# Distances in spaces of physical models: partition functions versus spectra

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## Abstract

We study the relation between convergence of partition functions (seen as general Dirichlet series) and convergence of spectra and their multiplicities. We describe applications to convergence in physical models, e.g., related to topology change and averaging in cosmology.

## Keywords

Zeta function Partition function Riemannian manifold Spectrum Convergence Cosmological model## Mathematics Subject Classification

30B50 58C40 83F05## 1 Introduction

In this paper, we study the relation between closeness of spectra of operators and of spectral partition functions. Spectra of operators play a central role in physical theories, as outcomes of a physical measurement. As motivation for our problem, we provide two examples where questions about closeness of spectra of operators (as describing specific physical models) come up naturally in cosmology.

The first one arises in connection with the averaging problem in cosmology (compare [4, 18]) and the question of topology change under evolution of the universe. It is clear that spectra contain topological information, cf. e.g., [14]. How to make mathematical sense (in terms of spectra) of such statements as “the universe is homogeneous *on average*”, or “a sudden change of topology in the universe (e.g., from orientable to non-orientable) is unlikely?”.

Seriu [17] proposes to use eigenvalues of the Laplace–Beltrami operator on spatial sections of a cosmological model to construct a metric on the space of such Riemannian manifolds up to some notion of “large scale isospectrality”. He argues that the use of the plain difference of spectra as a measure is flawed: large energy contributions (corresponding to small-scale geometry) should carry a lower weight, and the dominant weight should be put on the small spectrum (corresponding to large-scale geometry). Therefore, he introduces a cut-off *N* and introduces a metric that compares the first *N* eigenvalues. Second, the eigenvalue difference is not a dimensionless quantity, and because of this, he suggests comparing quotients of spectra. However, as \(N \rightarrow +\infty \), the distance he proposes diverges.

We argue in this paper that it is natural not to use a cut-off function, but to rather use a distance *between the zeta functions* (which, like partition functions, give more weight to low energy in their region of convergence), considered as complex functions; here, one may use classical notions of distance between complex functions [6] used in the study of limits of holomorphic or meromorphic functions. Also, the zeta functions are dimensionless. We explain this in Sect. 2.

The second set of examples relates to the use of eigenvalues as dynamical variables in gravity. Gravity coupled to matter can be given a spectral description using the framework of noncommutative geometry [5]. Even by ignoring the matter part, one arrives at an interesting description of classical gravity (general relativity) in terms of spectral data. These spectra form a diffeomorphism-invariant set of coordinates on the space of manifolds, up to isospectrality. Diffeomorphism invariant coordinates are an important prerequisite for certain programmes to quantize gravity (although ’t Hooft [19] has argued that “deterministic quantum mechanics” might require a preferred coordinate frame that becomes irrelevant by information loss). In this way, spectra were used as dynamical variables for classical gravity by Landi and Rovelli [12]; see also [1].

The distance above (and its generalizations) provides a topology on the space of partition functions and it is a natural question to study the meaning of convergence of partition functions of models in terms of the spectrum itself. This is exactly what we study more abstractly: our Theorem 3.2 shows that it is a certain \(\ell ^1\)-convergence of sequences of (suitable powers of) the eigenvalues. The same problem makes sense for generalized Dirichlet series/partition functions, and in the final sections of the paper, we study this problem from various perspectives, including via the Laplace-Stieltjes transform. At the end of Sect. 4, we give an example of how to describe convergence of eigen*functions* in terms of convergence of certain spectral zeta functions.

Finally, we remark that in recent years, Bayesian inference has been applied successfully to the comparison of cosmological models [11]. For example, Niarchou and Jaffe [15] have used cosmic microwave background radiation measurements to study the most likely topology of the universe. In brief, the Bayesian method investigates, under certain hypotheses, which is the most likely of a finite list of cosmological models (in [15], five different topologies) to match observational data (in [15], WMAP data). By contrast, the spectral distance seems a more theoretical tool, that can show how a characteristic of a model (e.g., in [17], orientability) is stable or unstable by a small perturbation of the model. It seems this is related to the discussion on the final page of [15] on the nature of the primordial power spectrum, and whether it is possible to keep the spectrum identical at small scales (matching observations), but perturbed at large scales (changing topology). Whereas in the Bayesian paradigm, one weighs finitely many possible points in the space of all models, spectral distances relate to navigating continuously in the space of all models.

