2E.

We have now established theorem 3. So, for example, a star graph has β=0\beta=0 and one vertex has degree EE while the others have degree 11. Then, using the spectral determinant of an equilateral star graph (corollary 1), we see

# spanning trees =v𝒱dvE2Eβ+12E=1\#\mbox{ spanning trees }=\dfrac{\prod_{v\in\mathcal{V}}d_{v}}{E2^{E}\ell^{\beta+1}}2^{E}\ell=1 (39)

as required.

5 Spectral determinants of generic quantum graphs

In this section we compare the spectral determinants of equilateral and generic quantum graphs where the corresponding discrete graphs are the same. In particular, given an equilateral graph Γ~\widetilde{\mathit{\Gamma}} with edge length \ell, we will consider a generic graph whose edge lengths lie in the interval [,+δ)[\ell,\ell+\delta). Friedlander computed the spectral determinant of a generic quantum graph Fri06 .

Theorem 4.

Suppose Γ\mathit{\Gamma} is a connected metric graph. Then

det()=2EtotVeev𝒱dvdet(𝐑){\det}^{\prime}(\mathcal{L})=\frac{2^{E}\ell_{\mathrm{tot}}}{V}\frac{\prod_{e\in\mathcal{E}}\ell_{e}}{\prod_{v\in\mathcal{V}}d_{v}}{\det}^{\prime}(\mathbf{R}) (40)

where 𝐑\mathbf{R} is the V×VV\times V matrix defined by

𝐑uv={wv(w,v)1if u=v(u,v)1if uv0otherwise.\mathbf{R}_{uv}=\begin{cases}\sum_{w\sim v}\ell_{(w,v)}^{-1}&\text{if }u=v\\ -\ell_{(u,v)}^{-1}&\text{if }u\sim v\\ 0&\text{otherwise}\end{cases}\ . (41)

First, we note that the proof of lemma 2 also showed

det(𝐋)=Vv𝒱dv2Edet(𝚫).{\det}^{\prime}(\mathbf{L})=\frac{V\prod_{v\in\mathcal{V}}d_{v}}{2E}{\det}^{\prime}(\mathbf{\Delta})\ . (42)

In the case of an equilateral graph with edge length \ell, we will define 𝐑~=1𝐋\widetilde{\mathbf{R}}=\ell^{-1}\mathbf{L}, which agrees with (41) when e=\ell_{e}=\ell for every edge ee. In fact, setting the edge lengths equal in theorem 4,

det()|le=\displaystyle{\det}^{\prime}(\mathcal{L})\rvert_{l_{e}=\ell} =2EEEV+2Vv𝒱dvdet(𝐋)\displaystyle=\frac{2^{E}E\ell^{E-V+2}}{V\prod_{v\in\mathcal{V}}d_{v}}{\det}^{\prime}(\mathbf{L}) (43)
=2E1β+1det(𝚫)\displaystyle=2^{E-1}\ell^{\beta+1}{\det}^{\prime}(\mathbf{\Delta}) (44)
=det(~),\displaystyle={\det}^{\prime}(\widetilde{\mathcal{L}})\ , (45)

where we used proposition 2 for the last step. This demonstrates that evaluating (40) with equal edge lengths produces the spectral determinant of the equilateral graph as expected.

5.1 Bound on the spectral norm of R~R\widetilde{R}-R

Let e=+δe\ell_{e}=\ell+\delta_{e} where δe[0,δ)\delta_{e}\in[0,\delta). Then |1e1|<δ2\lvert\ell^{-1}-\ell_{e}^{-1}\rvert<\delta\ell^{-2}. To bound the spectral norm ||𝐑~𝐑||2\lvert\lvert\widetilde{\mathbf{R}}-\mathbf{R}\rvert\rvert_{2}, we use the fact that ||𝐀||2ij|𝐀ij|2\lvert\lvert\mathbf{A}\rvert\rvert_{2}\leq\sqrt{\sum_{ij}\lvert\mathbf{A}_{ij}\rvert^{2}} for a matrix 𝐀\mathbf{A}. From (41),

𝐑~uv𝐑uv={ruδ(r,u)(+δ(r,u))if u=vδ(u,v)(+δ(u,v))if uv0otherwise.\widetilde{\mathbf{R}}_{uv}-\mathbf{R}_{uv}=\begin{cases}\sum_{r\sim u}\frac{\delta_{(r,u)}}{(\ell+\delta_{(r,u)})\ell}&\text{if }u=v\\ -\frac{\delta_{(u,v)}}{(\ell+\delta_{(u,v)})\ell}&\text{if }u\sim v\\ 0&\text{otherwise}\end{cases}\ . (46)

