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DIR A C – C O U L O M B O PE R ATO R S W IT H GE N E R A L C H A R GE DIST RIB U TIO N I. DISTIN G UIS H E D E X T E N SIO N A N D MIN - M A X F O R M U L A S

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M A R I A J . E S T E B A N M AT H IE U L E W I N

É R IC S É R É

DIR A C – C O U L O M B O P E R AT O R S W I T H G E N E R A L C H A R G E

DIS T R I B U T IO N

I. DIS T I N G UIS H E D E X T E N SIO N A N D M I N - M A X F O R M U L A S

O P É R AT E U R S D E DIR A C AV E C

DIS T R I B U T IO N D E C H A R G E A R BI T R A IR E I. E X T E N SIO N DIS T I N G U É E E T

F O R M U L E S D E M I N - M A X

Keywords:Dirac-Coulomb operators, self-adjointness, min-max formulas.

2020Mathematics Subject Classification:81Q05, 47A10, 49J35.

DOI:https://doi.org/10.5802/ahl.106

(*) This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement MDFT No 725528 of M.L.), and from the Agence Nationale de la Recherche (grant agreement molQED).

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Abstract. — This paper is the first of a series where we study the spectral properties of Dirac operators with the Coulomb potential generated by any finite signed charge distribution µ. We show here that the operator has a unique distinguished self-adjoint extension under the sole condition thatµhas no atom of weight larger than or equal to one. Then we discuss the case of a positive measure and characterize the domain using a quadratic form associated with the upper spinor, following earlier works [EL07, EL08] by Esteban and Loss. This allows us to provide min-max formulas for the eigenvalues in the gap. In the event that some eigenvalues have dived into the negative continuum, the min-max formulas remain valid for the remaining ones. At the end of the paper we also discuss the case of multi-center Dirac–Coulomb operators corresponding toµbeing a finite sum of deltas.

Résumé. — Dans ce premier article nous étudions les propriétés spectrales d’un opérateur de Dirac auquel on ajoute le potentiel de Coulomb généré par une distribution de chargeµ quelconque. Nous montrons l’existence d’une unique extension auto-adjointe distinguée, sous la seule condition que µne possède aucun atome de poids supérieur ou égal à un. Ensuite, lorsque la mesureµest positive nous caractérisons le domaine à l’aide d’une forme quadratique pour le spineur haut, suivant une méthode introduite par Esteban et Loss dans [EL07, EL08].

Ceci nous permet de prouver des formules de min-max pour les valeurs propres situées dans le trou spectral. La formule reste valable même dans le cas où certaines des valeurs propres ont plongé dans le spectre continu inférieur. À la fin de l’article nous discutons du cas d’une molécule, ce qui correspond à prendreµégal à une somme finie de deltas.

1. Introduction

Relativistic effects play an important role in the description of quantum electrons in molecules containing heavy nuclei, even for not so large values of the nuclear charge.

Without relativity, gold would have the same color as silver [GAD10], mercury would be solid at room temperature [CPWS13] and batteries would not work [ZEP11]. This is due to the very strong Coulomb forces experienced by the core electrons, which can then attain large velocities of the order of the speed of light.

A proper description of such atoms and molecules is based on the Dirac oper- ator [ELS08, Tha92]. This is an order-one differential operator which has several famous mathematical difficulties, all associated with important physical features.

For instance the spectrum of the free Dirac operator is not semi-bounded which prevents from giving an unambiguous definition of a “ground state” and turns out to be related to the existence of the positron [ELS08]. In addition, the Dirac operator has a critical behavior with respect to the Coulomb potential 1/|x| which gives a bound Z 6 137 on the highest possible charge of atoms in the periodic table, for point nuclei.

This paper is the first in a series where we study the spectral properties of Dirac operators with the Coulomb potential generated by any finite (signed) measure µ representing an external charge:

(1.1) D0µ∗ 1

|x| =−i

3

X

j=1

αjxj +βµ∗ 1

|x|.

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One typical example is when the measure µ describes the M nuclei in a molecule and this corresponds to

µ=

M

X

m=1

αZm δRm

where Rm ∈ R3 and Zm ∈ (0,∞) are, respectively, the positions and charges of theM nuclei, and where α'1/137 is the Sommerfeld fine structure constant. For instance for water (H2O) we have M = 3, Z1 = Z2 = 1 and Z3 = 8. In practice, one should also take into account the Coulomb repulsion between the electrons. In mean-field type models such as Dirac–Fock or Kohn–Sham [ES99], this is described by a nonlinear potential which is often more regular than the nuclear attraction.

