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Interpolation inequalities and spectral estimates for magnetic operators

Jean Dolbeault

http://www.ceremade.dauphine.fr/∼dolbeaul Ceremade, Université Paris-Dauphine

May 14, 2018

IML workshop onEigenvlaues and inequalities(14-18/5/2018) Joint work with M.J. Esteban, A. Laptev & M. Loss

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Magnetic interpolation in the Euclidean space

Outline

Magnetic rings

BResults: a one-dimensional magnetic interpolation inequality BConsequences: Keller-Lieb-Thirring estimates,

Bohm-Aharonov magnetic fields and a new Hardy inequality inR2

Interpolation inequalities and spectral estimates for magnetic operators in dimensions 2 and 3

BTheoretical results

BEstimates, numerics and a conjecture

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space

Preliminaries: a simple interpolation on the circle

On (−π, π]≈S13s, let us consider the uniform probability measure dσ= ds/(2π) and denote bykψkLp(S1)the corresponding Lp norm The inequality

0k2L2(S1)+αkψk2L2(S1)µ0,p(α)kψk2Lp(S1) (1) holds for some concave functionα7→µ0,p(α) on (0,+∞)

Lemma

If p >2 and0< α≤1/(p−2), thenµ0,p(α) =α

If p=−2 andα= 1/(p−2) =−1/4, then µ0,p(−1/4) =−1/4 In both cases, equality achieved only by constant functions

Casep=−2(Exner, Harrell, Loss, 1998)):

0k2L2(S1)+1

4kψk2Lp(S1)≥1

4kψk2L2(S1)

Casep >2: Bakry-Emery method applies toKolmogorov’s inequality

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space

Carré du champ method

LetF[u] :=ku0k2L2(S1)+p−21 kuk2L2(S1)− kuk2Lp(S1)

and consider a positive solution of the parabolic equation

∂u

∂t =u00+ (p−1)|u0|2 u

Ifp=−2 (new application of thecarré du champmethod)

d

dtF[u(t,·)] = Z π

−π

|u00|2− |u0|2

| {z }

≥0(Poincaré) +

Z π

−π

|u0|4 u2

Ifp >1,p6= 2, the method is well known(Bakry, Emery, 85)

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

Magnetic rings

BA magnetic interpolation inequality onS1: withp >2 kψ0+i a ψk2L2(S1)+αkψk2L2(S1)µa,p(α)kψk2Lp(S1)

BConsequences

A Keller-Lieb-Thirring inequality

A new Hardy inequality for Bohm-Aharonov magnetic fields inR2

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

Magnetic flux, a reduction

Assume thata:R→Ris a 2π-periodic function such that its restriction to (−π, π]≈S1 is in L1(S1) and define the space

Xa:=

ψCper(R) : ψ0+i a ψ∈L2(S1)

A standard change of gauge (see e.g.(Ilyin, Laptev, Loss, Zelik, 2016))

ψ(s)7→ei Rs

−π(a(s)−¯a) dσ

ψ(s) where ¯a:=Rπ

−πa(s) dσis themagnetic flux, reduces the problem to a is a constant function

For anyk∈Z,ψbys7→eiksψ(s) shows thatµa,p(α) =µk+a,p(α) a∈[0,1]

µa,p(α) =µ1−a,p(α) because

0+i a ψ|2=|χ0+i(1−a)χ|2=

ψ0i a ψ

2 ifχ(s) =e−isψ(s) a∈[0,1/2]

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

Optimal interpolation

We want to characterize theoptimal constant in the inequality kψ0+i a ψk2L2(S1)+αkψk2L2(S1)µa,p(α)kψk2Lp(S1)

written for anyp >2,α∈(−a2,+∞),ψXa

µa,p(α) := inf

ψ∈Xa\{0}

Rπ

−π0+i a ψ|2+α|ψ|2 dσ kψk2Lp(

S1)

p=−2 = 2d/(d−2) withd= 1(Exner, Harrell, Loss, 1998) p= +∞(Galunov, Olienik, 1995) (Ilyin, Laptev, Loss, Zelik, 2016) limα→−a2µa,p(α) = 0 (JD, Esteban, Laptev, Loss, 2016)