Hence by Bergström’s inequality,

v|𝐑~uv𝐑uv|2\displaystyle\sum_{v}\lvert\widetilde{\mathbf{R}}_{uv}-\mathbf{R}_{uv}\rvert^{2} =(ruδ(r,u)(+δ(r,u)))2+uv(δ(u,v)(+δ(u,v)))2\displaystyle=\left(\sum_{r\sim u}\frac{\delta_{(r,u)}}{(\ell+\delta_{(r,u)})\ell}\right)^{2}+\sum_{u\sim v}\left(\frac{\delta_{(u,v)}}{(\ell+\delta_{(u,v)})\ell}\right)^{2} (47)
<(du+1)uvδ24.\displaystyle<(d_{u}+1)\sum_{u\sim v}\delta^{2}\ell^{-4}\ . (48)

From this we see,

||𝐑~𝐑||2<δ2E(dmax+1)2<δ2EV2,\lvert\lvert\widetilde{\mathbf{R}}-\mathbf{R}\rvert\rvert_{2}<\frac{\delta\sqrt{2E(d_{\textrm{max}}+1)}}{\ell^{2}}<\frac{\delta\sqrt{2EV}}{\ell^{2}}\ , (49)

where dmaxd_{\textrm{max}} is the maximum degree of any vertex.

Consequently, if the eigenvalues of 𝐑\mathbf{R} are 0=λ1<λ2<<λV0=\lambda_{1}<\lambda_{2}<\dots<\lambda_{V} and the eigenvalues of 𝐑~\widetilde{\mathbf{R}} are 0=λ~1<λ~2<<λ~V0=\tilde{\lambda}_{1}<\tilde{\lambda}_{2}<\dots<\tilde{\lambda}_{V} then,

|λ~jλj|<||𝐑~𝐑||2<δ2EV2.\lvert\tilde{\lambda}_{j}-\lambda_{j}\rvert<\lvert\lvert\widetilde{\mathbf{R}}-\mathbf{R}\rvert\rvert_{2}<\frac{\delta\sqrt{2EV}}{\ell^{2}}\ . (50)

5.2 A bound on the change in a spectral determinant

Given a set of real numbers 0<a<α1α2αn0<a<\alpha_{1}\leq\alpha_{2}\leq\dots\leq\alpha_{n},

j=1n(αj+a)j=1nαj\displaystyle\prod_{j=1}^{n}(\alpha_{j}+a)-\prod_{j=1}^{n}\alpha_{j}
=an+an1i=1nαi+an2i1i2αi1αi2++ai1,,in1:ijikαi1αiV1\displaystyle=a^{n}+a^{n-1}\sum_{i=1}^{n}\alpha_{i}+a^{n-2}\sum_{i_{1}\neq i_{2}}\alpha_{i_{1}}\alpha_{i_{2}}+\dots+a\sum_{\begin{subarray}{c}i_{1},\dots,i_{n-1}:\\ i_{j}\neq i_{k}\end{subarray}}\alpha_{i_{1}}\dots\alpha_{i_{V-1}} (51)
<a(i=2nαi)(j=0n1(nj))\displaystyle<a\left(\prod_{i=2}^{n}\alpha_{i}\right)\left(\sum_{j=0}^{n-1}{n\choose j}\right) (52)
<a2n(i=2nαi).\displaystyle<a2^{n}\left(\prod_{i=2}^{n}\alpha_{i}\right)\ . (53)

Now we compare the spectral determinants of 𝐑\mathbf{R} and 𝐑~\widetilde{\mathbf{R}}. From (50), we know that the difference between the corresponding eigenvalues of 𝐑\mathbf{R} and 𝐑~\widetilde{\mathbf{R}} is at most

a=δ2EV2.a=\frac{\delta\sqrt{2EV}}{\ell^{2}}. (54)

In our situation, we have 0=λ1<a<λ2λ3λV0={\lambda}_{1}<a<{\lambda}_{2}\leq{\lambda}_{3}\leq\ldots\leq{\lambda}_{V} (assuming that δ\delta is small enough so that a<λ2a<{\lambda}_{2}). Then from (53),

|det(𝐑)det(𝐑~)|<δ2V12EV2λ2det(𝐑).\lvert{\det}^{\prime}(\mathbf{R})-{\det}^{\prime}(\widetilde{\mathbf{R}})\rvert<\frac{\delta 2^{V-1}\sqrt{2EV}}{\ell^{2}{\lambda}_{2}}{\det}^{\prime}(\mathbf{R})\ . (55)

