1 Introduction

In this paper we investigate the spectral properties of the perturbed discrete biharmonic operator

$$\begin{aligned} {\widehat{{ H}}}_{{\mu }}:={\widehat{\varDelta }} {\widehat{\varDelta }} - \mu {\widehat{{ V}}},\qquad \mu \in {\mathbb {R}}, \end{aligned}$$
(1.1)

in the d-dimensional cubical lattice \({\mathbb {Z}}^d,\) where \({\widehat{\varDelta }}\) is the discrete Laplacian and \({\widehat{{ V}}}\) is a is rank-one potential with a generating potential \({\widehat{v}}.\) This model is associated to a one-particle system in \({\mathbb {Z}}^d\) with a potential field \({\widehat{v}},\) in which the particle freely “jumps” from a node X of the lattice not only to one of its nearest neighbors Y (similar to the discrete Laplacian case), but also to the nearest neighbors of the node Y. From the mathematical point of view, the discrete bilaplacian represents a discrete Schrödinger operator with a degenerate bottom, i.e., \({\widehat{\varDelta }}{\widehat{\varDelta }}\) is unitarily equivalent to a multiplication operator by a function \({\mathfrak {e}}\) which behaves as \(o(|p-p_0|^2)\) close to its minimum point \(p_0.\)

The spectral properties of discrete Schrödinger operators with non-degenerate bottom (i.e., \({\mathfrak {e}}\) behaves as \(O(|p-p_0|^2)\) close to its minimum point \(p_0\)), in particular with discrete Laplacian, have been extensively studied in recent years (see e.g. [1, 2, 7, 8, 10, 11, 20, 21, 23, 26, 28] and references therein) because of their applications in the theory of ultracold atoms in optical lattices [16, 24, 35, 36]. In particular, it is well-known that the existence of the discrete spectrum is strongly connected to the threshold phenomenon [18, 20,21,22], which plays an role in the existence the Efimov effect in three-body systems [31, 32, 34]: if any two-body subsystem in a three-body system has no bound state below its essential spectrum and at least two two-body subsystem has a zero-energy resonance, then the corresponding three-body system has infinitely many bound states whose energies accumulate at the lower edge of the three-body essential spectrum.

Recall that the Efimov effect may appear only for certain attractive systems of particles [29]. However, recent experimental results in the theory of ultracold atoms in an optical lattice have shown that two-particle systems can have repulsive bound states and resonances (see e.g. [36]), thus, one expects the Efimov effect to hold also for some repulsive three-particle systems in \({\mathbb {Z}}^3\).

The strict mathematical justification of the Effect effect including the asymptotics for the number of negative eigenvalues of the three-body Hamiltonian has been successfully established in 3-space dimensions (for both \({\mathbb {R}}^3\) and \({\mathbb {Z}}^3\)) see e.g., [1, 4, 13, 19, 29, 31, 32, 34] and the references therein. In particular, the non-degeneracy of the bottom of the (reduced) one-particle Schrödinger operator played an important role in the study of resonance states of the associated two-body system [1, 31]. Another keypoint in the proof of the Efimov effect in \({\mathbb {Z}}^3\) was the asymptotics of the (unique) smallest eigenvalue of the (reduced) one-particle discrete Schrödinger operator which creates a singularity in the kernel of a Birman-Schwinger-type operator which used to obtain an asymptotics to the number of three-body bound states.

To the best of our knowledge, there are no published results related to the Efimov effect in lattice three-body systems in which associated (reduced) one-body Schrödinger operator has degenerate bottom.

We also recall that fourth order elliptic operators in \({\mathbb {R}}^d\) in particular, the biharmonic operator, play also a central role in a wide class of physical models such as linear elasticity theory, rigidity problems (for instance, construction of suspension bridges) and in streamfunction formulation of Stokes flows (see e.g. [9, 25, 27] and references therein). Moreover, recent investigations have shown that the Laplace and biharmonic operators have high potential in image compression with the optimized and sufficiently sparse stored data [15]. The need for corresponding numerical simulations has led to a vast literature devoted to a variety of discrete approximations to the solutions of fourth order equations [5, 12, 33]. The question of stability of such models is basically related to their spectral properties and therefore, numerous studies have been dedicated to the numerical evaluation of the eigenvalues [3, 6, 30].

The aim of the present paper is the study of the existence and asymptotics of eigenvalues as well as threshold resonance and bound states of \({\widehat{{ H}_\mu }}\) defined in (1.1), which corresponds to the one-body Schrödinger operator with degenerate bottom. Namely, we study the discrete spectrum of \({\widehat{{ H}_\mu }}\) depending on \(\mu \) and on \({\widehat{v}}.\) For simplicity we assume the generator \({\widehat{v}}\) of \({\widehat{{ V}}}\) to decay exponentially at infinity, however, we urge that our methods can also be adjusted to less regular cases (see Remark 2.6). Since the spectrum of \({\widehat{\varDelta }}\) consists of [0, 2d] (see e.g., [1]), by the compactness of \({\widehat{{ V}}}\) and Weyl’s Theorem, the essential spectrum of \({\widehat{{ H}_\mu }}\) fills the segment \([0,4d^2]\) independently of \(\mu .\) Moreover, the essential spectrum does not give birth to a new eigenvalue while \(\mu \) runs in some real interval \([-\mu ^o,\mu _o],\) and it turns out as soon as \(\mu \) leaves this interval through \(\mu _o\) resp. through \(-\mu ^o,\) a unique negative resp. a unique positive eigenvalue \(e(\mu )\) releases from the essential spectrum (Theorem 2.2).

Now we are interested in the absorption rate of \(e(\mu )\) as \(\mu \rightarrow \mu _o\) and \(\mu \rightarrow -\mu ^o.\) The associated asymptotics are highly dependent not only on the dimension d of the lattice (as in the discrete Laplacian case [20, 21]), but also values on the multiplicity \(2n_o\) and \(2n^o\) of \(0\in \{v=0\}\) (if \(v(0)=0\)) and \(\vec \pi \in \{v=0\}\) (if \(v(\vec \pi )=0\)), respectively. More precisely, depending on d and \(n_o\), \(e(\mu )\) has a convergent expansion

  • in \((\mu -\mu _o)^{1/3}\) for \(2n_o+d=1,7;\)

  • in \(\mu -\mu _o\) for \(2n_o+d=3,5;\)

  • in \((\mu -\mu _o)^{1/4}\) for \(2n_o+d\ge 9\) with d odd;

  • in \(\mu - \mu _o\) and \(-(\mu - \mu _o)\ln (\mu - \mu _o)\) for \(2n_o+d=2,6;\)

  • in \(\mu -\mu _o\) and \(e^{-1/(\mu -\mu _o)}\) for \(2n_o+d=4;\)

  • in \((\mu -\mu _o)^{1/2},\) \(-(\mu -\mu _o)\ln (\mu -\mu _o),\) \((-\frac{1}{\ln (\mu -\mu _o)})^{1/2}\) and \(-\frac{\ln \ln (\mu -\mu _o)^{-1}}{\ln (\mu -\mu _o)}\) for \(2n_o+d=8;\)

  • in \((\mu -\mu _o)^{1/2}\) and \(-(\mu -\mu _o)^{1/2}\ln (\mu -\mu _o)\) for \(2n^o+d\ge 10\) with d even

(see Theorem 2.4). Moreover, resonance states of 0-energy, i.e. non-zero solutions f of \({\widehat{{ H}}}_{\mu _o}f=0\) not belonging to \(\ell ^2({\mathbb {Z}}^d)\) appear if and only if \(2n_o+d\in \{5,6,7,8\}.\) Recall that the emergence of 0-energy resonances in more lattice dimensions could allow the Efimov effect to be observed in other dimensions than \(d=3.\)

Furthermore, observing that the top \({\mathfrak {e}}(\vec \pi )=4d^2\) of the essential spectrum is non-degenerate, one expects the asymptotics of \(e(\mu )\) as \(\mu \rightarrow -\mu ^o\) to be similar as in the discrete Laplacian case [20, 21]; more precisely, depending on d and \(n^o,\) \(e(\mu )\) has a convergent expansion

  • in \(\mu +\mu ^o\) for \(2n^o+d=1,3;\)

  • in \((\mu +\mu ^o)^{1/2}\) for \(2n^o+d\ge 5\) with d odd;

  • in \(\mu +\mu ^o\) and \(e^{-1/(\mu +\mu ^o)}\) for \(2n_o+d=2;\)