This leads us to consider the following class of (signed) measures µ=

M

X

m=1

αZm δRm +µ,e

where the measureµe is more regular (for instance absolutely continuous with respect to the Lebesgue measure).

In this paper, we first quickly recall existing results and then prove the existence of a distinguished self-adjoint extension for operators of the form (1.1), under the sole assumptions that

(1.2) |µ|R3

<∞ and |µ({R})|<1 for all R ∈R3.

In particular we allow an infinite number M = +∞ of atoms but assume that the total nuclear charge is bounded. We follow well established methods for singular Dirac operators [Kat83, Kla80, KW79, Nen76, Nen77, Sch72, Wüs73, Wüs75, Wüs77] but face several difficulties due to the generality of our measure µ. In a second step we consider the particular case of a positive measure (or more generally a measure so that the Coulomb potential µ∗ |x|−1 is bounded from below) and we characterize the domain using a method introduced in [EL07, EL08] and recently generalized in [SST20]. This method allows us to provide min-max formulas for the eigenvalues in the gap (−1,1), following [DES00a, DES00b, DES03, DES06, ELS19, GS99, MM15, Mül16, SST20]. In the event that some eigenvalues have dived into the negative continuum, we prove that the min-max formulas remain valid for the remaining ones.

In a second article [ELS21] we consider the problem of minimizing the first eigen- value with respect to the (non-negative) charge distribution µ at fixed maximal charge ν:

λ1(ν) := inf

µ>0 µ(R3)6ν

λ1 D0µ∗ 1

|x|

!

,

that is, we ask what is the lowest possible eigenvalue of all possible charge distri- butions with µ(R3)6 ν. This problem is indeed our main motivation for studying Dirac operators of the type (1.1) with general measuresµ. We prove in [ELS21] that

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there exists a critical coupling constant(1) 2

π

2 +π2 < ν1 61

such that λ1(ν) > −1 for all 0 6 ν < ν1, that is, the first eigenvalue cannot attain the bottom of the spectral gap if ν1µ(R3) remains positive. In addition, for 0 6 ν < ν1 we prove the existence of a minimizing measure for λ1(ν) and show that it concentrates on a set of Lebesgue measure zero. That the optimal measure is necessarily singular is the main justification for considering general charge distributions.

It is well known that the first eigenvalue of the non-relativistic Schrödinger operator is concave in µ, which implies that

µ>inf0 µ(R3)6ν

λ1 −∆

2 −µ∗ 1

|x|

!

=λ1 −∆ 2 − ν

|x|

!

=−ν2 2 .

We conjecture that a similar equality holds in the Dirac case, which would imply ν1 = 1 andλ1(ν) = √

1−ν2. We mention below some physical implications that the validity of this conjecture would have for the electronic contribution to the potential energy surface of diatomic systems and other molecules.

The paper is organized as follows. In the next section we show that the opera- tor (1.1) has a unique distinguished self-adjoint extension under the assumption (1.2), whereas in Section 3 we discuss the domain and min-max formulas for the eigenvalues under the additional condition thatµ>0. The rest of the paper is then devoted to the proofs of our main results.

2. Distinguished self-adjoint extension for a general charge

In this section we give a meaning to the operator D0µ∗ |x|−1 for the largest possible class of bounded measures µ. But first we need to clarify some notation.

2.1. Notation

We work in a system of units for which m =c=~= 1. The free Dirac operator D0 is given by

(2.1) D0 =−iα·+β = −i

3

X

k=1

αkxk + β,

where α1,α2,α3 and β are Hermitian matrices which satisfy the following anticom- mutation relations:

(2.2)

αkα`+α`αk = 2δk`1, αkβ+βαk = 0,

β2 = 1.

(1)In [ELS21]ν1 is simply denotedν1.

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The usual representation in 2×2 blocks is given by β = I2 0

0 −I2

!

, αk= 0 σk

σk 0

!

(k = 1,2,3), where the Pauli matrices are defined as

σ1 = 0 1 1 0

!

, σ2 = 0 −i i 0

!

, σ3 = 1 0 0 −1

!

.

The operator D0 is self-adjoint with domain H1(R3,C4) and its spectrum is Sp(D0) = (−∞,−1]∪[1,∞) [Tha92].