Using a Fourier seriesψ(s) =P

k∈Zψkeiks, we obtain that kψ0+i a ψk2L2(S1)=X

k∈Z

(a+k)2k|2a2kψk2L2(S1)

ψ7→ kψ0+i a ψk2L2(S1)+αkψk2L2(S1)is coercive for any α >a2

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

An interpolation result for the magnetic ring

Theorem

For anyp >2,a∈R, andα >a2a,p(α) is achieved and

(i) if a∈[0,1/2]anda2(p+ 2) +α(p−2)≤1, thenµa,p(α) =a2+α and equality in (1) is achieved only by the constant functions (ii) if a∈[0,1/2]anda2(p+ 2) +α(p−2)>1, thenµa,p(α)< a2+α

and equality in (1) is not achieved by the constant functions Ifα >a2,a7→µa,p(α)is monotone increasing on(0,1/2)

-0.2 -0.1 0.1 0.2 0.3 0.4

0.1 0.2 0.3 0.4 0.5

0.2 0.4 0.6 0.8 1.0 1.2 1.4

0.2 0.4 0.6 0.8 1.0 1.2

Figure:α7→µa,p(α) withp= 4 and (left)a= 0.45 or (right)a= 0.2

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

Reformulations of the interpolation problem (1/3)

Any minimizerψXa ofµa,p(α) satisfies the Euler-Lagrange equation

(Ha+α)ψ=|ψ|p−2ψ , Haψ=− d

ds+i a 2

ψ

up to a multiplication by a constant andv(s) =ψ(s)eias satisfies the condition

v(s+ 2π) =e2iπav(s)s∈R (2) Hence

µa,p(α) = min

v∈Ya\{0}Qp,α[v]

whereYa :=

vC(R) : v0∈L2(S1), (2) holds and Qp,α[v] := kv0k2L2(S1)+αkvk2L2(S1)

kvk2Lp(S1)

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

Reformulations of the interpolation problem (2/3)

Withv=u e the boundary condition becomes

u(π) =u(−π), φ(π) = 2π(a+k) +φ(−π) (3) for somek∈Z, and kv0k2L2(S1)=ku0k2L2(S1)+ku φ0k2L2(S1)

Hence

µa,p(α) = min

(u,φ)∈Za\{0}

ku0k2L2(S1)+ku φ0k2L2(S1)+αkuk2L2(S1)

kuk2Lp(S1)

whereZa:=

(u, φ)∈C(R)2 : u0, u φ0∈L2(S1), (3) holds

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

Reformulations of the interpolation problem (3/3)

We use the Euler-Lagrange equations

u00+|φ0|2u+α u=|u|p−2u and (φ0u2)0= 0

Integrating the second equation, andassuming thatunever vanishes, we find a constantLsuch thatφ0 =L/u2. Taking (3) into account, we deduce from

L Z π

−π

ds u2 =

Z π

−π

φ0ds= 2π(a+k) that

ku φ0k2L2(S1)=L2 Z π

−π

u2 = (a+k)2 ku−1k2L2(S1)

Hence

φ(s)φ(0) = a+k ku−1k2L2(S1)

Z s

−π

ds u2

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

Let us define

Qa,p,α[u] := ku0k2L2(S1)+a2ku−1k−2L2(S1)+αkuk2L2(S1)

kuk2Lp(S1)

Lemma

For anya∈(0,1/2),p >2,α >a2, µa,p(α) = min

u∈H1(S1)\{0}Qa,p,α[u]

is achieved by a functionu >0

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

Proofs

The existence proof is done on the original formulation of the problem using the diamagnetic inequality

ψ(s)eias=v1(s) +i v2(s), solves

vj00+α vj= (v12+v22)p2−1vj, j= 1, 2

and the Wronskianw= (v1v20v10v2) is constant so thatψ(s) = 0 is incompatible with the twisted boundary condition

ifa2(p+ 2) +α(p−2)≤1, thenµa,p(α) =a2+αbecause

ku0k2L2(S1)+a2ku−1k−2L2(S1)+αkuk2L2(S1)= (1−4a2)ku0k2L2(S1)+αkuk2L2(S1)