  • in \(\mu +\mu ^o,\) \(-\frac{1}{\ln (\mu +\mu ^o)}\) and \(-\frac{\ln \ln (\mu +\mu ^o)^{-1}}{\ln (\mu +\mu ^o)}\) for \(2n_o+d=4;\)

  • in \(\mu +\mu ^o\) and \(-(\mu +\mu ^o)\ln (\mu +\mu ^o)\) for \(2n^o+d\ge 6\) with d even

(see Theorem 2.5). Moreover, the resonance states of energy \(4d^2\), i.e. non-zero solutions f of \({\widehat{{ H}}}_{-\mu ^o}f=4d^2f\) not belonging to \(\ell ^2({\mathbb {Z}}^d)\) appear if and only if \(2n_o+d=3,4.\)

The threshold analysis for more general class of nonlocal discrete Schrödinger operators with \(\delta \)-potential of type

$$\begin{aligned} {\widehat{H}}_\mu = \Psi (-{\widehat{\varDelta }}) + \mu \delta _{x0}, \end{aligned}$$

can be found in [14], where \(\Psi \) is some strictly increasing \(C^1\)-function and \(\delta _{x0}\) is the Dirac’s delta-function supported at 0. Besides the existence of eigenvalues, authors of [14] classify (embedded) threshold resonances and threshold eigenvalues depending on the behaviour of \(\Psi \) at the edges of the essential spectrum of \(-{\widehat{\varDelta }}\) and on the lattice dimension d. The eigenvalue expansions for the discrete bilaplacian with \(\delta \)-perturbation have been established in [17] for \(d=1\) using the complex analytic methods.

The paper is organized as follows. In Sect. 2 after introducing some preliminaries we state the main results of the paper. In Theorem 2.2 we establish necessary and sufficient conditions for non-emptiness of the discrete spectrum of \({\widehat{{ H}_\mu }},\) and in case of existence, we study the location and the uniqueness, analiticity, monotonicity and convexity properties of eigenvalues \(e(\mu )\) as a function of \(\mu .\) In particular, we study the asymptotics of \(e(\mu )\) as \(\mu \rightarrow \mu _o\) and \(\mu \rightarrow -\mu ^o\) as well as \(\mu \rightarrow \pm \infty .\) As discussed above in Theorems 2.4 and 2.5 we obtain expansions of \(e(\mu )\) for small and positive \(\mu -\mu _o\) and \(\mu +\mu ^o\). In Sect. 3 we prove the main results. The main idea of the proof is to obtain a nonlinear equation \(\Delta (\mu ;z)=0\) with respect to the eigenvalue \(z=e(\mu )\) of \({\widehat{{ H}_\mu }}\) and then study properties of \(\Delta (\mu ;z).\) Finally, in appendix Section A we obtain the asymptotics of certain integrals related to \(\Delta (\mu ;z)\) which will be used in the proofs of main results.

1.1 Data availability statement

We confirm that the current manuscript has no associated data.

2 Preliminary and main results

Let \({\mathbb {Z}}^d\) be the d-dimensional lattice and \(\ell ^2({\mathbb {Z}}^d)\) be the Hilbert space of square-summable functions on \({\mathbb {Z}}^d.\) Consider the family

$$\begin{aligned} {\widehat{{ H}_\mu }}:={\widehat{{ H}}}_0 - \mu {\widehat{{ V}}},\qquad \mu \ge 0, \end{aligned}$$

of self-adjoint bounded discrete Schrödinger operators in \(\ell ^2({\mathbb {Z}}^d).\) Here \({\widehat{{ H}}}_0:={\widehat{\varDelta }}{\widehat{\varDelta }}\) is discrete bilaplacian, where

$$\begin{aligned} {\widehat{\varDelta }} f(x) = \frac{1}{2}\,\sum \limits _{|s|=1} [f(x) - f(x+s)],\qquad f\in \ell ^2({\mathbb {Z}}^d), \end{aligned}$$

is the discrete Laplacian, and \({\widehat{{ V}}}\) is a rank-one operator

$$\begin{aligned} {\widehat{{ V}}} {\widehat{f}}(x) = {\widehat{v}}(x) \sum \limits _{y\in {\mathbb {Z}}^d} {{\widehat{v}}(y)} {\widehat{f}}(y), \end{aligned}$$

where \({\widehat{v}}\in \ell ^2({\mathbb {Z}}^d)\setminus \{0\}\) is a given real-valued function.

Let \({\mathbb {T}}^d\) be the d-dimensional torus equipped with the Haar measure and \(L^2({\mathbb {T}}^d)\) be the Hilbert space of square-integrable functions on \({\mathbb {T}}^d.\) By \({\mathcal {F}}\) we denote the the standard Fourier transform

$$\begin{aligned} {\mathcal {F}}:\ell ^2({\mathbb {Z}}^d)\rightarrow L^2({\mathbb {T}}^d),\qquad {\mathcal {F}}{\widehat{f}}(p) = \frac{1}{(2\pi )^{d/2}}\,\sum \limits _{x\in {\mathbb {Z}}^d} {\widehat{f}}(x) e^{ixp}. \end{aligned}$$

Further we always assume that \({\widehat{v}}\) and its Fourier image

$$\begin{aligned} v(p):={\mathcal {F}}{\widehat{v}}(p)=\frac{1}{(2\pi )^{d/2}}\sum \limits _{x\in {\mathbb {Z}}^d} {\widehat{v}}(x)e^{ix\cdot p} \end{aligned}$$

satisfy the following assumptions:

figure a

here \(D^jf(p)\) is the j-th order differential of f at p,  i.e. the j-th order symmetric tensor

$$\begin{aligned} D^jf(p)[\underbrace{w,\ldots ,w}_{j-times}]= & {} \sum \limits _{i_1+\ldots +i_d =j,i_k\ge 0} \frac{\partial ^jf(p)}{\partial ^{i_1} p_1\ldots \partial ^{i_d}p_d} \,w_1^{i_1}\ldots w_d^{i_d},\nonumber \\&\qquad \quad w=(w_1,\ldots ,w_d)\in {\mathbb {R}}^d, \end{aligned}$$

and \(\vec {\pi }=(\pi ,\ldots ,\pi )\in {\mathbb {T}}^d.\) Notice that under assumption (H1), v is analytic on \({\mathbb {T}}^d.\)

Recall that \( \sigma ({\widehat{\varDelta }}) = \sigma _{\mathrm {ess}}({\widehat{\varDelta }}) =[0,2d] \) (see e.g. [1]). Hence, \( \sigma ({\widehat{{ H}}}_0) = \sigma _{\mathrm {ess}}({\widehat{{ H}}}_0) =[0,4d^2], \) and by the compactness of \({\widehat{{ V}}}\) and Weyl’s Theorem,

$$\begin{aligned} \sigma _{\mathrm {ess}}({\widehat{{ H}_\mu }}) = \sigma _{\mathrm {ess}}({\widehat{{ H}}}_0) =[0,4d^2] \end{aligned}$$

for any \(\mu \in {\mathbb {R}}.\)

Before stating the main results let us introduce the constants

$$\begin{aligned}&\mu _o:= \Big (\int _{{\mathbb {T}}^d} \frac{|v(q)|^2dq}{{\mathfrak {e}}(q)}\Big )^{-1},\qquad \mu ^o:= \Big (\int _{{\mathbb {T}}^d} \frac{|v(q)|^2dq}{4d^2 - {\mathfrak {e}}(q)}\Big )^{-1}, \end{aligned}$$
(2.2)
$$\begin{aligned}&{\widehat{c}}_v:= \int _{{\mathbb {T}}^d} \frac{|v(q)|^2dq}{{\mathfrak {e}}(q)^2},\qquad {\widehat{C}}_v:= \int _{{\mathbb {T}}^d} \frac{|v(q)|^2dq}{(4d^2 - {\mathfrak {e}}(q))^2}, \end{aligned}$$
(2.3)

and

$$\begin{aligned} c_v:=&\frac{2^{2n_o+d}}{(2n_o)!}\, \int _{{\mathbb {S}}^{d-1}} D^{2n_o}|v(0)|^2[w,\ldots , w]\,d{\mathcal {H}}^{d-1}(w), \end{aligned}$$
(2.4)
$$\begin{aligned} C_v:=&\frac{2^{2n^o+d-1}}{(8d)^{n^o+d/2}\,(2n^o)!}\, \int _{{\mathbb {S}}^{d-1}} D^{2n^o}|v(\vec \pi )|^2[w,\ldots ,w]\,d{\mathcal {H}}^{d-1}(w), \end{aligned}$$
(2.5)

where \({\mathbb {S}}^{d-1}\) is the unit sphere in \({\mathbb {R}}^d\) and

$$\begin{aligned} {\mathfrak {e}}(q): =\left( \sum \limits _{i=1}^d ( 1 - \cos q_i)\right) ^2. \end{aligned}$$

Remark 2.1

Under assumptions (H1)–(H3), \(\mu _o,\mu ^o\ge 0,\) \(c_v,C_v>0,\) and \({\widehat{c}}_v,{\widehat{C}}_v\in (0,+\infty ].\) Moreover, by Propositions A.1 and A.2:

  • \(\mu _o=0\) (resp. \(\mu ^o=0\)) if and only if \(2n_o+d\le 4\) (resp. \(2n^o+d\le 2\));

  • \({\widehat{c}}_v<\infty \) (resp. \({\widehat{C}}_v<\infty \)) if \(2n_o+d\ge 9\) (resp. \(2n^o+d\ge 5\)).