2.2. Distinguished self-adjoint extension

The study of self-adjoint extensions is a classical subject for Dirac-Coulomb oper- ators. For instance, the one-center Coulomb operator

D0ν

|x|

is known to be essentially self-adjoint on Cc(R3\ {0},C4) for 06ν 6√

3/2, with domain H1(R3,C4) when 06ν <

3/2, whereas it has several possible self-adjoint extensions for ν >

3/2. When √

3/2 < ν < 1, there is a unique extension which is distinguished by the property that its domain is included in the ‘energy space’

H1/2(R3,C4). The domain of the extension is always larger than H1(R3,C4) when ν ∈ [√

3/2,1), with a regularity at the origin which deteriorates when ν increases.

When ν = 1 one can also define a distinguished self-adjoint extension (obtained for instance by taking the limit ν → 1) but its domain is no longer included in H1/2(R3,C4). There is no physically relevant extension for ν >1. This corresponds to the previously mentioned property that we should work under the constraint ν = αZ 6 1 which implies the bound Z 6 137 on the maximal possible (integer) point charge in the periodic table, within Dirac theory.

These relatively simple ODE-type results for the one-center Dirac operator have been generalized in many directions. Investigating how robust the distinguished extension is with regard to perturbations has indeed been the object of many works.

A survey of known results, mainly in the one-center case, may be found for instance in [ELS19, Section 1.3]. A typical result is that Dirac operators in the form

(2.3) DV =D0+V(x) with |V(x)|6 ν

|x|, ν <1

also have a unique distinguished self-adjoint extension, characterized by the property that the domain is included in H1/2(R3,C4). Hence a pointwise bound on V is sufficient, which is rather remarkable for operators which are not semi-bounded. This extension can also be obtained as a norm-resolvent limit by truncating the singularity of the potentialV. Note that the critical caseν= 1 was handled in [EL07] forV >0 but the domain is not necessarily included in the energy space H1/2(R3,C4).

There are fewer results about the multi-center case, which is however as physi- cally important as the atomic case. The intuitive picture is that self-adjointness is

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essentially a local problem at the singularities of the potentials, hence the results should be similar for multi-center Coulomb potentials. Indeed, Nenciu [Nen77] and Klaus [Kla80] have proved that there is a unique distinguished self-adjoint extension forD0+V under the pointwise assumption that

(2.4) |V(x)|6

M

X

m=1

νm

|x−Rm|

with Rm 6= R` for m 6= ` and 0 6 νm < 1 for all m = 1, . . . , M. Note that we can add to V any bounded potential (or even a regular potential in the sense of [Nen76, Nen77]), without changing the domain of self-adjointness. For other results on multi-center Dirac operators, see [BH03, Kar85].

One important tool in these works is the Birman-Schwinger-type formula of the resolvent [Kla80, KW79, Nen76]

(2.5) (D0+Vz)−1

= (D0z)−1−(D0z)−1q|V|(1 +SKz)−1Sq|V|(D0z)−1 where

(2.6) Kz =q|V|(D0z)−1q|V|,

andS = sgn(V). This formula is valid as long as 1−SKz is invertible with bounded inverse, and it can serve to define DV via its resolvent. In the one-center case

|V(x)|6ν|x|−1 we have for z = 0

kK0k6ν

(this was conjectured in [Nen76] and then, proved in [ADV13, Kat83, Wüs77]). This gives the distinguished self-adjoint extension for 06ν <1. In the multi-center case one cannot always use z = 0 since it can be an eigenvalue, when PMj=1νj is large and the nuclei are close to each other. But the set of problematic z’s is at most countable, hence the formula also allows one to define the distinguished self-adjoint extension [Kla80, Nen77].

The above results do not cover the case where V(x) = −µ∗ |x|−1 for general measures µ. Such potentials indeed diverge like µ({R})|xR|−1 at points R∈ R3 where µ({R}) >0, but they can diverge at many other points in space where µis not necessarily a delta. In this paper, we prove the following result, which confirms the intuition that only deltas are problematic with regard to self-adjointness.

Theorem 2.1(Distinguished self-adjoint extension). — Letµbe any finite signed Borel measure onR3, such that

|µ({R})|<1 for all R∈R3. Then the operator

D0µ∗ 1

|x|,

defined first on H1(R3,C4) or on Cc(R3,C4), has a unique self-adjoint extension whose domain is included in H1/2(R3,C4). The functions in the domain D(D0

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µ∗ |x|−1) of the extension have a square-integrable gradient in R3\SKj=1Br(Rj)for all r >0, where R1, . . . , RK ∈R3 are all the points such that |µ({Rj})|>1/2. The operator D0µ∗ |x|−1 is the norm-resolvent limit ofD0µ|x|1 1(|µ∗|x|1 |6n)when

n→ ∞. Its essential spectrum is

SpessD0µ∗ |x|−1= (−∞,−1]∪[1,+∞).