## 2 A spectral distance for cosmological models

As we explained in the introduction, it is useful to have a metric between cosmological models. We will describe our construction for closed Riemannian spatial sections of Lorentzian spacetimes (it will work equally well for Euclidean gravity models, but not for metric of general signature). To compare spatial sections, one needs a metric between Riemannian manifolds. If *X* is such a closed (= compact, no boundary) smooth Riemannian manifold with Laplace–Beltrami operator \(\Delta _X\) and non-zero spectrum \(\lambda _1 \le \lambda _2 \le \cdots \), its *spectral zeta function* is \(\zeta _X(s):= \mathrm {Tr}(\Delta _X^{-s}) = \sum _{\nu \ge 1} \lambda ^{-s}\). The spectral zeta function \(\zeta _X\) converges absolutely for \(\mathfrak {R}(s)>d/2\), where *d* is the dimension of *X* [16]. We propose the following function as a distance on suitable spaces of Riemannian geometries up to isospectrality:

### Proposition 2.1

### Proof

The function *d* is positive, and if \(d(X_1,X_2)=0\), then \(|\zeta _{X_1}(s)|=|\zeta _{X_2}(s)|\) for all *s* in the interval \(]\gamma ,\gamma +1[\). Since this set has accumulation points, and since the zeta function is positive real for such values of *s*, we find that \(\zeta _{X_1} = \zeta _{X_2}\) as complex functions. Hence, the identity theorem for Dirichlet series [10] implies that \(X_1\) and \(X_2\) are isospectral. The function *d* is symmetric, since \(\left| \log (x^{-1}) \right| = \left| \log (x) \right| \). Finally, the triangle inequality follows from \( {\zeta _{X_1}(s)}/{\zeta _{X_3}(s)} = {\zeta _{X_1}(s)/}{\zeta _{X_2}(s)} \cdot {\zeta _{X_2}(s)}/{\zeta _{X_3}(s)} \) and the usual properties of the absolute value. \(\square \)

This is a distance that weighs correctly the energy contributions (large-scale geometries contribute more), but does not depend on a cut-off in the spectrum, nor diverges if a cut-off tends to infinity.

### Remark 2.2

Taking the supremum over \(\gamma< s < \gamma +1\) is quite random: any set with an accumulation point and avoiding the poles of the zeta functions will do. Also, the distance *d* can be replaced by \(d/(1+d)\) to have it take values in the unit interval. The exact numerical values of the metric are not so relevant, but rather, their interrelation and the topology and uniformity that they induce.

### Example 2.3

If \(S_r\) denotes a circle of radius *r*, then \( d(S_{r_1}, S_{r_2}) = 4 \left| \log (r_1/r_2) \right| . \) This example shows that the distance can be non-differentiable in the parameter space of a family.

### Example 2.4

*S*and a real projective space \(\mathbf {R} \mathbf {P} ^2\) with the same volume \(4 \pi \); this example was considered in [17] to argue that topological change of spatial slices during cosmological evolution is not unlikely. The zeta functions are

### Remark 2.5

A distance between Riemannian manifolds *up to isometry* was constructed by the first author and de Jong, who have, furthermore, given a spectral characterization of when a diffeomorphism of closed, smooth Riemannian manifolds is an isometry, in terms of equality of more general zeta functions under pullback by the map [7]. Also, this distance is based on a dimensionless object (zeta functions). However, such distance is much more involved than the one above (it uses infinitely many zeta functions), and the one above suffices from the spectral point of view.

*strictly*increasing sequence of real numbers. Examples: if all coefficients \(a_{\nu }\) are one,

*D*(

*s*) is the partition function of a classical discrete canonical ensemble with total energy \(\mu _\nu \) in the \(\nu \)-th microstate for \(s=1/kT\) (

*T*temperature,

*k*Boltzmann constant); if all coefficients are integers,

*D*(

*s*) is the partition function of a discrete quantum system whose Hamiltonian has eigenvalues \(\mu _\nu \) with multiplicity \(a_{\nu }\) (or a classical system with degeneracies), etc.

In this paper, we study what this implies about “convergence” of the sequences \((a_{n,\nu })\) and \((\mu _{n,\nu })\). First, we consider the case of classical Dirichlet series, where \(a_*=1\) and \(\mu _* = \log \lambda _*\), and in Theorem 3.2, we prove that (1) is equivalent to the \(\ell ^1\)-convergence of \((\lambda ^\gamma _{n,\nu })\) to \((\lambda ^\gamma _{\nu })\), for any real \(\gamma \) strictly larger than the common abscissa of absolute convergence of the series \(D_n\). In Theorem 4.3, we consider the case where \(\mu _{n,\nu }=\mu _\nu \) is independent of *n*; then, for every *n*, \((a_{n,\nu })\) converges to \((a_n)\). The most general case is studied in Sect. 5 from the point of view of the Perron’s formula for Dirichlet series (where we give a concrete result under some hypotheses), and from the point of view of the Laplace–Stieltjes transform in Sect. 6, where we prove the equivalence to Lipschitz convergence of some step functions.