2.1 Main results

First we concern with the existence of the discrete spectrum of \({\widehat{{ H}_\mu }}.\)

Theorem 2.2

Let \(\mu _o,\mu ^o\ge 0\) be given by (2.2). Then \(\sigma _{\mathrm {disc}}({\widehat{{ H}_\mu }})=\emptyset \) for any \(\mu \in [-\mu ^o,\mu _o]\) and \(\sigma _{\mathrm {disc}}({\widehat{{ H}_\mu }})\) is a singleton \(\{e(\mu )\}\) for any \(\mu \in {\mathbb {R}}\setminus [-\mu ^o,\mu _o].\) Moreover, the associated eigenfunction \({\widehat{f}}_\mu \) to \(e(\mu )\) is given by \({\widehat{f}}_\mu :={\mathcal {F}}^*f_\mu ,\) where

$$\begin{aligned} f_\mu (p) = \frac{v(p)}{{\mathfrak {e}}(p) - e(\mu )}. \end{aligned}$$

Furthermore, if \(\mu <-\mu ^o\) (resp. \(\mu >\mu _o\)), then \(e(\mu )>4d^2\) (resp. \(e(\mu )<0\)). Moreover, the function \(\mu \in {\mathbb {R}}\setminus [-\mu ^o,\mu _o]\mapsto e(\mu )\) is real-analytic strictly decreasing, convex in \((-\infty ,-\mu ^o)\) and concave in \((\mu _o,+\infty ),\) and satisfies

$$\begin{aligned} \lim \limits _{\mu \searrow \mu _o} e(\mu ) =0\qquad \text {and}\qquad \lim \limits _{\mu \nearrow -\mu ^o} e(\mu ) =4d^2 \end{aligned}$$
(2.6)

and

$$\begin{aligned} \lim \limits _{\mu \rightarrow \pm \infty } \frac{e(\mu )}{\mu } = - \int _{{\mathbb {T}}^d}|v(q)|^2dq. \end{aligned}$$
(2.7)

Next we study the threshold resonances of \({\widehat{{ H}_\mu }}.\)

Theorem 2.3

Let \(n_o,n^o\ge 0\) be given by (H2)–(H3).

  1. (a)

    Let \(2n_o+d\ge 5.\) Then \({\widehat{f}}:={\mathcal {F}}^*f\in c_0({\mathbb {Z}}^d),\) i.e., \({\widehat{f}}(x)\rightarrow 0\) as \(|x|\rightarrow +\infty ,\) where

    $$\begin{aligned} f(p) = \frac{v(p)}{{\mathfrak {e}}(p)} \in L^1({\mathbb {T}}^d). \end{aligned}$$

    Moreover, \({\widehat{f}}\in c_0({\mathbb {Z}}^d)\setminus \ell ^2({\mathbb {Z}}^d)\) for \(2n_o+d\in \{5,6,7,8\},\) \({\widehat{f}}\in \ell ^2({\mathbb {Z}}^d)\) for \(2n_o+d\ge 9,\) and \({\widehat{f}}\) solves the equation \({\widehat{{ H}}}_{\mu _o} f=0.\)

  2. (b)

    Let \(2n^o+d\ge 3.\) Then \({\widehat{g}}:={\mathcal {F}}^*g\in \ell ^0({\mathbb {Z}}^d),\) where

    $$\begin{aligned} g(p) = \frac{v(p)}{4d^2 - {\mathfrak {e}}(p)}. \end{aligned}$$

    Moreover, \({\widehat{g}}\in \ell ^0({\mathbb {Z}}^d)\setminus \ell ^2({\mathbb {Z}}^d)\) for \(2n^o+d\in \{3,4\},\) \({\widehat{g}}\in \ell ^2({\mathbb {Z}}^d)\) for \(2n^o+d\ge 5,\) and \({\widehat{g}}\) solves the equation \({\widehat{{ H}}}_{-\mu ^o} f=4d^2f.\)

We recall that in the literature the non-zero solutions of equations \({\widehat{{ H}_\mu }} {\widehat{f}}=0\) and \({\widehat{{ H}_\mu }}{\widehat{g}}= 4d^2 {\widehat{g}}\) not belonging to \(\ell ^2({\mathbb {Z}}^d)\) are called the resonance states [1, 2].

Now we study the rate of the convergences in (2.6).

Theorem 2.4

(Expansions of \(e(\mu )\) at \(\mu =\mu _o\)) For \(\mu >\mu _o\) let \(e(\mu )<0\) be the eigenvalue of \({\widehat{{ H}_\mu }}.\)

  1. (a)

    Suppose that d is odd:

    1. (a1)

      if \(2n_o+d=1,3,\) then \(\mu _o=0\) and for sufficiently small and positive \(\mu ,\)

      $$\begin{aligned} (- e(\mu ))^{1/4}= {\left\{ \begin{array}{ll} \Big (\frac{\pi c_v}{4}\Big )^{1/3}\,\mu ^{1/3} + \sum \limits _{n\ge 1} c_{1,n} \mu ^{\frac{n+1}{3}}, &{} 2n_o+d=1,\\ \frac{\pi c_v}{8}\,\mu + \sum \limits _{n\ge 1} c_{3,n} \mu ^{n+1}, &{} 2n_o+d=3, \end{array}\right. } \end{aligned}$$

      where \(\{c_{1,n}\}\) and \(\{c_{3,n}\}\) are some real coefficients;

    2. (a2)

      if \(2n_o+d=5,7,\) then \(\mu _o>0\) and for sufficiently small and positive \(\mu -\mu _o,\)

      $$\begin{aligned}&(- e(\mu ))^{1/4}\\&\quad = {\left\{ \begin{array}{ll} \frac{8}{\pi c_v\mu _o^2} \, (\mu -\mu _o) +\sum \limits _{n\ge 1} c_{5,n} (\mu -\mu _o)^{n+1}, &{} 2n_o+d=5,\\ \Big (\frac{8}{\pi c_v\mu _o^2}\Big )^{1/3}\, (\mu -\mu _o)^{1/3} + \sum \limits _{n\ge 1} c_{7,n} (\mu -\mu _o)^{\frac{n+1}{3}}, &{} 2n_o+d=7, \end{array}\right. } \end{aligned}$$

      where \(\{c_{5,n}\}\) and \(\{c_{7,n}\}\) are some real coefficients;

    3. (a3)

      if \(2n_o+d\ge 9,\) then \(\mu _o>0\) and for sufficiently small and positive \(\mu -\mu _o,\)

      $$\begin{aligned} (- e(\mu ))^{1/4}= (\mu _o^2{\widehat{c}}_v)^{-1/4}\,(\mu -\mu _o)^{1/4} + \sum \limits _{n\ge 1} c_{9,n} (\mu -\mu _o)^{n/4}, \end{aligned}$$

      where \(\{c_{9,n}\}\) are some real coefficients.