The proof of Theorem 2.1 is provided later in Section 4.

Note that in generalD(D0µ∗ |x|−1) may differ from the domain of the operator D0PKj=1µ({Rj})|x−Rj|−1, because the behavior of µin the vicinity of the nuclei also plays a role.

Although we think that there should be a similar result with a larger space than H1/2(R3,C4) under the weaker condition that|µ({R})|61, we have not investigated this question in the general setting. More about the critical case can be read in Section 3.3 where we investigate the particular case of a measureµ which is a pure sum of deltas, following [ELS19].

One important argument of the proof is to show that the operator 1BR

s

µe∗ 1

|x|

1

|p|12

is compact, for every positive measure µe with no atom. Here we have used the notationp=−i∇andBR for the ball of radiusR centered at the origin. Then, after separating the region about each nucleus from the rest of space, we show that

q|Vµ| 1 D0+is

q|Vµ|

<1

for s large enough, where Vµ =µ∗ |x|−1. This is what is needed to apply Nenciu’s method [Nen76, Corollary 2.1].

3. Domain and min-max formulas for positive measures

By following a method introduced in [EL07, EL08] and further developed in [ELS19, SST20], one can describe the distinguished self-adjoint extension more precisely in the case of a positive measure:

µ>0.

What we really need in this section is that Vµ be bounded from below, but for simplicity we require the positivity of µeverywhere. We use the notation

Vµ=µ∗ 1

|x|

for the Coulomb potential induced byµ.

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3.1. Description of the domain

Following [ELS19], we introduce a new space for the upper component ϕL2(R3,C2) of a four-spinor. We define the following norm

(3.1) kϕkV

µ :=

Z

R3

|σ· ∇ϕ(x)|2 1 +Vµ(x) dx+

Z

R3

|ϕ(x)|2 dx

!1/2

which is well defined onH1(R3,C2) and controlled by the H1–norm since (1 +Vµ)−1 61. We can in fact replace 1 +Vµby any λ+Vµ withλ >0 and we get an equivalent norm. Recall thatVµ >0.

Like in [ELS19] we need to know whether the completionVµ ofH1(R3,C2) for the norm in (3.1) is the same as the largest space given by the conditions

ϕL2R3,C2

, σ· ∇ϕ

(1 +Vµ)1/2L2R3,C2

.

The following answers this question affirmatively.

Theorem 3.1 (The upper-spinor space Vµ). — Let µ > 0 be any finite Borel measure on R3 so that

µ({R})<1 for all R∈R3. We have

(3.2) kϕk2H1/2(R3,C2)

max2,16µ(R3) 6kϕk2V

µ 6kϕk2H1(R3,C2)

for allϕH1(R3,C2). The completion ofH1(R3,C2)for the normk·kVµis a subspace Vµ of H1/2(R3,C2) satisfying the continuous embeddings in (3.2). It coincides with the completion of Cc(R3,C2) for the same norm and is given by

(3.3) Vµ =nϕL2R3,C2

:∃gL2R3,C2

, σ· ∇ϕ= (1 +Vµ)1/2go where σ· ∇ϕis understood in the sense of distributions.

The proof of Theorem 3.1 is provided later in Section 5. The first part of the theorem says that there is a Hardy-type inequality

(3.4)

Z

R3

|σ· ∇ϕ(x)|2 1 +Vµ(x) dx+

Z

R3

|ϕ(x)|2dx>

(−∆)14ϕ2

L2(R3,C2)

max2,16µ(R3),

forϕH1(R3,C2) and all positive measuresµ. The second part says that the space of functions ϕL2(R3,C2) such that (1 +Vµ)−1/2σ· ∇ϕ ∈L2(R3,C2) (this being interpreted as in (3.3)), which could a priori be larger than the completion Vµ, is equal to Vµ. This is an important property for what follows and it allows one to extend the inequality (3.4) to all such functionsϕ. With regard to (3.3), we remark thatVµL1loc(R3) for every Radon measure µ, so that (1 +Vµ)1/2gL1loc(R3,C2) is a distribution whengL2(R3,C2). Moreover, we prove later in Lemma 5.1 that

∇(1 +Vµ)−1/2L2(R3) for everyµ. This implies that (1 +V)−1/2σ· ∇ϕmakes sense as a distribution and, in (3.3), it is then equivalent to requiring that this distribution belongs toL2(R3,C2).