Specifically, if \(\{X_n\}_{n=1}^\infty \cup \{X\}\) is a sequence of connected, closed, smooth Riemannian manifolds such that \(d:=\sup \dim X_n\) is finite, convergence of their zeta functions implies convergence of their spectra in the sense of Theorem 3.2.

## 3 Convergence of Dirichlet series

### Notation 3.1

Let us, once and for all, introduce the following convenient notation: if \(s \in \mathbf {C}\) and \(\Lambda =(\lambda _\nu )_{\nu =1}^\infty \) is a sequence of positive real numbers, we denote by \(\Lambda ^s\) the sequence \((\lambda _\nu ^s)_{\nu =1}^\infty \).

### Theorem 3.2

*n*, \(\Lambda _n:=(\lambda _{n,\nu })_{\nu =1}^\infty \) forms a sequence of increasing positive real numbers with finite multiplicities. Assume that all series \(D_n(s)\) are convergent in a common right half-plane \(\mathfrak {R}(s)>\tilde{\gamma }>0\). Then, the following are equivalent:

- (i)
As \(n \rightarrow +\infty \), the functions \(D_n(s)\) converge to

*D*(*s*), pointwise in*s*with \(\mathfrak {R}(s)>\tilde{\gamma }\); - (ii)For every fixed \(\nu \), any bounded subsequence of \(\{\lambda _{n,\nu }\}_{n=1}^\infty \) converges to the same element \(\lambda \in \Lambda \), and$$\begin{aligned} \#\{ (\lambda _{n,\nu })_{n=1}^\infty : \lim _{n \rightarrow \infty }\lambda _{n,\nu }= \lambda \}= \#\{ \lambda _\nu : \lambda _\nu =\lambda \}. \end{aligned}$$
- (iii)
For some (equivalently, all) \(\gamma > \tilde{\gamma }\), \(\Lambda ^{-\gamma }_n\) converges to \(\Lambda ^{-\gamma }\) in \(\ell ^1\).

### Remark 3.3

The assumption that all series \(D_n(s)\) are convergent in a common right half-plane \(\mathfrak {R}(s)>\tilde{\gamma }\) is a minimal necessary assumption, since if this is not the case, the questions we ask are void.

*Proof of Theorem* 3.2 Since we later want to interchange some limits, we will first prove:

### Lemma 3.4

The sequences \(S_{n,N}(s):= \sum _{\nu =1}^N \lambda _{n,\nu }^{-s} \) converge to \(D_n(s)\) for \(N \rightarrow + \infty \) *uniformly in* *n*.

*Proof of Lemma*3.4 The uniform convergence means that

*does not depend on*

*n*.

*N*, independent of

*n*(compare also the proof on page 7 of [10]).

*s*real positive (hence for all

*s*by analytic continuation). In the above equation, we were allowed to interchange the order of the limits (in \(n_k\) and the summation variable of \(D_{n_k}\)) since the series converge uniformly in \(n_k\). Since we assume that \(D_n\) is a convergent sequence of functions, it has the same limit as its the subsequence \(D_{n_k}\).

*n*, for all \(\nu \), i.e., \( \forall n\in \mathbf {N}\;\; \lambda _{n,\nu } \le c_\nu . \) Then, we can select a subsequence so that for all \(\nu \), the limit \(\lim \nolimits _{k\rightarrow \infty } \lambda _{n_k,\nu }=\ell _\nu \) exists. Not to overload notation, we will momentarily relabel the convergent subsequence \(\lambda _{n_k,\nu }\) as \(\lambda _{n,\nu }\). In particular, \(\lambda _{n,1}\) converges to \(\ell _1\). We will prove that \(\lambda _{n,1}\) converges to \(\lambda _1\). Let us rewrite

*s*

*is an integer*\(s>\tilde{\gamma }\). Since \(D_n(s)\rightarrow D(s)\), we have that

*same*limit \(\lambda _{1}\). Therefore, \((\lambda _{n,1})_{n\in \mathbf {N}}\) itself is convergent to \(\lambda _1\). We conclude that in general (viz., before erasing all unbounded subsequences), every bounded subsequence of \((\lambda _n)_{n\in \mathbf {N}}\) converges to \(\lambda _1\).