  2. (b)

    Suppose that d is even:

    1. (b1)

      if \(2n_o+d=2,4,\) then \(\mu _o=0\) and for sufficiently small and positive \(\mu ,\)

      $$\begin{aligned}&(- e(\mu ))^{1/2}\\&\quad = {\left\{ \begin{array}{ll} \frac{\pi c_v}{8}\,\mu + \sum \limits _{n+m\ge 1,n,m\ge 0} c_{2,nm} \mu ^{n+1}(-\mu \ln \mu )^{m}, &{} 2n_o+d=2,\\ ce^{-\frac{8}{c_v\mu }} +\sum \limits _{n+m\ge 1,n,m\ge 0} c_{4,nm} \mu ^{n+1}\left( \frac{1}{\mu }\,e^{-\frac{8}{c_v\mu }}\right) ^{m+1}, &{} 2n_o+d=4, \end{array}\right. } \end{aligned}$$

      where \(\{c_{2,nm}\}\) and \(\{c_{4,nm}\}\) are some real coefficients and \(c>0;\)

    2. (b2)

      if \(2n_o+d=6,8,\) then \(\mu _o>0\) and for sufficiently small and positive \(\mu -\mu _o,\)

      $$\begin{aligned}&(- e(\mu ))^{1/2}\\&\quad = {\left\{ \begin{array}{ll} \frac{8}{\pi c_v\mu _o^2}\,\tau ^2 + \sum \limits _{n+m\ge 1,n,m\ge 0} c_{6,nm} \tau ^{2n+2}\theta ^m, &{} 2n_o+d=6,\\ \Big (\frac{8}{c_v\mu _o^2}\Big )^{1/2}\,\tau \sigma + \sum \limits _{n+m+k\ge 1,n,m,k\ge 0} c_{8,nmk} \tau ^{n+1} \sigma ^{m+1}\eta ^k, &{} 2n_o+d=8, \end{array}\right. } \end{aligned}$$

      where \(\{c_{4,nm}\}\) and \(\{c_{8,nmk}\}\) are some real coefficients and

      $$\begin{aligned} \tau :=(\mu -\mu _o)^{1/2},\,\,\, \theta :=-\tau ^2\ln \tau ,\,\,\, \sigma :=\Big (-\frac{1}{\ln \tau }\Big )^{1/2},\,\,\, \eta :=-\frac{\ln \ln \tau ^{-1}}{\ln \tau },\nonumber \\ \end{aligned}$$
      (2.8)
    3. (b3)

      if \(2n_o+d\ge 10,\) then \(\mu _o>0\) and for sufficiently small and positive \(\mu -\mu _o,\)

      $$\begin{aligned} (- e(\mu ))^{1/2}= (\mu _o^2{\widehat{c}}_v)^{-1/2}\,\tau + \sum \limits _{n+m\ge 1,n,m\ge 0} c_{10,nm} \tau ^{n+1}\theta ^m, \end{aligned}$$

      where \(\{c_{10,nm}\}\) are some real coefficients.

Here \(c_v>0\) and \({\widehat{c}}_v>0\) are given by (2.4) and (2.3), respectively.

Theorem 2.5

(Expansions of \(e(\mu )\) at \(\mu =-\mu ^o\)) For let \(\mu <-\mu ^o\) let \(e(\mu )>4d^2\) be the eigenvalue of \({\widehat{{ H}_\mu }}.\)

  1. (a)

    Suppose that d is odd:

    1. (a1)

      if \(2n^o+d=1,\) then \(\mu ^o=0\) and for sufficiently small and negative \(\mu ,\)

      $$\begin{aligned} (e(\mu ) - 4d^2)^{1/2}= -\pi C_v\,\mu + \sum \limits _{n\ge 1} C_{1,n} \mu ^{n+1}, \end{aligned}$$

      where \(\{C_{1,n}\}\) are some real coefficients;

    2. (a2)

      if \(2n^o+d=3,\) then \(\mu ^o>0\) and for sufficiently small and positive \(\mu +\mu ^o,\)

      $$\begin{aligned} (e(\mu ) - 4d^2)^{1/2}= (\pi C_v{\mu ^o}^2)^{-1}\,(\mu +\mu ^o) +\sum \limits _{n\ge 1} C_{3,n} (\mu +\mu ^o)^{n+1}, \end{aligned}$$

      where \(\{C_{3,n}\}\) and \(\{C_{7,n}\}\) are some real coefficients;

    3. (a3)

      if \(2n^o+d\ge 5,\) then \(\mu ^o>0\) and for sufficiently small and positive \(\mu +\mu ^o,\)

      $$\begin{aligned} (e(\mu ) - 4d^2)^{1/2}= ({\widehat{C}}_v {\mu ^o}^2)^{-1/2}\,(\mu +\mu ^o)^{1/2} + \sum \limits _{n\ge 1} C_{5,n} (\mu +\mu ^o)^{(n+1)/2}, \end{aligned}$$

      where \(\{C_{5,n}\}\) are some real coefficients.

  2. (b)

    Suppose that d is even:

    1. (b1)

      if \(2n_o+d=2,\) then \(\mu _o=0\) and for sufficiently small and negative \(\mu ,\)

      $$\begin{aligned} e(\mu ) - 4d^2= C\,e^{\frac{1}{C_v\mu }} +\sum \limits _{n+m\ge 1,n,m\ge 0} C_{2,nm} \mu ^{n+1}\left( -\frac{1}{\mu }\,e^{\frac{1}{C_v\mu }}\right) ^{m+1}, \end{aligned}$$

      where \(\{C_{2,nm}\}\) are some real coefficients and \(C>0;\)

    2. (b2)

      if \(2n_o+d=4,\) then \(\mu ^o>0\) and for sufficiently small and positive \(\mu +\mu ^o,\)

      $$\begin{aligned} e(\mu ) - 4d^2= (C_v{\mu ^o}^2)^{-1}\,\mu \sigma + \sum \limits _{n+m+k\ge 1,n,m,k\ge 0} C_{4,nmk} \tau ^{n+1} \sigma ^{m+1}\eta ^k, \end{aligned}$$

      where \(\{C_{4,nm}\}\) are some real coefficients and

      $$\begin{aligned} \tau :=\mu +\mu ^o,\qquad \sigma :=-\frac{1}{\ln \tau },\qquad \eta :=-\frac{\ln \ln \tau ^{-1}}{\ln \tau }; \end{aligned}$$
    3. (b3)

      if \(2n_o+d\ge 6,\) then \(\mu ^o>0\) and for sufficiently small and positive \(\mu +\mu ^o,\)

      $$\begin{aligned} e(\mu )-4d^2= & {} ({\widehat{C}}_v{\mu ^o}^2)^{-1}\,(\mu +\mu ^o)\\&+ \sum \limits _{n+m\ge 1,n,m\ge 0} C_{6,nm} (\mu +\mu ^o)^{n+1}[-(\mu +\mu ^o)\ln (\mu +\mu ^o)]^m, \end{aligned}$$

      where \(\{C_{6,nm}\}\) are some real coefficients.

Here \(C_v\) and \({\widehat{C}}_v\) are given by (2.5) and (2.3), respectively.

Remark 2.6

Few comments on the main results are in order.

  1. 1.

    The assertions of Theorem 2.2 hold in fact for any \({\widehat{v}}\in \ell ^2({\mathbb {Z}}^d)\) (see Remark 3.2);

  2. 2.

    Similar expansions of \(e(\mu )\) in Theorems 2.4 and 2.5 at \(\mu =\mu _o\) and \(\mu =-\mu ^o,\) respectively, still hold for any exponentially decaying \({\widehat{v}}:{\mathbb {Z}}^d\rightarrow {\mathbb {C}}\) (see Remark 3.3);

  3. 3.

    If \({\widehat{v}}\) decays at most polynomially at infinity, i.e. \({\widehat{v}}(x) = O(|x|^{-\alpha })\) for some \(\alpha >0,\) then instead of the expansions in Theorem 2.4 and 2.5 we obtain only asymptotics of \(e(\mu )\) (see Remark 3.4).