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In the special case of

µ=

M

X

m=1

νmδRm

with 0< νm <1, we have by [ELS19]

Vµ=

(

ϕL2R3,C2

:

Z

R3 M

Y

m=1

|x−Rm|

1 +|x−Rm||σ · ∇ϕ(x)|2 dx <

)

. In other words, the functions in Vµ must be in Hloc1 (R3 \ {R1, . . . , RM},C2) and behave as stated close to the singularities. In general the space Vµ depends on the size and location of the singularities of the potential Vµ, which are not necessarily produced by the atomic part of µ. Recall that the potential V

eµ of the non-atomic partµe ofµ can still diverge in some places, namely at all the pointsR ∈R3 so that

Z

R3

dµ(x)e

|x−R| = +∞.

At each of these points, the norm is affected because 1/(1+Vµ) tends to zero, allowing thereby|σ· ∇ϕ|2 to diverge a bit.

We can now describe the domain of the distinguished self-adjoint extension using the space Vµ.

Theorem 3.2 (Domain of the distinguished self-adjoint extension forµ>0). — Letµ>0be any finite Radon measure on R3 so that

µ({R})<1 for all R∈R3.

Then the domain of the self-adjoint extension from Theorem 3.2 is explicitly given by (3.5) D(D0Vµ) =

(

Ψ = ϕ χ

!

L2R3,C4

:ϕ∈ Vµ, D0Ψ−VµΨ∈L2R3,C4

)

where in the last conditionD0ΨandVµΨare understood in the sense of distributions.

Moreover, this extension is the unique one included in Vµ×L2(R3,C2). We have D(D0Vµ)⊂ Vµ× VµH1/2R3,C4

.

In addition, the Birman–Schwinger principle holds: λ∈ (−1,1) is an eigenvalue of D0Vµ if and only if 1is an eigenvalue of the bounded self-adjoint operator

Kλ =qVµ 1 D0λ

qVµ.

The condition µ>0 is used to have Vµ>0 which simplifies the definition of the space Vµ. If Vµ is bounded-below, then the exact same result is valid with 1 +Vµ replaced byC+Vµ with a large enough constant C everywhere.

The proof of Theorem 3.2 is provided below in Section 6.

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3.2. Min-max formulas for the eigenvalues

Related to the above characterization of the domain are min-max formulas for eigenvalues [DES00a, DES00b, DES03, DES06, ELS19, GS99, MM15, Mül16, SST20].

Our main result is the following

Theorem 3.3 (Min-max formulas). — Letµ>0be any finite non-trivial Radon measure on R3 so that

µ({R})<1 for all R ∈R3. Define the min-max values

(3.6) λ(k) := inf

W subspace ofF+ dim W=k

sup

Ψ(WF)\{0}

hΨ,(D0Vµ) Ψi

kΨk2 , k >1, where F is any chosen vector space satisfying

CcR3,C4

FH1/2R3,C4

,

and

F+ :=

(

Ψ = ϕ 0

!

F

)

, F:=

(

Ψ = 0 χ

!

F

)

.

Then we have

(i) λ(k) is independent of the chosen spaceF; (ii) λ(k) ∈[−1,1) for all k;

(iii) it is a non-decreasing sequence converging to 1:

(3.7) lim

k→∞λ(k) = 1.

Letk0 be the first integer so that

λ(k0) >−1.

Then(λ(k))k>k0 are all the eigenvalues of D0Vµ in non-decreasing order, repeated according to their multiplicity, which are larger than −1:

Sp D0µ∗ 1

|x|

!

∩(−1,1) =nλ(k0), λ(k0+1),· · ·o. Finally, if

(3.8) µ(R3)6 2

π/2 + 2/π '0.9, then we have λ(1) >0 and there is no eigenvalue in (−1,0).

The min-max formula (3.6) for the eigenvalues ofD0Vµ is based on a decompo- sition of the four-component wavefunction into its upper and lower spinors,

Ψ = ϕ χ

!

.

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That one can obtain the eigenvalues by maximizing overχand minimizing overϕwas suggested first in the Physics literature by Talman [Tal86] and Datta–Devaiah [DD88].

The min-max is largely based on the fact that the energyhΨ,(D0Vµ)Ψiis concave inχ and more or less convex in ϕ (up to finitely many directions corresponding to the indicesk < k0). This approach is reminiscent of the Schur complement formula, which is an important ingredient in the proof. Indeed, writing the eigenvalue equation in terms ofϕ andχ, solving the one for χ and inserting it in the equation of ϕ, one formally finds that

(3.9) −σ· ∇ 1

1 +λ+Vµσ· ∇+ 1−λVµ

!