+ 4a2

ku0k2L2(S1)+14ku−1k2L2(S1)

ifa2(p+ 2) +α(p−2)>1, the test functionuε:= 1 +ε w1

Qa,p,α[uε] =a2+α+ 1−a2(p+ 2)−α(p−2)

ε2+o(ε2) proves the linear instability of the constants andµa,p(α)< a2+α

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

Qa,p,α[u] := ku

0k2L2 (S1 )+a2ku−1k−2L2 (S1 )kuk2L2 (S1 ) kuk2

Lp(S1 )

, µa,p(α) = min

u∈H1(S1)\{0}Qa,p,α[u]

Qp,α[u] =Qa=0,p,α[u], νp(α) := inf

v∈H10(S1)\{0}

Qp,α[v]

Proposition

p >2,α >a2, we have µa,p(α)< µ1/2,p(α)≤νp(α) =µ1/2,p(α)

0.5 1.0 1.5 2.0 2.5 3.0

0.1 0.2 0.3 0.4 0.5 0.6

Figure: p= 4,α= 0,a= 0.40, 0.41,. . . 0.49;u00+up−1= 0

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

A Keller-Lieb-Thirring inequality

Magnetic Schrödinger operatorHaϕ=− dsd +i a2 ψϕ The functionα7→µa,p(α) is monotone increasing, concave, and therefore has an inverse, denoted byαa,p:R+→(−a2,+∞), which is monotone increasing, and convex

Corollary

Letp >2,a∈[0,1/2],q=p/(p−2) and assume thatϕ is a non-negative function inLq(S1). Then

λ1(Haϕ)≥ −αa,p kϕkLq(S1)

andαa,p(µ) =µa2 iff4a2+µ(p−2)≤1 (optimalϕis constant) Equality is achieved

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

Bohm-Aharonov magnetic fields

On the two-dimensional Euclidean spaceR2, let us introduce the polar coordinates (r, ϑ)∈[0,+∞)×S1 ofx∈R2 and consider a magnetic potentialain a transversal (Poincaré) gauge, or Poincaré gauge

(a,er) = 0 and (a,eϑ) =aϑ(r, ϑ) Magnetic Schrödinger energy

Z

R2

|(i∇+a) Ψ|2dx= Z +∞

0

Z π

−π

|∂rΨ|2+ 1

r2|ϑΨ +i r aϑΨ|2

rdϑdr Bohm-Aharonov magnetic fields: aϑ(r, ϑ) =a/rfor some constant a∈R(ais themagnetic flux), with magnetic field b= curla Z

R2

|(i∇+a) Ψ|2dxτ Z

R2

ϕ(x/|x|)

|x|2 |Ψ|2dx ∀ϕ∈Lq(S1), q∈(1,+∞)

=⇒τ=τ a,kϕkLq(S1)

?

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

Hardy inequalities

(Hoffmann-Ostenhof, Laptev, 2015)proved Hardy’s inequality Z

Rd

|∇Ψ|2dx≥τ Z

Rd

ϕ(x/|x|)

|x|2 |Ψ|2dx

where the constantτ depends on the value ofkϕkLq(Sd−1)andd≥3 Bohm-Aharonov vector potentialin dimensiond= 2

a(x) =a x2

|x|2,−x1

|x|2

, x= (x1, x2)∈R2, a∈R and recall the inequality(Laptev, Weidl, 1999)

Z

R2

|(i∇+a) Ψ|2dx≥min

k∈Z

(a−k)2 Z

R2

|Ψ|

|x|2dx

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

A new Hardy inequality

Z

R2

|(i∇+a) Ψ|2dxτ Z

R2

ϕ(x/|x|)

|x|2 |Ψ|2dx ∀ϕ∈Lq(S1), q∈(1,+∞) Corollary

Letp >2,a∈[0,1/2],q=p/(p−2) and assume thatϕ is a

non-negative function inLq(S1). Then the inequality holds withτ >0 given by

αa,p τkϕkLq(S1)