3 Proof of main results

In this section we prove the main results. By the Birman-Schwinger principle and the Fredholm Theorem we have

Lemma 3.1

A complex number \(z\in {\mathbb {C}}\setminus [0,4d^2]\) is an eigenvalue of \({\widehat{{ H}_\mu }}\) if and only if

$$\begin{aligned} \Delta (\mu ;z):=1 - \mu \int _{{\mathbb {T}}^d} \frac{|v(q)|^2dq}{{\mathfrak {e}}(q) - z}=0. \end{aligned}$$

Proof of Theorem 2.2

By the definition of \(\mu _o,\) for any \(\mu <-\mu ^o:\)

$$\begin{aligned} \lim \limits _{z\nearrow -\mu ^o} \Delta (\mu ;z) = 1 + \frac{\mu }{\mu ^o}<0,\qquad \lim \limits _{z\rightarrow +\infty } \Delta (\mu ;z) =1. \end{aligned}$$

Since \(\Delta (\mu ;z)>1\) for \(z<0\) and \(\mu >-\mu ^o,\) in view of the strict monotonicity \(\Delta (\mu ;\cdot )\) in \((4d^2,\infty ),\) for any \(\mu <-\mu ^o\) there exists a unique \(e(\mu )\in (4d^2,+\infty )\) such that \(\Delta (\mu ;e(\mu ))=0.\) Analogously, for any \(\mu >\mu _o\) there exists a unique \(e(\mu )\in (-\infty ,0)\) such that \(\Delta (\mu ;e(\mu ))=0.\) By the Implicit Function Theorem the function \(\mu \in {\mathbb {R}}\setminus [-\mu ^o,\mu _o]\mapsto e(\mu )\) is real-analytic. Moreover, computing the derivatives of the implicit function \(e(\mu )\) we find:

$$\begin{aligned} e'(\mu ) = - \frac{1}{\mu }\,\int _{{\mathbb {T}}^d} \frac{|v(q)|^2dq}{{\mathfrak {e}}(q) - e(\mu )}\,\Big ( \int _{{\mathbb {T}}^d} \frac{|v(q)|^2dq}{({\mathfrak {e}}(q) - e(\mu ))^2}\Big )^{-1},\qquad \mu \ne 0, \end{aligned}$$
(3.1)

thus, using \(\mu ({\mathfrak {e}}(q) - e(\mu ))>0\) we get \(e'(\mu )<0,\) i.e. \(e(\cdot )\) is strictly decreasing in \({\mathbb {R}}\setminus \{0\}.\) Differentiating (3.1) one more time we get

$$\begin{aligned} e''(\mu ) = \frac{2e'(\mu )}{\mu }\,\left( 1-\mu e'(\mu )\,\int _{{\mathbb {T}}^d} \frac{|v(q)|^2dq}{({\mathfrak {e}}(q) - e(\mu ))^3}\,\left( \int _{{\mathbb {T}}^d} \frac{|v(q)|^2dq}{({\mathfrak {e}}(q) - e(\mu ))^2}\right) ^{-1}\right) . \end{aligned}$$

Therefore, \(e''(\mu )>0\) (i.e. \(e(\cdot )\) is strictly convex) for \(\mu <0\) and \(e''(\mu )<0\) (i.e. \(e(\cdot )\) is strictly concave) for \(\mu >0.\)

To prove (2.7), first we let \(\mu \rightarrow \pm \infty \) in

$$\begin{aligned} 1= \mu \int _{{\mathbb {T}}^d} \frac{|v(q)|^2dq}{{\mathfrak {e}}(q) - e(\mu )} \end{aligned}$$
(3.2)

and find \(\lim \limits _{\mu \rightarrow \pm \infty } e(\mu )=\mp \infty .\) In particular, if \(|\mu |\) is sufficiently large, \(|\frac{{\mathfrak {e}}(q)}{e(\mu )}|<\frac{1}{2}\) and hence, by (3.2) and the Dominated Convergence Theorem,

$$\begin{aligned} \lim \limits _{\mu \rightarrow \pm \infty } \frac{e(\mu )}{\mu } = - \lim \limits _{\mu \rightarrow \pm \infty } \int _{{\mathbb {T}}^d}\frac{|v(q)|^2dq}{1- \frac{{\mathfrak {e}}(q)}{e(\mu )}} = -\int _{{\mathbb {T}}^d} |v(q)|^2dq. \end{aligned}$$

To prove that \({\widehat{f}}_\mu \) solves \({\widehat{{ H}_\mu }} {\widehat{f}}_\mu =e(\mu ){\widehat{f}}_\mu \) we consider the equivalent equality \({\mathcal {F}}{\widehat{{ H}_\mu }} {\mathcal {F}}^* f_\mu =e(\mu )f_\mu ,\) which is easily reduced to the equality \(\Delta (\mu ;e(\mu ))=0.\) \(\square \)

Remark 3.2

In view of Lemma 3.1 and the proof of Theorem 2.2, their assertions still hold for any \(v\in \ell ^2({\mathbb {Z}}^d).\)

Proof of Theorem 2.3

We prove only (a), the proof of (b) being similar. Repeating the proof of the continuity (resp. differentiability) of \(\mathfrak {l}_f\) at \(z=0\) in Proposition A.1 one can show that \(f\in L^1({\mathbb {T}}^d)\setminus L^2({\mathbb {T}}^d)\) for \(2n_o+d\in \{5,6,7,8\}\) and \(f\in L^2({\mathbb {T}}^d)\) for \(2n_o+d\ge 9.\) Thus, by the Riemann-Lebesgue Lemma, \({\widehat{f}}\in \ell ^0({\mathbb {Z}}^d).\) To show that \({\widehat{{ H}}}_{\mu _o}{\widehat{f}}=0\) it suffices to observe that \({\mathcal {F}}{\widehat{{ H}}}_{\mu _0} {\mathcal {F}}^*f=0.\) \(\square \)

Proof of Theorem 2.4

Since

$$\begin{aligned} |v(p)|^2= (2\pi )^{-d}\left( \sum \limits _{x\in {\mathbb {Z}}^d} {\widehat{v}}(x)\cos p\cdot x\right) ^2+(2\pi )^{-d}\left( \sum \limits _{x\in {\mathbb {Z}}^d} {\widehat{v}}(x)\sin p\cdot x\right) ^2,\nonumber \\ \end{aligned}$$
(3.3)

the function \(p\in {\mathbb {T}}^d\mapsto |v(p)|^2\) is nonnegative even real-analytic function. Notice also that if \(n_o\ge 1,\) then by the nonnegativity of \(|v|^2,\) \(p=0\) is a global minimum for \(|v|^2.\) Therefore, the tensor \( D^{2n_o}|v(0)|^2 \) is positively definite and

$$\begin{aligned} c_v:=\frac{2^{2n_o+d}}{(2n_o)!} \int _{{\mathbb {S}}^{d-1}} D^{2n_o} |v(0)|^2[w,\ldots ,w]d{\mathcal {H}}^{d-1}>0. \end{aligned}$$

Note that

$$\begin{aligned} {\widehat{c}}_v = \mathfrak {l}_{|v|^2}'(0)= \int _{{\mathbb {T}}^d}\frac{|v(q)|^2dq}{{\mathfrak {e}}(q)^2}, \end{aligned}$$

where \(\mathfrak {l}_f\) is defined in (A.1). By Proposition A.1, \(f(p)=\frac{v(p)}{{\mathfrak {e}}(p)}\in L^2({\mathbb {T}}^d)\) if and only if \(2n_o+d\ge 9.\) Moreover, by definition, \(\mu _o>0\) and \(\Delta (\mu _o;0)=0\) for \(2n_o+d\ge 5,\) and hence, as in the proof of Lemma 3.1 for such d one can show that \({ H}_{\mu _o}f=0.\)

In view of the strict monotonicity and (2.6) there exists a unique \(\mu _1>0\) such that \(e(\mu )\in (-\frac{1}{128},0)\) for any \(\mu \in (0,\mu _1).\) Since

$$\begin{aligned} \mu = (\mathfrak {l}_{|v|^2}(e(\mu )))^{-1}, \end{aligned}$$
(3.4)

we can use Proposition A.1 with \(f=|v|^2\) and \(e:=e(\mu ),\) to find the expansions of the inverse function \(\mu :=\mu (e).\) Then applying the appropriate versions of the Implicit Function Theorem in analytical case we get the expansions of \(e=e(\mu ).\) Notice that from (A.3) and (A.4) as well as (3.5) it follows that \(\mu _o=0\) for \(2n_o+d \le 4\) and \(\mu _o=\Big (\int _{{\mathbb {T}}^d} \frac{|v(q)|^2dq}{{\mathfrak {e}}(q)}\Big )^{-1}>0\) for \(2n_o+d\ge 5.\)

(a) Suppose that d is odd. In view of the expansions (A.3) of \(\mathfrak {l}_f\), in this case, (3.4) is reduced to the inverting the equation

$$\begin{aligned} \mu = g(\alpha ), \end{aligned}$$
(3.5)

where \(\alpha :=(-e)^{1/4}\) and g is an analytic function around \(\alpha =0.\)