We now use an inductive argument to treat the general term. Namely, consider the Dirichlet series \(D^{\ge 2}_n(s):=D_n(s) -\lambda _{n,1}^{-s}\) which (by what we have proven) converges to \(D^{\ge 2}(s):=D(s)-\lambda _1^{-s}.\) These are still sequences of Dirichlet series of the same form, but with first eigenvalues \(\lambda _{n,2}\) and \(\lambda _2\). We can repeat the argument with this series, to conclude \(\lambda _{n,2} \rightarrow \lambda _2\), etc. This finishes the proof that (i) implies (ii).

Since we assume that \(\mathfrak {R}(s)>\tilde{\gamma }\) is a common half-plane of convergence of all series \(D_n\) (\(n=\emptyset ,1,2,\ldots \)), for any \(\gamma >\tilde{\gamma }\), the sums \(\sum _{\nu =1}^\infty {\lambda _{n,\nu }^{-\gamma }}\) converge, and hence, the sequences \(\Lambda _n^{-\gamma }\) (\(n=\emptyset ,1,2,\ldots \)) belong to the Banach space \(\ell ^1\). We will now prove that \(\Lambda ^{-\gamma }_n\rightarrow \Lambda ^{-\gamma }\) as elements of \(\ell ^1\).

*n*(using the same \(\gamma \) for all

*n*), such that for \(N\ge n_0\)

This proves that (ii) implies (iii). Finally, if \(\Lambda _n^{-\gamma }\) converges to \(\Lambda ^{-\gamma }\) for some \(\gamma \in \mathbf {R} \), we have for every \(s \in \mathbf {C}\) with \(\mathfrak {R}(s)>\gamma \) that \(\Lambda _n^{-s}\) converges to \(\Lambda ^{-s}\), and it follows easily that \(D_n(s)\) converges to *D*(*s*), pointwise in *s*. This proves that (iii) implies (i) and finishes the proof of the theorem.

For an application to the meaning of convergence in the cosmological distance from the previous section, suppose that \(X=(X,g_X)\) and \(Y=(Y,g_Y)\) are two isospectral, connected, smooth, closed Riemannian manifolds, i.e., suppose their Laplace–Beltrami operators \(\Delta _X\) and \(\Delta _Y\) have the same spectrum with multiplicities: \(\Lambda _X=\Lambda _Y\) [16]. The spectrum \(\Lambda _X\) is considered as a sequence \((\lambda _\nu )_{\nu =1}^\infty \) with \(0 \le \lambda _1 \le \lambda _2 \le \ldots \), with finite repetitions.

The identity theorem for Dirichlet series [10] shows that such isospectrality can also be described as the manifolds having the same zeta function: \(\zeta _X = \zeta _Y\), where \( \zeta _{X}(s) := \mathrm {tr}(\Delta _X^{-s}) = \sum \nolimits _{0 \ne \lambda \in \Lambda _X} \lambda ^{-s}, \) since connectedness implies that the zero eigenvalue has multiplicity one. The function \(\zeta _X\) converges absolutely for \(\mathfrak {R}(s)>d/2\), where *d* is the dimension of *X* [16]. In this context, Theorem 3.2 says the following:

### Proposition 3.5

*X*is another closed, smooth, Riemannian manifold. Then, the following statements are equivalent:

- (i)
For \(\mathfrak {R}(s)>d/2\), the functions \(\zeta _{X_n}(s)\) converge pointwise to \(\zeta _X(s)\);

- (ii)
For some \(\gamma \in \mathbf {C}\) with \(Re(\gamma )>d/2\), the sequence of eigenvalues \(\Lambda ^{-\gamma }_{X_n}\) converges to \(\Lambda _X^{-\gamma }\) in \(\ell ^1\).

### Remark 3.6

If the manifolds are closed and smooth and *of odd dimension*, but possibly disconnected, the equality \(\zeta _X = \zeta _Y\) implies that also the multiplicity of the zero eigenvalue is equal for *X* and *Y*, namely, it is minus the value at 0 of the analytic continuation of \(\zeta _X\) ([16], 5.2).

The circle of radius *r* has \(\Delta =-r^2 \partial ^2_\theta \) (with \(\theta \in [0,2\pi )\) the angle coordinate), spectrum \(\lambda _{r,\nu } = r^{-2} \lceil \nu /2 \rceil ^2\) and zeta function \(\zeta _r(s)=r^{2s} \zeta (2s)\), where \(\zeta \) is the Riemann zeta function. For varying \(r \rightarrow r_0\), the convergence in the theorem happens for \(\gamma >1/2\).