ϕ= 0.

The formal operator on the left is associated with the quadratic form (3.10) qλ(ϕ) :=

Z

R3

|σ· ∇ϕ|2 1 +λ+Vµdx+

Z

R3

(1−λVµ)|ϕ|2

and most of the work is to show that it is bounded from below, and equivalent to the Vµ–norm squared, up to addition of a constant. This allows one to give a meaning to the operator in (3.9) by means of the Riesz–Friedrichs method, hence to transform the (strongly indefinite) Dirac eigenvalue problem into an elliptic eigenvalue problem, nonlinear in the parameterλ. In the proof of Theorems 3.2 and 3.3 we explain how to relate any information on the operatorKz in (2.6) to that on the quadratic form qλ and we then directly apply [DES00a, ELS19, SST20]. Note finally that condition (3.8) is directly related to an inequality due to Tix [Tix98] used in the proof.

3.3. Application to (critical and sub-critical) multi-center potentials Let us now discuss the special case of a positive measure made of a finite sum of deltas,

µ=

M

X

m=1

νmδRm, 0< νm 61,

which describes the nuclear density of a molecule. We always assume that the Rm

are all distinct from each other.

When ¯ν := maxνm < 1, Theorem 2.1 provides the self-adjointness of the corre- sponding multi-center Dirac–Coulomb operator. This was proved before in [Kla80, Nen77]. Theorem 3.2 gives the domain in terms of the spaceVµ which, as we have already mentioned, is equal to

Vµ=

(

ϕL2R3,C2

:

Z

R3 M

Y

m=1

|x−Rm|

1 +|x−Rm||σ· ∇ϕ(x)|2 dx <

)

. This is proved by localizing about each nucleus. One can also give a simple explicit lower bound on the quadratic form qλ in terms of the νm and of the Rm, which remains valid in the critical case maxνm= 1.

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Lemma 3.4 (Lower bound onqλ for multi-center). — Let µ=PMm=1νmδRm with 06νm 61and where the Rm are all distinct. Then we have

qλ(ϕ)>1−ν¯2

Z

R3

|σ· ∇ϕ|2

2 +Vµ dx− 2λ+2(M −1)¯ν

d + κ

d2(1 +λ)

!Z

R3

|ϕ|2dx for every ϕH1(R3,C2), where ν¯= max(νm), d= maxk6=`|RkR`| andκ > 0is a universal constant.

By arguing as in [EL07, EL08, ELS19], this allows us to find a self-adjoint extension distinguished from the property that its domain satisfies

D(D0Vµ)⊂ Wµ×L2R3,C2

where Wµ is the space obtained after closing the quadratic form qλ. This space is larger thanVµwhen max(νm) = 1. A simple localization as in the proof of Lemma 3.4 allows to apply the results of [ELS19] and deduce that

(3.11) Wµ =

ϕL2R3,C2

:

Z

R3

σ· ∇QMm=1|x−Rm|ϕ(x)2

QM

m=1|x−Rm|(1 +|x−Rm|)dx <

. Arguing like in [ELS19], one can prove that the distinguished self-adjoint extension is the norm-resolvent limit of the operators obtained after truncating the potential or after decreasing the critical nuclear charges. One can indeed treat any potential V so that

06V 6Vµ

but then the space Wµ has to be modified accordingly. The arguments are exactly the same as in [ELS19].

In chemistry one is interested in thepotential energy surface which, by definition, is the graph of the first eigenvalue of the multi-center Dirac-Coulomb operator, seen as a function of the locations of the nuclei at fixed νm and including the nuclear repulsion:

(R1, . . . , RM)7→λ1 D0

M

X

m=1

νm

|x−Rm|

!

+ X

16m < `6M

νmν`

|RmR`|.

The following is an extension of similar results proved before for M = 2 in [BH03, HK83, Kla80].

Theorem 3.5 (Molecular case). — Assume that R1, . . . , RM are M distinct points in R3, and that µ=PMm=1νmδRm with 0< νm <1. Let

λ1 D0

M

X

m=1

νm

|x−Rm|

!

be the first min-max level as in (3.6). Then,

(i) the map (R1, . . . , RM)7→λ1(D0PMm=1 |x−Rνm

m|) is a continuous function on the open set Ωdefined as

Ω =

(

(R1, . . . , RM)∈R3

M

: λ1 D0

M

X

m=1

νm

|x−Rm|

!