= 0

Moreover,τ=a2/kϕkLq(S1) if 4a2+kϕkLq(S1)(p−2)≤1

For anya∈(0,1/2), by takingϕconstant, small enough in order that 4a2+kϕkLq(S1)(p−2)≤1, we recover the inequality

Z

R2

|(i∇+a) Ψ|2dx≥a2 Z

R2

|Ψ|2

|x|2 dx

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

Proofs (Keller-Lieb-Thirring inequality)

Hölder’s inequality kψ0+i a ψk2L2(S1)

Z π

−π

ϕ|ψ|2dσ≥ kψ0+i a ψk2L2(S1)µkψk2Lp(S1)

whereµ=kϕkLq(S1)and 1q +2p = 1: choose µa,p(α) =µ0+i a ψk2L2(S1)µkψk2Lp(S1)≥ −αkψk2L2(S1)

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

Proofs (Hardy inequality)

Letτ ≥0,x= (r, ϑ)∈R2be polar coordinates inR2 Z

R2

|(i∇+a) Ψ|2τ ϕ

|x|2|Ψ|2

dx

= Z

0

Z

S1

r|∂rΨ|2

| {z }

≥0

+1

r|∂ϑΨ +i aΨ|2τ ϕ r |Ψ|2

dϑdr

λ1(Haτ ϕ) Z

0

Z

S1

1

r|Ψ|2dϑdr

≥ −αa,p(τkϕkLq(S1)) Z

0

Z

S1

1

r|Ψ|2dϑ Ifτ = 0, thenαa,p(τkϕkLq(S1)) =αa,p(0) =−a2

αa,p(τkϕkLq(S1))>0 forτ large

=⇒ ∃!τ >0 such thatαa,p(τkϕkLq(S1)) = 0

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Consequences

Comments

BThe regiona2(p+ 2) +α(p−2)<1 is exactly the set where the constant functions are linearly stable critical points

BThe proof of therigidity resultis based

- neither on thecarré du champmethod, at least directly

- nor on a Fourier representation of the operator as it was the case in earlier proofs (p= +∞, orp >2 andα= 0)

BMagnetic rings: see(Bonnaillie-Noël, Hérau, Raymond, 2017) BDeducingHardy’s inequalityapplied withBohm-Aharonovmagnetic fields from aKeller-Lieb-Thirring inequalityis an extension of

(Hoffmann-Ostenhof, Laptev, 2015)to the magnetic case BOur results are not limited to the semi-classical regime

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

Magnetic interpolation inequalities in the Euclidean space

BThree interpolation inequalities and their dual forms BEstimates in dimensiond= 2 for constant magnetic fields

Lower estimates

Upper estimates and numerical results

A linear stability result (numerical) and an open question Warning: assumptions are not repeated

Estimates are given only in the casep >2 but similar estimates hold in the other cases

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

Magnetic Laplacian and spectral gap

In dimensionsd= 2 andd= 3: themagnetic Laplacianis

−∆Aψ=−∆ψ−2iA· ∇ψ+|A|2ψi(divA)ψ

where the magnetic potential (resp. field) isA(resp.B= curlA) and HA1(Rd) :=

ψ∈L2(Rd) : ∇Aψ∈L2(Rd) ,A:=∇+iA Spectral gap inequality

k∇Aψk22≥Λ[B]kψk22ψ∈HA1(Rd) (4) Λ depends only onB= curlA

Assumption: equality in (4)holds for someψ∈HA1(Rd) IfBis a constant magnetic field, Λ[B] =|B|

Ifd= 2, spec(−∆A) ={(2j+ 1)|B| : j∈N}is generated by the Landau levels. TheLowest Landau Levelcorresponds to j= 0

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

Magnetic interpolation inequalities

k∇Aψk22+αkψk22µB(α)kψk2pψ∈HA1(Rd) (5) for anyα∈(−Λ[B],+∞) and anyp∈(2,2),

k∇Aψk22+βkψk2pνB(β)kψk22ψ∈HA1(Rd) (6) for anyβ∈(0,+∞) and anyp∈(1,2)

k∇Aψk22γ Z

Rd

|ψ|2 log |ψ|2

kψk22

dx+ξB(γ)kψk22ψ∈HA1(Rd) (7) (limit case corresponding top= 2) for anyγ∈(0,+∞)