*d*, the diameter

*D*, and a lower bound

*R*on the Ricci curvature of the manifolds under consideration. This implies that (at least if we fix the data

*d*,

*D*and

*R*, so we are in the Gromov precompact moduli space [9]) in unbounded subsequences, the volume should shrink to zero.

## 4 Series with general coefficients

In this section, we study what happens if we have pointwise convergence of general Dirichlet series in the sense of Eq. (1).

The previous case occurs when \(\{\mu _*\} = \{\log \lambda _*\}\) and \(a_*\) counts the multiplicities in \((\lambda _*)\). We start by discussing two special cases.

### 4.1

(Taylor series) The case appears when \(\mu _{n,\nu }= \nu \) for all \(n=\emptyset ,1,2,\ldots \). In this case, we set \(z=e^{-s}\) and we get a (pointwise) convergence of Taylor series \( D_n(z) = \sum \nolimits _{\nu \ge 0} a_{n,\nu } z^\nu \rightarrow D(z) = \sum \nolimits _{\nu \ge 0} a_{\nu } z^\nu . \) In this case, the individual series \(D_*\) converge in \(\Omega :=\{z>e^{-\gamma }\}\) to a holomorphic function (by assumption). Evaluation at zero gives \(\lim \nolimits _{n \rightarrow + \infty } a_{n,0} = a_0\), and we can proceed by induction to conclude that \(\lim \nolimits _{n \rightarrow + \infty } a_{n,\nu } = a_\nu \) for all \(\nu \).

*K*is a compact set. For a contour \(C \subset K\) around \(z=0\) (independent of

*n*), we have

### 4.2

(Constant exponents) The reason for providing this second proof is that it leads us to the next special case, in which we use the analogue of the integral representation for the coefficients for general Dirichlet series, also called Perron’s formula. This formula gives a representation of the terms of a general Dirichlet series by integration over a vertical line in the complex plane, and since this integration domain, unlike the contour in the Taylor series proof, is not compact, we will need to work more to establish the result (or assume uniform convergence on an entire half-line, which seems too strong an assumption). This second special case occurs if \(\mu _{n,\nu }\) is constant in *n*. Then we have the following result:

### Theorem 4.3

Assume that \(D_n\) (\(n=\emptyset ,1,2,\ldots \)) is a set of Dirichlet series that converge absolutely in a common half-plane \(\mathfrak {R}(s)>\tilde{\gamma }\), and such that \(D_n(s) \rightarrow D(s)\) converges pointwise there. Assume that \(\mu _{n,\nu }=\mu _\nu \) is independent of *n*. Then, for every *n*, we have \(\lim \nolimits _{n \rightarrow + \infty } a_{n,\nu } = a_\nu ;\) actually, for \(\sigma _1>\gamma \), we have a convergence of sequences \( (a_{n,\nu } e^{-\sigma _1 \mu _\nu })_{\nu =1}^\infty \rightarrow (a_\nu e^{-\sigma _1 \mu _\nu })_{\nu =1}^\infty \text{ in } \ell ^{\infty }. \)

### Proof

*n*and every fixed \(\nu \):

*D*on the entire line \(\mathfrak {R}(s)=\sigma _1\). However, we can avoid this (strong) hypothesis by proving the following lemma: \(\square \)

### Lemma 4.4

*Proof of Lemma*4.4 Since the series \(D_n\) are absolutely convergent on a common half-plane, their sequences of tails tend to zero uniformly in

*n*, that is, for every \(\epsilon >0\), there is an

*N*, that is independent of

*n*, such that

*N*terms on a vertical line \(\mathfrak {R}(s)=\sigma _1\). Consider the function

*f*: \(\mathbf {R} \rightarrow \left( S^1\right) ^{N}\) given by \( t\mapsto (e^{i t \mu _{1}}, \ldots , e^{i t \mu _{N}}) \) and the function

*F*: \(\left( S^1\right) ^{N} \rightarrow \mathbf {C} \) sending \( (P_1,\ldots , P_N) \mapsto \sum _{\nu =1}^N e^{-\sigma _1 \mu _\nu } P_\nu . \) The function

*F*is continuous on a compact set; therefore, it attains a maximal value

*M*at a point \(A^0:=(P_1^0,\ldots , P_N^0)\).