Case \(2n_o+d=1.\) In this case by (A.3),

$$\begin{aligned} g(\alpha ) := \frac{\alpha ^3}{c_1^3 + \sum \nolimits _{n\ge 1} a_n \alpha ^n}, \end{aligned}$$

where \(\{a_n \}\subset {\mathbb {R}}\) and \(c_1:=(\pi c_v/4)^{1/3}\) and (3.5) is equivalently represented as

$$\begin{aligned} \alpha = \mu \left( c_1^3 + \sum \limits _{n\ge 1} a_n \alpha ^{n}\right) ^{1/3}, \end{aligned}$$
(3.6)

where \(\mu =\mu ^{1/3}.\) Now setting

$$\begin{aligned} \alpha = \mu (c_1 + u), \end{aligned}$$
(3.7)

and using the Taylor series of \((c_1^3+x)^{1/3},\) for \(\mu \) and u sufficiently small we rewrite (3.6) as

$$\begin{aligned} F(u,\mu ):= u - \sum \limits _{n\ge 1} {\tilde{a}}_n \mu ^n(c_1 + u)^n =0, \end{aligned}$$
(3.8)

where \(F(\cdot ,\cdot )\) is analytic at \((u,\mu )=(0,0),\) \(F(0,0)=0\) and \(F_u(0,0) =1.\) Hence, by the Implicit Function Theorem, there exists \(\gamma _1>0\) such that for \(|\mu |<\gamma _1,\) (3.8) has a unique real-analytic solution \(u=u(\mu )\) which can be represented as an absolutely convergent series \(u=\sum \nolimits _{n\ge 1} b_n\mu ^n.\) Putting this in (3.7) and recalling the definitions of \(\alpha \) and \(\mu \) we get the expansion of \((-e(\mu ))^{1/4}\) for \(\mu >0\) small.

Case \(2n_o+d=3.\) By (A.3),

$$\begin{aligned} g(\alpha )=\alpha \left( c_3 + \sum \limits _{n\ge 1} a_n \alpha ^n\right) ^{-1}, \end{aligned}$$
(3.9)

where \(\{a_n\}\subset {\mathbb {R}}\) and \(c_3:=\pi c_v/8,\) and hence, (3.5) is represented as

$$\begin{aligned} \alpha = \mu \left( c_3 + \sum \limits _{n\ge 1} a_n \alpha ^n\right) . \end{aligned}$$

Then setting \(\alpha =\mu (c_3+u)\) we rewrite (3.9) in the form (3.8), and as in the case of \(2n_o+d=1,\) we get the expansion of \((-e(\mu ))^{1/4}.\)

Case \(2n_o+d=5.\) In this case by (A.3)

$$\begin{aligned} g(\alpha )= \left( \frac{1}{\mu _o} - \frac{\pi c_v\alpha }{8}\left( 1+ \sum \limits _{n\ge 1}a_n\alpha ^n \right) \right) ^{-1}, \end{aligned}$$

where \(\{a_n\}\subset {\mathbb {R}},\) and hence, by (3.5),

$$\begin{aligned} \frac{\mu - \mu _o}{\mu \mu _o}= \frac{\pi c_v\alpha }{8}\left( 1+ \sum \limits _{n\ge 1}a_n\alpha ^n \right) . \end{aligned}$$
(3.10)

Note that if \(|\mu -\mu _o|<\mu _o,\) then

$$\begin{aligned} \frac{\mu - \mu _o}{\mu \mu _o} = \frac{\mu - \mu _o}{{\mu _o}^2+ \mu _o(\mu - \mu _o)} = \frac{\mu - \mu _o}{{\mu _o}^2} \sum \limits _{n\ge 0} \left( \frac{\mu - \mu _o}{\mu _o}\right) ^n, \end{aligned}$$
(3.11)

thus from (3.10) we get

$$\begin{aligned} \alpha = (\mu - \mu _o)\left( c_5 + c_5 \sum \limits _{n\ge 1} \mu _o^{-n} (\mu - \mu _o)^n\right) \,\left( 1+ \sum \limits _{n\ge 1}a_n\alpha ^n \right) ^{-1}. \end{aligned}$$

and \(c_5:=8/(\pi c_v\mu _o^2).\) Now setting \(\alpha =(\mu -\mu _o)\,(c_5+u)\) for sufficiently small and positive \(\mu -\mu _o\) we get

$$\begin{aligned} u=\sum \limits _{n,m\ge 1} {\tilde{c}}_{n,m}(\mu - \mu _o)^n (c_5 + u)^m, \end{aligned}$$

where \({\tilde{c}}_{n,m}\subset {\mathbb {R}}.\) By the Implicit Function Theorem, for sufficiently small \(\mu -\mu _o\) there exists a unique real-analytic function \(u=u(\mu )\) given by the absolutely convergent series \(u(\mu ) = \sum \limits _{n\ge 1} b_n(\mu - \mu _o)^n.\) By the definition of \(\alpha , \) this implies the expansion of \((-e(\mu ))^{1/4}.\)

Case \(2n_o+d=7.\) As the previous case, by (A.3) and (3.11), the equation (3.5) is represented as

$$\begin{aligned} (\mu - \mu _o)\left( c_7^3 + c_7^3\sum \limits _{n\ge 1} \mu _o^{-n}(\mu - \mu _o)^n\right) = \alpha ^{3} \left( 1 + \sum \limits _{n\ge 1}a_n\alpha ^n \right) , \end{aligned}$$
(3.12)

where \(\{a_n\}\subset {\mathbb {R}}\) and \(c_7:=[8/(\pi c_v\mu _o^2)]^{1/3}\). When \(\mu -\mu _o>0\) is small enough, by the Taylor series of \((1+x)^{\pm 1/3}\) at \(x=0,\) (3.12) is equivalently rewritten as

$$\begin{aligned} \alpha = (\mu - \mu _o)^{1/3}\left( c_7 + \sum \limits _{n\ge 1} {\tilde{c}}_n(\mu - \mu _o)^n\right) \left( 1 + \sum \limits _{n\ge 1}{\tilde{a}}_n\alpha ^n \right) , \end{aligned}$$
(3.13)

Thus, for \(\rho =(\mu -\mu _o)^{1/3},\) setting \(\alpha =\rho \,(c_7+u)\) in (3.13), for sufficiently small and positive \(\rho \) we get

$$\begin{aligned} u=\sum \limits _{n,m\ge 1} {\tilde{c}}_{n,m}\rho ^n(c_7+u)^m. \end{aligned}$$

By the Implicit Function Theorem, this equation has a unique real-analytic solution \(u=u(\rho )\) given by the absolutely convergent series \(u=\sum \limits _{n\ge 1} b_n\rho ^n.\) This, definitions of \(\alpha \) and \(\rho \) imply the expansion of \((-e(\mu ))^{1/4}.\)

Case \(2n_o+d=9.\) In this case by (A.3) and (3.11)

$$\begin{aligned} (\mu - \mu _o)\left( c_9^4 + c_9^4\sum \limits _{n\ge 1} \mu _o^{-n}(\mu - \mu _o)^n\right) = \alpha ^4 \left( 1 + \sum \limits _{n\ge 1}a_n\alpha ^n \right) , \end{aligned}$$
(3.14)

where \(\{a_n\}\subset {\mathbb {R}}\) and \(c_9:=(\mu _o^2{\widehat{c}}_v)^{-1/4}.\) Thus, for sufficiently small and positive \(\mu -\mu _o\) using the Taylor series of \((1+x)^{\pm 1/4}\) at \(x=0,\) this equation can also be represented as

$$\begin{aligned} \alpha = \rho \left( c_9 + \sum \limits _{n\ge 1} {\tilde{b}}_n\rho ^{4n}\right) \left( 1 + \sum \limits _{n\ge 1}{\tilde{a}}_n\alpha ^n\right) , \end{aligned}$$

where \(\rho := (\mu - \mu _o)^{1/4}.\) Now setting \(\alpha = \rho (c_9+ u)\) in (3.14) we get

$$\begin{aligned} u=\sum \limits _{n,m\ge 1} {\tilde{c}}_{n,m}\rho ^n(c_9+u)^m, \end{aligned}$$

and the expansion of \((-e(\mu ))^{1/4}\) follows as in the case of \(2n_o+d=7.\)

(b) Suppose that d is even. In view of the expansion (A.3) of \(\mathfrak {l}_f\), in this case, (3.4) is reduced to the inverting the equation

$$\begin{aligned} \mu = \frac{\alpha ^l}{g(\alpha ) + h(\alpha ) \ln \alpha }, \end{aligned}$$
(3.15)

where \(\alpha :=(-e)^{1/2},\) \(l\in {\mathbb {N}}_0,\) and g and h are analytic around \(\alpha =0.\) Presence of \(\ln \alpha \) implies that unlike the case of odd dimensions, \(\alpha \) is not necessarily analytic with respect to \(\mu ^s.\) Therefore, we need to introduce new variables dependent on \(\ln \mu \) to reduce the problem to the Implicit Function Theorem.