6 Spanning trees of generic quantum graphs

For a generic quantum graph Γ\mathit{\Gamma} with edge lengths in [,+δ)[\ell,\ell+\delta), let

TΓ=v𝒱dvE 2Eβ+1det().T_{\mathit{\Gamma}}=\dfrac{\prod_{v\in\mathcal{V}}d_{v}}{E\,2^{E}\,\ell^{\beta+1}}{\det}^{\prime}(\mathcal{L})\ . (56)

Notice that, by theorem 3, TΓ~T_{\widetilde{\mathit{\Gamma}}} is the number of spanning trees of an equilateral graph. For δ\delta sufficiently small, the value of TΓT_{\mathit{\Gamma}} will be close enough to TΓ~T_{\widetilde{\mathit{\Gamma}}} to determine the number of spanning trees of a generic quantum graph. Using theorem 4,

TΓ=toteeEVβ+1det(𝐑),T_{\mathit{\Gamma}}=\frac{\ell_{\mathrm{tot}}\prod_{e\in\mathcal{E}}\ell_{e}}{EV\ell^{\beta+1}}{\det}^{\prime}(\mathbf{R})\ , (57)

and similarly,

TΓ~=EβVdet(𝐑~).T_{\widetilde{\mathit{\Gamma}}}=\frac{\ell^{E-\beta}}{V}{\det}^{\prime}(\widetilde{\mathbf{R}})\ . (58)

We will determine a bound on δ\delta such that |TΓTΓ~|<1/2|T_{\mathit{\Gamma}}-T_{\widetilde{\mathit{\Gamma}}}\rvert<1/2, and hence the number of spanning trees is the closest integer to TΓT_{\mathit{\Gamma}}. To this end, we employ two bounds on the spectrum of 𝐋\mathbf{L}. The first is a lower bound on the second smallest eigenvalue in terms of the graph diameter DD, the maximum distance between a pair of vertices, due to McKay Moh91 .

Theorem 5.

The second smallest eigenvalue of 𝐋\mathbf{L} is bounded below, μ24DV\mu_{2}\geq\dfrac{4}{DV}.

The second is an upper bound on the eigenvalues of 𝐋\mathbf{L} , see Kel67 ; AndMor ; Mer94 .

Theorem 6.

The eigenvalues of 𝐋\mathbf{L} are bounded above, λjV\lambda_{j}\leq V for j=1,,Vj=1,\dots,V.

Proof: [Proof of Theorem 2] From equations (57) and (58),

|TΓTΓ~|toteeEVβ+1|det(𝐑)det(𝐑~)|+|det(𝐑~)|V|toteeEβ+1Eβ|.\lvert T_{\mathit{\Gamma}}-T_{\widetilde{\mathit{\Gamma}}}\rvert\leq\frac{\ell_{\mathrm{tot}}\prod_{e\in\mathcal{E}}\ell_{e}}{EV\ell^{\beta+1}}\lvert{\det}^{\prime}(\mathbf{R})-{\det}^{\prime}(\widetilde{\mathbf{R}})\rvert+\frac{\lvert{{\det}^{\prime}(\widetilde{\mathbf{R}})}\rvert}{V}\left\lvert\frac{\ell_{\mathrm{tot}}\prod_{e\in\mathcal{E}}\ell_{e}}{E\ell^{\beta+1}}-\ell^{E-\beta}\right\rvert. (59)

Using (55) and assuming that δ<\delta<\ell,

|TΓTΓ~|<(2)E+1Vβ+12V12EVδ|det(𝐑~)|2λ~2+|det(𝐑~)|Vβ+1|(+δ)E+1E+1|.\lvert T_{\mathit{\Gamma}}-T_{\widetilde{\mathit{\Gamma}}}\rvert<\frac{(2\ell)^{E+1}}{V\ell^{\beta+1}}\frac{2^{V-1}\sqrt{2EV}\delta\lvert{\det}^{\prime}(\widetilde{\mathbf{R}})\rvert}{\ell^{2}\tilde{\lambda}_{2}}+\frac{\lvert{{\det}^{\prime}(\widetilde{\mathbf{R}})}\rvert}{V\ell^{\beta+1}}\left\lvert(\ell+\delta)^{E+1}-\ell^{E+1}\right\rvert. (60)

Using (53), we can see that

|(+δ)E+1E+1|<δ2E+1E.\lvert(\ell+\delta)^{E+1}-\ell^{E+1}\rvert<\delta 2^{E+1}\ell^{E}\ . (61)