>−1

)

.

(13)

(ii) Moreover,

(3.12) lim

mink6=`|Rk−R`|→ ∞λ1 D0

M

X

m=1

νm

|x−Rm|

!

=q1−maxνm2. (iii) If in addition PMm=1νm <2(π/2 + 2/π)−1 then

(3.13) lim

maxk6=`|Rk−R`| →0λ1 D0

M

X

m=1

νm

|x−Rm|

!

=

v u u u t1−

M

X

m=1

νm

!2

.

The part (iii) of the theorem actually holds for PMm=1νm < ν1 where ν1 is a constant defined in the second part [ELS21] of this work (denoted there simply by ν1). If ν1 = 1 as we believe, then (iii) holds for allPMm=1νm <1. In [BH03] the result is claimed for M = 2 and ν1 = ν2 <1/2 but we could not fill all the details of the argument of the proof of [BH03, Lemma 3.1].

For M = 2 it is a famous conjecture that the energy of a diatomic molecule is always greater than the single atom with the two nuclei merged. This property was conjectured for two-atoms Dirac operators by Klaus in [Kla80, p. 478] and by Briet–

Hogreve in [BH03, Section 2.4]. Numerical simulations from [ASI+10, McC13] seem to confirm the conjecture for M = 2, even for large values of the nuclear charges.

We make the stronger conjecture that the same holds for any M. Conjecture 3.6. — We have

(3.14) λ1 D0

M

X

m=1

νm

|x−Rm|

!

>λ1

D0

M

P

m=1

νm

|x|

=

v u u u t1−

M

X

m=1

νm

!2

for all M >2, all R1, . . . , RM ∈R3 and allνm >0so that PMm=1νm 61.

In [ELS21] we discuss a stronger conjecture which implies Conjecture 3.6. Note that Conjecture 3.6 has been proved in the non-relativistic case, as recalled in the introduction.

4. Proof of Theorem 2.1

The proof relies on two preliminary lemmas which we first state and show, before we turn to the actual proof of the theorem.

Loosely speaking, the first lemma asserts that g(x)|p|−sf(x) is compact when f and g have disjoint supports. Recall that everywhere p=−i∇.

Lemma 4.1 (Compactness for disjoint supports). — LetfL2(Rd)with support in a compact set B ⊂ Rd. Let Ω be a (bounded or unbounded) set in Rd so that d(B,Ω)>0 and let gL2loc(Rd) supported on Ω, such that

Z

|g(x)|2

(1 +|x|)2(d−s) dx <,

(14)

where 0< s < d. Then the operator

K =g(x) 1

|p|sf(x) is compact and its norm can be estimated by

(4.1) kKk6CkfkL2(B)

Z

|g(x)|2

|x|2(d−s)dx

!1

2

.

where C only depends on s, on the dimension, ond(B,Ω) and onsupxB|x|.

Proof. — The kernel of the operator K is given by K(x, y) = κ1(x)g(x)f(y)

|x−y|d−s

for some constant κ. Since the two functions f and g have supports at a finite distance from each other, we have|x−y|>d(B,Ω)>0 and the denominator never vanishes. Since B is compact, we even have |x−y|>|x| −R whereR = maxyB|y|.

In particular, we conclude that |x−y| > c(|x|+ 1) for all x ∈ Ω and all yB.

Therefore, the kernel of K is pointwise bounded by

|K(x, y)|6 κ cd−s

|g(x)|

(1 +|x|)d−s|f(y)|.

The right side is a rank-one operator which is bounded under the condition that fL2 and g(1 +|x|)s−dL2. This shows that K is bounded as in (4.1).

To prove the compactness of K we can approximatef and g by functions in Cc and use classical compactness results. But we can also argue directly as follows. Let un*0 be any sequence converging weakly to 0 withkunkL2 = 1. We remark that

(Kun)(x) = κ g(x)

Z

B

f(y)un(y)

|x−y|d−sdy

converges to 0 almost everywhere, since y 7→ f(y)|xy|s−d belongs to L2 for all x∈Ω. In addition, we have the pointwise bound

|(Kun)(x)|6 κ cd−s

|g(x)|

(1 +|x|)d−skfkL2(B)

which, by the dominated convergence theorem, implies thatkKunk →0.

Using Lemma 4.1 we can show the following result.

Lemma 4.2 (Local compactness in the absence of atoms). — Let µe > 0 be a finite Radon measure onR3, with no atom. Then

1BR

s

µe∗ 1

|x|

1

|p|12 is a compact operator for every finite R >0.