Cp:=

minu∈H1(Rd)\{0}

k∇uk22+kuk22

kuk2p if p∈(2,2) minu∈H1(Rd)\{0}

k∇uk22+kuk2p

kuk22 if p∈(1,2) µ0(1) =Cpifp∈(2,2),ν0(1) =Cp ifp∈(1,2)

ξ0(γ) =γlog π e2

ifp= 2

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

Technical assumptions

A∈Lαloc(Rd),α >2 ifd= 2 orα= 3 ifd= 3 and

σ→+∞lim σd−2 Z

Rd

|A(x)|2e−σ|x|dx= 0 if p∈(2,2)

σ→+∞lim σd2−1

logσ Z

Rd

|A(x)|2e−σ|x|2dx= 0 if p= 2

σ→+∞lim σd−2 Z

|x|<1/σ

|A(x)|2dx if p∈(1,2)

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

A statement

Theorem

p∈(2,2): µBis monotone increasing on (−Λ[B],+∞), concave and lim

α→(−Λ[B])+

µB(α) = 0 and lim

α→+∞µB(α)αd−22 dp =Cp

p∈(1,2): νB is monotone increasing on(0,+∞), concave and

β→0lim+νB(β) = Λ[B] and lim

β→+∞νB(β)β2p+d(2−p)2p =Cp

ξB is continuous on(0,+∞), concave,ξB(0) = Λ[B]and ξB(γ) =d2γlog π eγ2

(1 +o(1)) as γ→+∞

Constant magnetic fields: equality is achieved

Nonconstant magnetic fields: only partial answers are known

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

2 4 6 8 10

2 4 6 8

Figure: Cased= 2,p= 3,B= 1: plot ofα7→(2π)2p−1µB(α)

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

0 1 2 3 4 5 6

0 2 4 6 8

Figure: Cased= 2,p= 1.4,B= 1: plot ofβ7→νB(β). The horizontal axis is measured in units of (2π)1−2pβ

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

Magnetic Keller-Lieb-Thirring inequalities

λA,V is the principal eigenvalue of−∆A+V

αB: (0,+∞)→(−Λ,+∞) is the inverse function ofα7→µB(α) Corollary

(i) For any q=p/(p−2)∈(d/2,+∞)and any potential 0≥V ∈Lq(Rd)

λA,V ≥ −αB(kVkq)

limµ→0+αB(µ) = Λand limµ→+∞αB(µ)µd−2−22 (q+1)q =−C

2 (q+1) d−2−2q

p

(ii) For any q=p/(2p)∈(1,+∞)and any 0< W−1∈Lq(Rd) λA,WνB kW−1k−1q

(iii) For any γ >0 and any W ≥0 s.t.e−W/γ∈L1(Rd) λA,WξB(γ)−γ log R

Rde−W/γdx

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

A more general duality result

Proposition

Letd= 2 or3. Letφ∈L1loc(Rd)be an arbitrary potential (i) If q > d/2,p=q−12q , we have

λA,φ≥ −(αB(k(λ−φ)kq,+)−λ) (ii) If q∈(1,+∞),p= q+12q , we have

λA,φλ+νB k(φ−λ)−1k−1q

These estimates hold for anyλ∈Rsuch that all above norms are well defined, with the additional condition thatφλa.e. in Case (ii)

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

Preliminaries: interpolation without magnetic field

Assume thatp >2 and letCp denote the best constant in k∇uk22+kuk22≥Cpkuk2pu∈H1(Rd) By scaling, if we test the inequality byu ·

, we find that k∇uk22+λ2kuk22≥Cpλ2−d(1−p2)kuk2pu∈H1(Rd) ∀λ >0 An optimization onλ >0 shows that the best constant in the scale-invariant inequality

k∇ukd(1−

2 p)

2 kuk2−d(1−

2 p)