Consequently,

|TΓTΓ~|<δ|det(𝐋)|2E+1V[2V12EVλ~2+1]\lvert T_{\mathit{\Gamma}}-T_{\widetilde{\mathit{\Gamma}}}\rvert<\delta\lvert{\det}^{\prime}(\mathbf{L})\rvert\frac{2^{E+1}}{\ell V}\left[\frac{2^{V-1}\sqrt{2EV}}{\ell\tilde{\lambda}_{2}}+1\right] (62)

since det(𝐑~)=(V1)det(𝐋){\det}^{\prime}(\widetilde{\mathbf{R}})=\ell^{-(V-1)}{\det}^{\prime}(\mathbf{L}).

We can conclude from theorem 5 that λ~2>4/V2\tilde{\lambda}_{2}>4/V^{2}\ell, and we know by applying theorem 6 that det(𝐋)VV1{\det}^{\prime}(\mathbf{L})\leq V^{V-1}. Using these inequalities we see that

|TΓTΓ~|<δVV2 2E+1[V22V32EV+1]<δVV 2E+V12EV,\lvert T_{\mathit{\Gamma}}-T_{\widetilde{\mathit{\Gamma}}}\rvert<\frac{\delta}{\ell}V^{V-2}\,2^{E+1}\left[V^{2}2^{V-3}\sqrt{2EV}+1\right]<\frac{\delta}{\ell}V^{V}\,2^{E+V-1}\sqrt{2EV}, (63)

which establishes theorem 2.

6.1 Star graph example

For comparison, we write an equivalent bound in the case of the star graph where there are explicit formulae for the spectral determinants of the equilateral and generic quantum graphs. From HarKir11 ,

det()=2EEee,{\det}^{\prime}(\mathcal{L})=\frac{2^{E}}{E}\sum_{e\in\mathcal{E}}\ell_{e}\ , (64)

which agrees with the spectral determinant of the equilateral graph, corollary 1. For e[,+δ)\ell_{e}\in[\ell,\ell+\delta),

|det(~)det()|<2Eδ.\lvert{\det}^{\prime}(\widetilde{\mathcal{L}})-{\det}^{\prime}(\mathcal{L})\rvert<2^{E}\delta\ . (65)

Hence,

|TΓTΓ~|<δ.\lvert T_{\mathit{\Gamma}}-T_{\widetilde{\mathit{\Gamma}}}\rvert<\frac{\delta}{\ell}\ . (66)

Therefore, the closest integer to TΓT_{\mathit{\Gamma}} is the number of spanning trees if δ/2\delta\leq\ell/2.

If we have a star graph, then E=V1E=V-1 and the condition on δ\delta from theorem 2 is

δ<VV 22V12V(V1).\delta<\frac{\ell}{V^{V}\,2^{2V-1}\sqrt{2V(V-1)}}\ . (67)

Clearly, the demand on the edge lengths in theorem 2 is suboptimal so, in fact, one may expect that the nearest integer to TΓT_{\mathit{\Gamma}} gives the number of spanning trees even when the edge lengths are less tightly constrained.

7 Discussion

In this paper, we proved an analog of Kirchhoff’s matrix tree theorem for quantum graphs. In particular, we determined the number of spanning trees of an equilateral quantum graph from its spectral determinant. To do this we related the spectral determinant of an equilateral quantum graph to the spectral determinant of the harmonic Laplacian of the corresponding discrete graph. We extended this to non-equilateral quantum graphs where the edge lengths are sufficiently constrained.

The bound on the permitted variance in the edge lengths in theorem 2 is suboptimal but requires minimal information on the structure of the graph. However, the constraint may be loosened in some situations, even if there is no additional information about the graph’s structure. For example, all eigenvalues of 𝐋\mathbf{L} satisfy AndMor ,

λjmax(u,v)(du+dv).\lambda_{j}\leq\mbox{max}_{(u,v)\in\mathcal{E}}(d_{u}+d_{v})\ . (68)

As we assume in theorem 2 that we know the product of the vertex degrees, if we also know that max(u,v)(du+dv)<V\mbox{max}_{(u,v)\in\mathcal{E}}(d_{u}+d_{v})<V, then we can use (68) in place of theorem 6 which weakens the constraint on the spread of the edge lengths.

\bmhead

Acknowledgments

The authors would like to thank Gregory Berkolaiko for helpful comments. This work was partially supported by a grant from the Simons Foundation (354583 to Jonathan Harrison).

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