### Lemma 4.5

There exists \(t_0 \in \mathbf {R}\) such that all the numbers \(\{t_0 \mu _\nu \}_{\nu =1}^\infty \) are irrational.

### Proof

The set of multiples \(\{ b \rho \}\) of a given real number \(\rho \in \mathbf {R}\) such that \(b\rho \in \mathbf {Q}\) is just \(\frac{1}{\rho } \mathbf {Q}\) and this set is denumerable. A denumerable union of denumerable sets cannot exhaust the set of reals and the result follows. \(\square \)

*F*is continuous,

*M*is the maximum, for all \(t\in \mathbf {R}\), we have

### 4.6

*functions*from a spectral convergence, following a method introduced in [7], 2.5–2.7. Let

*X*denote a closed, smooth, Riemannian manifold and let \(a \in C^{\infty }(X)\) denote a smooth function. Define a generalized Dirichlet series by \( \zeta _{X,a}:=\mathrm {tr}(a\Delta _X^{-s}), \) cf. [7]. Then,

*X*and a family \(\{g_r\}\) (\(r \in \mathbf {R} \)) of isospectral metrics with simple eigenvalues on

*X*(cf. Gordon and Wilson [8] for the existence of such families). Denote by \(\Psi _{r,\lambda }\) the normalized real eigenfunction for the metric \(g_r\) corresponding to the eigenvalue \(\lambda \). If all zeta functions converge in the sense that

*a*, then we find from the above result that \(\int a \Psi ^2_{r,\lambda } d\mu _r \rightarrow \int a \Psi ^2_{0,\lambda } d\mu _0 \) for all functions \(a \in C^\infty (X)\), where \(\mu _r\) is the measure belonging to the metric \(g_r\), so a weak convergence of measures \( \Psi ^2_{r,\lambda } d\mu _r \rightarrow \Psi ^2_{0,\lambda } d\mu _0.\) Taking residues at \(\dim (X)/2\) in (9) for \(a=1\), we find that the volume of \((X,g_r)\) is constant in

*r*, and then taking residues for general

*a*, we find that for all \(a \in C^\infty (X)\), \( \int a d\mu _r \rightarrow \int a d\mu _0\): there is a weak convergence of measures \(\mu _r \rightarrow \mu _0\). Hence, we have a (pointwise) convergence of squared eigenfunctions: \(\Psi ^2_{r,\lambda } \rightarrow \Psi ^2_{0,\lambda }\).

## 5 General case

Finally, in the most general case of varying coefficients *and* varying exponents, we prove a theorem about accumulation points. First, we do some preparation.

### Definition 5.1

*g*, define for a real function

*f*, the

*g*-sup norm as

*converges multiplicatively*to a real function

*f*if there exists a strictly positive real function

*g*that is integrable with respect to the multiplicative Haar measure on \(\mathbf {R} ^*\) (i.e., such that \(\int _{\mathbf {R} } g(x)\frac{dx}{|x|}<+\infty \)), such that \(|| f_n(x) - f(x) ||_{\infty ,g} \rightarrow 0\) for \(n \rightarrow + \infty \).

### Definition 5.2

*f*, a complex function defined for \(\mathfrak {R}(s)=c\), and \(x \in \mathbf {R} \), denote by

*x*equals \(\mu _n\).

Since \(I^c_x(D)\) does not depend on *c* once it satisfies the conditions for Perron’s formula, we will now write \(I_x(D)\) for \(I^c_x(D)\) with any suitable *c*.

### Lemma 5.3

*t*, then for all \(x \in \mathbf {R} \),

### Proof

*n*sufficiently large. This proves the desired result. \(\square \)

Before stating the main result of this section, we need to introduce some notation:

### Notation 5.4

Write \(\mu _{n,j} = \log \lambda _{n,j}\), and assume that all sequences \((\lambda _{n,j})_{n=1}^\infty \) are bounded. Let \( \ell _i^{(j)}\), \(i\in I_j\) be the accumulation points of sequence \((\lambda _{n,j})_{n=1}^\infty \).

We consider a subsequence \(n_k\) such that for all *j* \( \lim \nolimits _{n_k\rightarrow \infty }\lambda _{n_k,j}=\ell _{i_j}^{(j)}\) for a selection \(i_j \in I_j\). Notice that the sequences \((\lambda _{n_k,j})_{k=1}^\infty \) and \((\lambda _{n_k,j+1})_{k=1}^\infty \) satisfy \(\lambda _{n_k,j} < \lambda _{n_k,j+1}\), but they can tend to the same accumulation point.