(15)

Note that the operator qV

eµ|p|−1/2 is not compact since at infinity it essentially behaves like

q

µ(e R3)|x|−1/2|p|−1/2

which is not compact. The characteristic function1BR is really necessary. In addition, the corresponding result cannot hold for a measure which comprises some deltas, due to the lack of compactness at the corresponding centers.

Proof of Lemma 4.2. — First we write µe =µe1BN+µe1R3\BN where BN is the ball of radiusN, and remark that

(4.2)

s

µe∗ 1

|x| −

s

(µe1BN)∗ 1

|x|

! 1

|p|12

6

s

µe1R3\BN

∗ 1

|x|

1

|p|12

6

rπ

2µe(R3\BN).

The first inequality holds because qVµqVµ1 6qVµ2 pointwise, for µ=µ1+µ2. The second uses Kato’s inequality

(4.3) 1

|x| 6 π 2|p|

which implies that

s

µ∗ 1

|x|

1

|p|12

=

1

|p|12

s

µ∗ 1

|x|

6

rπ 2

q

µ(R3)

for every bounded measure µ. The right side of (4.2) tends to zero when N → ∞ and this shows that we may assume for the rest of the proof that µe has compact support.

For r > 0, let us consider two tilings of the whole space R3 with cubes Cj = 3r(j+[−1/2,1/2)3) andCk0 =r(k+[−1/2,1/2)3) of side length 3randr, respectively, where j, k ∈Z3. For everyk, we call jk the index of the large cube Cjk of which Ck0 is exactly at the center. Letε >0. By compactness of the support ofµe and the fact that it has no atom, we can find r >0 so that µ(Ce j)6ε for every j.

We then write 1

|p|121BR µe∗ 1

|x|

! 1

|p|12 =X

k

1

|p|121BR∩Ck0 µe1Cjk +1R3\Cjk

∗ 1

|x|

! 1

|p|12. Recall that the sum is finite. The sets Ck0 and R3\Cjk are at a distance at least equal tor from each other. Then

1Ck0 µe1R3\Cjk ∗ 1

|x|

!

6 c r.

In particular this function is in Lp(Ck0) for all 16p6∞ and the operator 1

|p|121BR∩Ck0 µe1R3\Cjk ∗ 1

|x|

! 1

|p|12

(16)

is compact. This is true for instance because|p|−1/2f(x)|p|−1/2 is compact under the condition that fL3(R3), by Cwikel’s inequality [Sim05]. Hence, at this step we have written

1

|p|121BR µe∗ 1

|x|

! 1

|p|12 =X

k

1

|p|121BRCk0 µe1Cjk ∗ 1

|x|

! 1

|p|12 +K1 where K1 is compact.

Next, for everyk we insert another localization as follows 1

|p|121Ck0 µe1Cjk ∗ 1

|x|

! 1

|p|12

=1Cjk +1R3\Cjk

1

|p|121Ck0 µe1Cjk ∗ 1

|x|

! 1

|p|12

1Cjk +1R3\Cjk

.

The operator

1R3\Cjk

1

|p|121Ck0

s

µe1Cjk ∗ 1

|x|

is compact, by Lemma 4.1. Indeed, we have 1Ck0 µe1Cjk ∗ 1

|x|

!

=1Ck0 µe1Cjk ∗1Cjk+Ck0

|x|

!

L1(Ck0) so that its square root is in L2(Ck0), and

Z

R3\Cjk

dx

(1 +|x|)5 <∞.

This proves that 1

|p|121BR µe∗ 1

|x|

! 1

|p|12 =X

k

1Cjk

1

|p|121BR∩Ck0 µe1Cjk ∗ 1

|x|

! 1

|p|121Cjk +K2 where K2 is compact. By Kato’s inequality (4.3) the first operator is bounded above as follows:

X

k

1Cjk

1

|p|121BR∩Ck0 µe1Cjk ∗ 1

|x|

! 1

|p|121Cjk

6 π 2

X

k: CkBR6=

1Cjkµ(Ce jk)6επ 2

X

k: CkBR6=

1Cjk 6 27π 2 ε.

Here we have used that µ(Ce j) 6 ε for every j by our choice of r. Therefore our initial operator is the norm-limit of a sequence of compact operators and it must be

compact.

Now we can provide the

Proof of Theorem 2.1. — Our goal is to show that

(4.4) lim sup

|s| → ∞

q|Vµ| 1 D0+is

q|Vµ|

6 max

RR3

|µ({R})|<1,

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