2 ≥Spkuk2pu∈H1(Rd) is given by

Sp= 21p (2pd(p−2))1−d

p−2

2p (d(p−2))

d(p−2) 2p Cp

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

... and with magnetic field

Proposition

Letd= 2 or3. For anyp∈(2,+∞), anyα >−Λ =−Λ[B]<0

µB(α)≥µinterp(α) :=

Sp(α+ Λ) Λ−dp−22p ifα∈h

−Λ,Λ (2dp−d(p−2)(p−2))i Cpα1−dp−22p ifαΛ (2dp−d(p−2)(p−2)) Lett∈[0,1]. From the diamagnetic inequalityk∇|ψ|k2≤ k∇Aψk2

and from the inequality withλ=α+Λ1−tt, we deduce that k∇Aψk22+αkψk22t k∇Aψk22−Λkψk22

+ (1−t)

k∇|ψ|k2+α+ Λt 1−t kψk22

≥Cp(1−t)d(p−2)2p (α+tΛ)1−dp−22p kψk2p and optimize ont∈[max{0,−α/Λ},1]

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

Lower estimates: d = 2, constant magnetic field

Assume thatB= (0, B) is constant, d= 2 and choose A1=B2x2, A2=−B2x1x= (x1, x2)∈R2 Proposition

(Loss, Thaller, 1997)Consider a constant magnetic field with field strengthB in two dimensions. For everyc∈[0,1], we have

Z

R2

|∇Aψ|2dx≥ 1−c2 Z

R2

|∇ψ|2dx+c B Z

R2

ψ2dx

and equality holds withψ=u eiS andu >0 if and only if

−∂2u2, ∂1u2

= 2u2

c (A+∇S)

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

... a computation (d = 2, constant magnetic field)

Z

R2

|∇Aψ|2dx= Z

R2

|∇u|2dx+ Z

R2

|A+∇S|2u2dx

= 1−c2 Z

R2

|∇u|2dx+ Z

R2

c2|∇u|2+|A+∇S|2u2 dx

| {z }

R

R22c|∇u| |A+∇S|u dx

with equality only ifc|∇u|=|A+∇S|u

2|∇u| |A+∇S|u=|∇u2| |A+∇S| ≥ ∇u2

·(A+∇S) where ∇u2

:= −∂2u2, ∂1u2 Equality case: −∂2u2, ∂1u2

=γ(A+∇S) forγ= 2u2/c Integration by parts yields

Z

R2

c2|∇u|2+|A+∇S|2u2

dxB c Z

R2

u2dx

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

Lower estimate (d = 2, constant magnetic field):

a result

Proposition

Consider a constant magnetic field with field strengthB in two dimensions. Given anyp∈(2,+∞), and any α >−B, we have

µB(α)≥Cp 1−c21−2p (α+c B)2p =:µLT(α) with

c=c(p, η) =

pη2+p−1−η

p−1 = 1

η+p

η2+p−1 ∈(0,1) andη=α(p−2)/(2B)

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

Upper estimate (1): d = 2, constant magnetic field

For every integerk∈Nwe introduce the special symmetry class ψ(x) =

x2+i x1

|x|

k

v(|x|)x= (x1, x2)∈R2 (Ck) (Esteban, Lions, 1989): ifψ∈Ck, then

1 2π

Z

R2

|∇Aψ|2dx= Z +∞

0

|v0|2r dr+ Z +∞

0 k

rB r2 2

|v|2r dr and optimality is achieved inCk

Test functionvσ(r) =er2/(2σ): an optimization on σ >0 provides an explicit expression ofµGauss(α) such that

Proposition Ifp >2, then

µB(α)≤µGauss(α) ∀α >−Λ[B]

This estimate is not optimal becausevσ does not solve the Euler-Lagrange equations

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

Upper estimate (2): d = 2, constant magnetic field

A more numerical point of view. The Euler-Lagrange equation inC0 is

v00v0 r +

B2

4 r2+α

v=µEL(α) Z +∞

0

|v|pr dr 2p−1

|v|p−2v

We can restrict the problem to positive solutions such that µEL(α) =

Z +∞

0

|v|pr dr 1−p2

and then we have to solve the reduced problem

v00v0 r +

B2

4 r2+α

v=|v|p−2v

J. Dolbeault Magnetic interpolation inequalities

(38)

Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

2 4 6 8 10

-1 1 2 3

0.004 0.003 0.002 0.001 0.001 0.002 0.003

-0.02

-0.04

-0.06

-0.08

2 4

-1

6

Figure: Cased= 2,p= 3,B= 1: comparison of the upper estimates α7→µGauss(α) andα7→µEL(α) with the lower estimatesα7→µinterp(α) andα7→µLT(α)

Plots represent the curves log10GaussEL), log10LTEL) and log10interpEL) so thatα7→µEL(α) corresponds to a straight line at level 0. The exact value associated withµBlies in the grey area

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

Asymptotics (1): Lowest Landau Level

Proposition

Letd= 2 and consider a constant magnetic field with field strengthB.

Ifψα is a minimizer forµB(α)such thatαkp= 1, then there exists a non trivialϕα∈LLL such that

lim

α→(−B)+

αϕαkH1

A(R2)= 0

Letψα∈HA1(R2) be an optimal function for (5) such thatkψαkp= 1 and let us decompose it asψα=ϕα+χα, where ϕα∈LLL andχαis in the orthogonal of LLL

µB(α)≥(α+B)kϕαk22+(α+3B)kχαk22≥(α+3B)kχαk22∼2Bkχαk22 asα→(−B)+ becausek∇χαk22≥3Bkχαk22

Since limα→(−B)+µB(α) = 0, limα→(−B)+αk2= 0 and

µB(α) = (α+B)kϕαk22+ k∇Aχαk22+ααk2223k∇Aχαk22 concludes the proof

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

Asymptotics (2): semi-classical regime

Let us consider the small magnetic field regime. We assume that the magnetic potential is given by

A1=B2x2, A2=−B2x1x= (x1, x2)∈R2 ifd= 2. In dimension d= 3, we chooseA= B2(−x2, x1,0) and observe that the constant magnetic field isB= (0,0, B), while the spectral gap in (4) is Λ[B] =B.

Proposition

Letd= 2 or3 and consider a constant magnetic fieldB of intensityB with magnetic potential A

For anyp∈(2,2)and any fixedαandµ >0, we have

ε→0lim+

µεB(α) =Cpαdpd−22 Consider any functionψ∈HA1(Rd) and letψ(x) =χ(

ε x),

εA x/ε

=A(x) with our conventions onA

J. Dolbeault Magnetic interpolation inequalities

(41)

Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

Numerical stability of radial optimal functions

Let us denote byψ0 an optimal function in (C0) such that

ψ000ψ00 r +

B2

4 r2+α

ψ0=|ψ0|p−2ψ0 and consider the test function

ψε=ψ0+ε ei θv wherev=v(r) andei θ= (x1+i x2)/r Asε→0+, the leading order term is

2π Z

R2

|v0|2dx+ Z

R2

1 rB r2 2

+α

|v|2dxp2 Z +∞

0

0|p−2v2r dr

ε2

and we have to solve the eigenvalue problem

v00v0 r +

1

rB r2 2 +α

vp20|p−2v=µ v

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

2 4 6 8

1 2 3 4

Figure: Casep= 3 andB= 1: plot of the eigenvalueµas a function ofα A careful investigation shows thatµis always positive, including in the limiting case asα→(−B)+, thus proving the numerical stability of the optimal function inC0with respect to perturbations inC1

J. Dolbeault Magnetic interpolation inequalities

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Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields

An open question of symmetry

(Bonheure, Nys, Van Schaftingen, 2016)for a fixed α >0 and forB small enough, the optimal functions are radially symmetric functions,i.e., belong toC0

This regime is equivalent to the regime asα→+∞for a givenB, at least if the magnetic field is constant

Numerically our upper and lower bounds are (in dimensiond= 2, for a constant magnetic field) numerically extremely close

The optimal function inC0with respect to perturbations inC1

Prove that the optimality case is achieved among radial function if d= 2 andB is a constant magnetic field

J. Dolbeault Magnetic interpolation inequalities

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