### Theorem 5.5

We use the notation of (5.4). Assume that \(D_n\) converges multiplicatively to \(D(s)=\sum _{j \ge 1} a_j e^{-s \log \lambda _j}\). Then, \(\lambda _j\) are accumulation points for some sequence \((\lambda _{n,j'})_{n=1}^\infty \).

### Proof

Assume that the set of subsequences \(\big ( (\lambda _{n_k,j})_{k=1}^\infty \big )_{j\ge 1}\) converges to the set of accumulation points \((\ell _i^{(j)})\).

*D*. If \(\ell \) is the first element in the set \(\ell _i^{(j)}\) that is smaller than \(\lambda _1\), then by choosing

*x*such that \(\ell< x < \lambda _1\), by Perron’s formula, we have that \(I_x(D_{n_k})=\sum _{j=1}^{m_1} a_{n_k,j}=A_{n_k}^{(0)}\) should tend to \(I_x(D)=0\) since \(x<\lambda _1\). This proves that \(A_{n_k}^{(0)}\) tends to zero as desired. We proceed, now, to the next accumulation point that is smaller than \(\lambda _1\), and by the same argument, we prove that \(\lim \nolimits _{n_k\rightarrow \infty } \sum _{j=1}^{m_2} a_{n_k,j}=0\). Then, since the limit of the sum of the first \(m_1\) terms tends to zero, we have that

We continue the proof by induction by taking \(\ell \) to be between \(\lambda _1\) and \(\lambda _2\), so that the corresponding sum tends to zero; then, we take \(\ell \) to be \(\lambda _2\), then between \(\lambda _2\) and \(\lambda _3\) etc. \(\square \)

## 6 Relation with Laplace–Stieltjes transform

The notion of Dirichlet series and Laplace transforms can be unified in terms of the Riemann–Stieltjes integrals (Widder [20], compare [2]).

### Definition 6.1

- 1.The space \(\mathrm {Lip}_\omega \) is defined as the set of functions \(F :\mathbf {R} _{ \ge 0} \rightarrow \mathbf {R} \) with bounded norm$$\begin{aligned} ||F||_{\mathrm {Lip},\omega }:= \sup _{0 \le s< t}\frac{ |F(t)-F(s) |}{(t-s)e^{\omega t}} < \infty . \end{aligned}$$
- 2.The space \(\mathrm {Wid}_\omega \) is defined as the space of smooth function \((\omega ,\infty ) \rightarrow \mathbf {R} \) with bounded norm$$\begin{aligned} ||D||_{\mathrm {Wid},\omega }:= \sup _{\begin{array}{c} {s>\omega }\\ {k \in \mathbf {N}} \end{array}} \frac{(s-\omega )^{k+1}}{k!} \left| \frac{d^k D}{ds^k}(s) \right| < \infty . \end{aligned}$$

The main result is now that the so-called *Laplace–Stieltjes transform* \( F \mapsto \int _0^\infty e^{-st} dF(t) \) induces an isometric isomorphism \( \mathrm {Lip}_\omega \rightarrow \mathrm {Wid}_\omega \) ([2], Thm. 2.4.1).

Widder ([20], Theorems 11.2 , 12.4) proved that a Dirichlet series of the form \(D(s)=\sum _{\nu } a_\nu e^{-s \mu _\nu }\) convergent for \(\mathfrak {R}(s)>\omega \) is in the space \(\mathrm {Wid}_{\omega }\). Also, such *D* is the Laplace–Stieltjes transform of \( F(t)=\sum _{\nu =0}^\infty a_\nu H(t-\mu _\nu ), \) where *H* is the Heaviside step function. Thus, we immediately conclude the following:

### Theorem 6.2

Suppose \(D_n(s)=\sum _{\nu \ge 1} a_{n,\nu } e^{ -s \mu _{n,\nu }}\) is a sequence of Dirichlet series each converging absolutely in a common half-plane \(\mathfrak {R}(s)>\gamma \); then for any \(\omega >\gamma \), \(D_n\) converges to a Dirichlet series \(D(s)=\sum _{\nu \ge 1} a_\nu e^{ -s \mu _\nu }\) in \(\mathrm {Wid}_{\omega }\)-norm if and only if \( \sum \nolimits _{\nu =0}^\infty \big ( a_{n,\nu } H(t-\mu _{n,\nu }) - a_\nu H(t-\mu _\nu ) \big ) \rightarrow 0\) in \(\mathrm {Lip}_\omega \)-norm.

It would be interesting to deduce Theorems 4.3 and 5.5 from Theorem 6.2.