Case \(2n_o+d=2.\) By (A.4), in this case for \(c_2:=\pi c_v/8\)

$$\begin{aligned} l=1,\qquad g(\alpha )=c_2 + \sum \limits _{n\ge 1} a_n\alpha ^n,\qquad h(\alpha ) =\sum \limits _{n\ge 1} b_n\alpha ^{2n}. \end{aligned}$$

Hence, setting

$$\begin{aligned} \alpha =\mu (c_2 + u) \end{aligned}$$
(3.16)

and \(\tau = -\mu \ln \mu \) we represent (3.15) as

$$\begin{aligned}&F(u,\mu ,\tau ):=u - \sum \limits _{n\ge 1} a^n\mu ^n(c_2+u)^n&+ \ln (c_2+u)\sum \limits _{n\ge 1} b^n\mu ^n(c_2+u)^n\\&\quad -\tau \sum \limits _{n\ge 1} b^n\mu ^{n-1}(c_2+u)^n=0, \end{aligned}$$

where F is analytic around (0, 0, 0),  \(F(0,0,0)=0,\) \(F_u(0,0,0)=1.\) Hence, by the Implicit Function Theorem, there exists a unique real-analytic function \(u=u(\mu ,\tau )\) given by the convergent series \(u(\mu ,\tau ) = \sum \nolimits _{n+m\ge 1,n,m\ge 0} {\tilde{c}}_{n,m}\mu ^n\tau ^m\) for sufficiently small \(|\mu |\) and \(|\tau |,\) which satisfies \(F(u(\mu ,\tau ),\mu ,\tau )\equiv 0.\) Inserting u in (3.16) we get the expansion of \(\alpha =(-e)^{1/2}.\)

Case \(2n_o+d=4.\) In this case, by (A.4) for \(c_4:=8/ c_v\)

$$\begin{aligned} l=0,\qquad g(\alpha )=\sum \limits _{n\ge 0} a_n\alpha _n,\qquad h(\alpha ) = -c_4 + \sum \limits _{n\ge 1} b_n\alpha ^{2n}. \end{aligned}$$

Letting \(\alpha = e^{-\frac{1}{c_4\mu }}(c+u),\) where \(c= e^{a_0/c_4}>0,\) we represent (3.15) as

$$\begin{aligned} \ln (c+u) - b_0 =&\frac{1}{\mu }\,e^{-\frac{1}{c_4\mu }} \sum \limits _{n\ge 1} a^ne^{-\frac{n-1}{c_4\mu }} (c+u)^n\nonumber \\ +&\ln (c+u)\sum \limits _{n\ge 1} b^ne^{-\frac{n}{c_4\mu }}(c+u)^n -\sum \limits _{n\ge 1} a^ne^{-\frac{n}{c_4\mu }}(c+u)^n=0. \end{aligned}$$
(3.17)

Writing \(\tau :=\frac{1}{\mu }\,e^{-\frac{1}{c_4\mu }}\) so that \(e^{-\frac{1}{c_4\mu }} = \mu \tau ,\) (3.17) is represented as

$$\begin{aligned} F(u,\mu ,\tau ):=&\ln (c+u) - b_0 -\mu \sum \limits _{n\ge 1} a^n\mu ^{n-1}\tau ^{n-1} (c+u)^n\\&-\ln (c+u)\sum \limits _{n\ge 1} b^n\mu ^n\tau ^n(c+u)^n +\sum \limits _{n\ge 1} a^n\mu ^n\tau ^n(c+u)^n=0, \end{aligned}$$

where F is analytic around (0, 0, 0),  \(F(0,0,0)=0,\) and \(F_u(0,0,0)=\frac{1}{c}>0.\) Thus, by the Implicit Function Theorem, for \(|\mu |,\) \(|\tau |\) and |u| small there exists a unique real analytic function \(u=u(\mu ,\tau )\) given by the convergent series \(u=\sum \limits _{n+m\ge 1,n,m\ge 0} {\tilde{c}}_{n,m}\mu ^n\tau ^m\) such that \(F(u(\mu ,\tau ),\mu ,\tau )\equiv 0.\) Since \(\tau = \frac{1}{\mu }e^{-\frac{1}{c_4\mu }},\) this implies

$$\begin{aligned} \alpha = e^{-\frac{1}{c_4\mu }}(c+u) = ce^{-\frac{1}{c_4\mu }} + \sum \limits _{n+m\ge 1,n,m\ge 0} {\tilde{c}}_{n,m}\mu ^{n+1}\left( \frac{1}{\mu }e^{-\frac{1}{c_4\mu }}\right) ^{m+1}. \end{aligned}$$

Case \(2n_o+d=6.\) In this case, by (A.4), for \(c_6:=8/(\pi c_v\mu _o^2)\)

$$\begin{aligned} l=0,\qquad g(\alpha )=\frac{1}{\mu _o} -\frac{1}{c_6\mu _o^2} \left( \alpha + \sum \limits _{n\ge 2} a_n\alpha ^n\right) ,\qquad h(\alpha ) = \frac{1}{c_6\mu _o^2} \sum \limits _{n\ge 1} b_n\alpha ^{2n}, \end{aligned}$$

and hence, (3.15) is represented as

$$\begin{aligned} \frac{1}{\mu } -\frac{1}{\mu _o} = \frac{1}{c_6\mu _o^2}\left( \alpha +\sum \limits _{n\ge 2} a_n\alpha ^n + \ln \alpha \sum \limits _{n\ge 1} b_n\alpha ^{2n}\right) , \end{aligned}$$

or equivalently, by (3.11),

$$\begin{aligned} \alpha = c_6(\mu - \mu _o) \sum \limits _{n\ge 0} \left( \frac{\mu - \mu _o}{\mu _o}\right) ^n - \sum \limits _{n\ge 2} a_n\alpha ^n -\ln \alpha \sum \limits _{n\ge 1} b_n\alpha ^{2n}. \end{aligned}$$
(3.18)

Recalling the definitions of \(\tau \) and \(\theta \) in (2.8), setting \(\alpha = \tau ^2\,(c_6+u),\) we represent (3.18) as

$$\begin{aligned} F(u,\tau , \theta ):= u&-c_6\sum \limits _{n\ge 1}\frac{\tau ^{2n}}{\mu _o^n}- \sum \limits _{n\ge 2} a_n\tau ^{2n-2}(c_6+u)^n\nonumber \\&- \ln (c_6+u) \sum \limits _{n\ge 1} b_n\tau ^{4n}(c_6+u)^{2n} - \theta \sum \limits _{n\ge 1} b_n\tau ^{4n-4}(c_6+u)^{2n}=0, \end{aligned}$$

where F is real-analytic around (0, 0, 0),  \(F(0,0,0)=0\) and \(F_u(0,0,0)=1,\) and F is even in \(\tau .\) Thus, by the Implicit Function Theorem, for |u|,  \(|\tau |\) and \(|\theta |\) small there exists a unique real analytic function \(u=u(\tau ,\theta ),\) even in \(\tau ,\) given by the convergent series \(u=\sum \limits _{n+m\ge 1,n,m\ge 0} {\tilde{c}}_{n,m}\tau ^{2n}\theta ^m\) such that \(F(u(\tau ,\theta ),\tau ,\theta )\equiv 0.\) Thus,

$$\begin{aligned} \alpha = \tau ^2\,(c_6+u) = c_6\sigma + \sum \limits _{n+m\ge 1,n,m\ge 0} {\tilde{c}}_{n,m}\tau ^{2n+2}\theta ^m. \end{aligned}$$