## References

- 1.Aasen, D., Bhamre, T., Kempf, A.: Shape from sound: toward new tools for quantum gravity. Phys. Rev. Lett.
**110**(12), 121301 (2013)ADSCrossRefGoogle Scholar - 2.Arendt, W., Batty, C.J.K., Hieber, M., Neubrander, F.: Vector-valued Laplace transforms and Cauchy problems. In: Monographs in mathematics, vol. 96. Birkhäuser, Basel (2001)Google Scholar
- 3.Bérard, P., Besson, G., Gallot, S.: Embedding Riemannian manifolds by their heat kernel. Geom. Funct. Anal.
**4**(4), 373–398 (1994)MathSciNetCrossRefMATHGoogle Scholar - 4.Buchert, T., Ehlers, J.: Averaging inhomogeneous Newtonian cosmologies. Astron. Astrophys.
**320**, 1–7 (1997)ADSGoogle Scholar - 5.Connes, A.: Gravity coupled with matter and the foundation of non-commutative geometry. Commun. Math. Phys.
**182**(1), 155–176 (1996)ADSMathSciNetCrossRefMATHGoogle Scholar - 6.Conway, J.B.: Functions of one complex variable. In: Graduate Texts in Mathematics, 2nd ed., vol. 11, Springer, New York (1978)Google Scholar
- 7.Cornelissen, G., de Jong, J.W.: The spectral length of a map between Riemannian manifolds. J. Noncommut. Geom.
**6**(4), 721–748 (2012)MathSciNetCrossRefMATHGoogle Scholar - 8.Gordon, C.S., Wilson, E.N.: Continuous families of isospectral Riemannian metrics which are not locally isometric. J. Differ. Geom.
**47**(3), 504–529 (1997)MathSciNetMATHGoogle Scholar - 9.Gromov, M.: Metric structures for Riemannian and non-Riemannian spaces. In: Modern Birkhäuser Classics. Birkhäuser Boston Inc., Boston (2007)Google Scholar
- 10.Hardy, G.H., Riesz, M.: The general theory of Dirichlet’s series. In: Cambridge Tracts in Mathematics and Mathematical Physics, No. 18, Stechert-Hafner Inc, New York (1964)Google Scholar
- 11.Hobson, M.P., Jaffe, A.H., Liddle, A.R., Mukherjee, P., Parkinson, D. (eds.): Bayesian Methods in Cosmology. Cambridge University Press, Cambridge (2010)MATHGoogle Scholar
- 12.Landi, G., Rovelli, C.: General relativity in terms of Dirac eigenvalues. Phys. Rev. Lett.
**78**(16), 3051–3054 (1997)ADSMathSciNetCrossRefMATHGoogle Scholar - 13.Mandelbrojt, S.: Séries de Dirichlet. Principes et méthodes, Monographies Internationales de Mathématiques Modernes, vol. 11. Gauthier-Villars, Paris (1969)Google Scholar
- 14.Marcolli, M., Pierpaoli, E., Teh, K.: The spectral action and cosmic topology. Commun. Math. Phys.
**304**, 125–174 (2011)ADSMathSciNetCrossRefMATHGoogle Scholar - 15.Niarchou, A., Jaffe, A.: Imprints of spherical non-trivial topologies on the CMB. Phys. Rev. Lett.
**99**, 081302 (2007)ADSCrossRefGoogle Scholar - 16.Rosenberg, S.: The Laplacian on a Riemannian manifold, London Mathematical Society Student Texts, vol. 31. Cambridge University Press, Cambridge (1997)CrossRefGoogle Scholar
- 17.Seriu, M.: Spectral representation of the spacetime structure: the “distance” between universes with different topologies. Phys. Rev. D (3)
**53**(12), 6902–6920 (1996)ADSMathSciNetCrossRefGoogle Scholar - 18.Seriu, M.: Spectral representation and the averaging problem in cosmology. General. Relariv. Gravit
**32**, 1473–1485 (2000)ADSMathSciNetCrossRefMATHGoogle Scholar - 19.’t Hooft, G.: The fundamental nature of space and time. In: Oriti, D. (ed.) Approaches to Quantum Gravity, pp. 13–25. Cambridge University Press, Cambridge (2009)Google Scholar
- 20.Widder, D.V.: A generalization of Dirichlet’s series and of Laplace’s integrals by means of a Stieltjes integral. Trans. Am. Math. Soc.
**31**(4), 694–743 (1929)MathSciNetMATHGoogle Scholar

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