Case \(2n_o+d=8.\) By (A.4), for \(c_8:=[8/c_v\mu _o^2]^{-1/2},\)

$$\begin{aligned} l=0,\qquad g(\alpha )= \frac{1}{\mu _o^2c_8^2}\sum \limits _{n\ge 2} a_n\alpha ^n,\qquad h(\alpha ) =\frac{1}{\mu _o^2c_8^2}\left( \alpha ^2 + \sum \limits _{n\ge 2} b_n\alpha ^{2n}\right) , \end{aligned}$$

thus, as in the case of \(2n_o+d=6,\) (3.15) is represented as

$$\begin{aligned} c_8^2(\mu - \mu _o) \sum \limits _{n\ge 0} \left( \frac{\mu - \mu _o}{\mu _o}\right) ^n = \alpha ^2\ln \alpha +\ln \alpha \sum \limits _{n\ge 2} b_n\alpha ^{2n}+\sum \limits _{n\ge 2} a_n\alpha ^n. \end{aligned}$$
(3.19)

For \(\tau ,\) \(\sigma \) and \(\eta \) given in (2.8) set \(\alpha = \tau \sigma (c_8+u)\) and represent (3.19) as

$$\begin{aligned} 2c_8u+ u^2 =&c_8^2\sum \limits _{n\ge 1} \frac{\tau ^{2n}}{\mu _o^n} + \sum \limits _{n\ge 2}a_n \tau ^{n-1} \sigma ^{n+1}(c_8+u)^{n+2} \\&-\sum \limits _{n\ge 2}b_n (\tau \sigma )^{2n-2}(c_8+u)^{2n+2}\\&+ \left( \sigma ^2\ln (c_8+u) -\frac{\eta }{2} \right) \left( (c_8+u)^2+\sum \limits _{n\ge 2}b_n (\tau \sigma )^{2n-2}(c_8+u)^{2n+2}\right) . \end{aligned}$$

This equation is represented as \( F(u,\tau ,\sigma ,\eta )=0, \) where F is real-analytic in a neighborhood of (0, 0, 0, 0),  \(F(0,0,0,0)=0\) and \(F_u(0,0,0,0) =2c_8>0.\) Hence, for |u|,  \(|\tau |,\) \(|\sigma |\) and \(|\eta |\) small, by the Implicit Function Theorem, there exists a unique real-analytic function \(u=u(\tau ,\sigma ,\eta )\) given by the convergent series \(u=\sum \limits _{n+m+k\ge 1,n,m,k\ge 0} {\tilde{c}}_{n,m,k}\tau ^n\sigma ^m\mu ^k\) such that \(F(u(\tau ,\sigma ,\eta ),\tau ,\sigma ,\eta )\equiv 0.\) Thus,

$$\begin{aligned} \alpha = \tau \sigma (c_8+u) =c_8\tau \sigma + \sum \limits _{n+m+k\ge 1,n,m,k\ge 0} {\tilde{c}}_{n,m,k}\tau ^{n+1}\sigma ^{m+1}\eta ^k. \end{aligned}$$

Case \(2n_o+d\ge 10.\) By (A.4) for \(c_{10}:=(\mu _o^2{\widehat{c}}_v)^{-1/2},\)

$$\begin{aligned} l=0,\qquad g(\alpha )= \frac{1}{\mu _o} + {\widehat{c}}_v \alpha ^2 + \sum \limits _{n\ge 2} a_n\alpha ^{n+2},\qquad h(\alpha ) =\sum \limits _{n\ge 2} b_n\alpha ^{2n}, \end{aligned}$$

and as in the case of \(2n_o+d=6,\) (3.15) is represented as

$$\begin{aligned} \frac{\mu - \mu _o}{\mu _o^2} \sum \limits _{n\ge 0} \left( \frac{\mu - \mu _o}{\mu _o}\right) ^n = {\widehat{c}}_v \alpha ^2 + \sum \limits _{n\ge 2} a_n\alpha ^{n+2}+ \ln \alpha \sum \limits _{n\ge 2} b_n\alpha ^{2n}. \end{aligned}$$
(3.20)

Recalling the definitions of \(\tau \) and \(\theta \) in (2.8), we set \(\alpha =\tau (c_{10} +u).\) Then (3.20) is represented as

$$\begin{aligned} F(u,\tau ,\theta ):=&2c_{10}u + u^2 - c_{10}^2\sum \limits _{n\ge 1} \frac{\tau ^{2n}}{\mu _o^n} + \sum \limits _{n\ge 2}a_n \tau ^n (c_{10}+u)^{n+2}\\&- \theta \sum \limits _{n\ge 2}b_n \tau ^{2n-4}(c_8+u)^{2n} + \ln (c_{10}+u)\sum \limits _{n\ge 2}b_n \tau ^{2n-2}(c_8+u)^{2n}=0, \end{aligned}$$

where F is analytic at (0, 0, 0),  \(F(0,0,0)=0\) and \(F_u(0,0,0)=2c_{10}>0.\) Thus, by the Implicit Function Theorem, for |u|,  \(|\tau |\) and \(|\theta |\) small there exists a unique real-analytic function \(u=u(\tau ,\theta )\) given by the convergent series \(u=\sum \limits _{n+m\ge 1,n,m\ge 0}{\tilde{c}}_{n,m}\tau ^n\theta ^n\) such that \(F(u(\tau ,\theta ),\tau ,\theta )\equiv 0.\) Then

$$\begin{aligned} \alpha = \mu (c_{10} +u) = c_{10}\mu + \sum \limits _{n+m\ge 1,n,m\ge 0}{\tilde{c}}_{n,m}\mu ^{n+1}\theta ^n. \end{aligned}$$

Theorem is proved. \(\square \)

Proof of Theorem 2.5

From (3.3) it follows that the map \(p\in {\mathbb {T}}^d\mapsto |v|^2(\vec \pi +p)\) is even. Now the expansions of \(e(\mu )\) at \(\mu =-\mu ^o\) can be proven along the same lines of Theorem 2.4 using Proposition A.2 with \(f=|v|^2\). \(\square \)

Remark 3.3

Let \({\widehat{v}}:{\mathbb {Z}}^d\rightarrow {\mathbb {C}}\) satisfy (H1). Since \({\mathfrak {e}}(\cdot )\) is even,

$$\begin{aligned} \int _{{\mathbb {T}}^d} \frac{|v(p)|^2dp}{{\mathfrak {e}}(p) -z} =\frac{1}{(2\pi )^d} \, \int _{{\mathbb {T}}^d} \frac{f(p)dp}{{\mathfrak {e}}(p) -z}, \end{aligned}$$

where

$$\begin{aligned} \begin{aligned} f(p):=&\left( \sum \limits _{x\in {\mathbb {Z}}^d} {\widehat{v}}_1(x) \cos p\cdot x\right) ^2 + \left( \sum \limits _{x\in {\mathbb {Z}}^d} {\widehat{v}}_2(x) \cos p\cdot x\right) ^2\\&+ \left( \sum \limits _{x\in {\mathbb {Z}}^d} {\widehat{v}}_1(x) \sin p\cdot x\right) ^2 + \left( \sum \limits _{x\in {\mathbb {Z}}^d} {\widehat{v}}_2(x) \sin p\cdot x\right) ^2 \end{aligned} \end{aligned}$$

and \({\widehat{v}}= {\widehat{v}}_1+ i{\widehat{v}}_2\) for some \({\widehat{v}}_1,{\widehat{v}}_2:{\mathbb {Z}}^d \rightarrow {\mathbb {R}}.\) By Lemma 3.1, the unique eigenvalue \(e(\mu )\) of \({ H}_\mu \) solves

$$\begin{aligned} 1-\mu \int _{{\mathbb {T}}^d} \frac{f(p)dp}{{\mathfrak {e}}(p) - e(\mu )} =0. \end{aligned}$$

Since both \(p\in {\mathbb {T}}^d\mapsto f(p)\) and \(p\in {\mathbb {T}}^d\mapsto f(\vec \pi + p)\) are even analytic functions, we can still apply Propositions A.1 and A.2 to find the expansions of \(z\mapsto \int _{{\mathbb {T}}^d} \frac{f(p)dp}{{\mathfrak {e}}(p) - z}\) and thus, repeating the same arguments of the proofs of Theorems 2.4 and 2.5 one can obtain the corresponding expansions of \(e(\mu ).\)

Remark 3.4

When

$$\begin{aligned} |{\widehat{v}}(x)| = O(|x|^{2n_0+d+1})\qquad \hbox { as}\ |x|\rightarrow \infty \end{aligned}$$

for some \(n_0\ge 1,\) in view of Remark A.3, we need to solve equation (3.4) with respect to \(\mu \) using only that left-hand side is an asymptotic sum (not a convergent series). This still can be done using appropriate modification of the Implicit Function Theorem for differentiable functions. As a result, we obtain only (Taylor-type) asymptotics of \(e(\mu ).\)