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
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
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
kψ0k2L2(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)):
kψ0k2L2(S1)+1
4kψk2Lp(S1)≥1
4kψk2L2(S1)
Casep >2: Bakry-Emery method applies toKolmogorov’s inequality
J. Dolbeault Magnetic interpolation inequalities
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 dσ
| {z }
≥0(Poincaré) +
Z π
−π
|u0|4 u2 dσ
Ifp >1,p6= 2, the method is well known(Bakry, Emery, 85)
J. Dolbeault Magnetic interpolation inequalities
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
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:=
ψ∈Cper(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
|ψ0+i a ψ|2=|χ0+i(1−a)χ|2=
ψ0−i a ψ
2 ifχ(s) =e−isψ(s) a∈[0,1/2]
J. Dolbeault Magnetic interpolation inequalities
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,+∞),ψ∈Xa
µa,p(α) := inf
ψ∈Xa\{0}
Rπ
−π |ψ0+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)2|ψk|2≥a2kψk2L2(S1)
ψ7→ kψ0+i a ψk2L2(S1)+αkψk2L2(S1)is coercive for any α >−a2
J. Dolbeault Magnetic interpolation inequalities
Magnetic interpolation in the Euclidean space Consequences
An interpolation result for the magnetic ring
Theorem
For anyp >2,a∈R, andα >−a2,µa,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
Magnetic interpolation in the Euclidean space Consequences
Reformulations of the interpolation problem (1/3)
Any minimizerψ∈Xa 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 :=
v∈C(R) : v0∈L2(S1), (2) holds and Qp,α[v] := kv0k2L2(S1)+αkvk2L2(S1)
kvk2Lp(S1)
J. Dolbeault Magnetic interpolation inequalities
Magnetic interpolation in the Euclidean space Consequences
Reformulations of the interpolation problem (2/3)
Withv=u eiφ 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
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
dσ
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
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
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= (v1v20 − v10v2) 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
Magnetic interpolation in the Euclidean space Consequences
Qa,p,α[u] := ku
0k2L2 (S1 )+a2ku−1k−2L2 (S1 )+αkuk2L2 (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
Magnetic interpolation in the Euclidean space Consequences
A Keller-Lieb-Thirring inequality
Magnetic Schrödinger operatorHa−ϕ=− dsd +i a2 ψ−ϕ 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(Ha−ϕ)≥ −αa,p kϕkLq(S1)
andαa,p(µ) =µ−a2 iff4a2+µ(p−2)≤1 (optimalϕis constant) Equality is achieved
J. Dolbeault Magnetic interpolation inequalities
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|2dx≥τ Z
R2
ϕ(x/|x|)
|x|2 |Ψ|2dx ∀ϕ∈Lq(S1), q∈(1,+∞)
=⇒τ=τ a,kϕkLq(S1)
?
J. Dolbeault Magnetic interpolation inequalities
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
Magnetic interpolation in the Euclidean space Consequences
A new Hardy inequality
Z
R2
|(i∇+a) Ψ|2dx≥τ 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
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) =µ kψ0+i a ψk2L2(S1)−µkψk2Lp(S1)≥ −αkψk2L2(S1)
J. Dolbeault Magnetic interpolation inequalities
Magnetic interpolation in the Euclidean space Consequences
Proofs (Hardy inequality)
Letτ ≥0,x= (r, ϑ)∈R2be polar coordinates inR2 Z
R2
|(i∇+a) Ψ|2−τ ϕ
|x|2|Ψ|2
dx
= Z ∞
0
Z
S1
r|∂rΨ|2
| {z }
≥0
+1
r|∂ϑΨ +i aΨ|2−τ ϕ r |Ψ|2
dϑdr
≥λ1(Ha−τ 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
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
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
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|2ψ− i(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]kψk22 ∀ψ∈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
Magnetic interpolation in the Euclidean space Estimates in dimensiond= 2 for constant magnetic fields
Magnetic interpolation inequalities
k∇Aψk22+αkψk22≥µB(α)kψk2p ∀ψ∈HA1(Rd) (5) for anyα∈(−Λ[B],+∞) and anyp∈(2,2∗),
k∇Aψk22+βkψk2p≥νB(β)kψk22 ∀ψ∈HA1(Rd) (6) for anyβ∈(0,+∞) and anyp∈(1,2)
k∇Aψk22≥γ Z
Rd
|ψ|2 log |ψ|2
kψk22
dx+ξB(γ)kψk22 ∀ψ∈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/γ
ifp= 2
J. Dolbeault Magnetic interpolation inequalities
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
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)β−2p+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
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
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
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/(2−p)∈(1,+∞)and any 0< W−1∈Lq(Rd) λA,W ≥νB kW−1k−1q
(iii) For any γ >0 and any W ≥0 s.t.e−W/γ∈L1(Rd) λA,W ≥ξB(γ)−γ log R
Rde−W/γdx
J. Dolbeault Magnetic interpolation inequalities
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,φ≥λ+νB k(φ−λ)−1k−1q
These estimates hold for anyλ∈Rsuch that all above norms are well defined, with the additional condition thatφ≥λa.e. in Case (ii)
J. Dolbeault Magnetic interpolation inequalities
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≥Cpkuk2p ∀u∈H1(Rd) By scaling, if we test the inequality byu ·/λ
, we find that k∇uk22+λ2kuk22≥Cpλ2−d(1−p2)kuk2p ∀u∈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 ≥Spkuk2p ∀u∈H1(Rd) is given by
Sp= 21p (2p−d(p−2))1−d
p−2
2p (d(p−2))
d(p−2) 2p Cp
J. Dolbeault Magnetic interpolation inequalities
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 ifα≥ Λ (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+αkψk22≥t 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]
J. Dolbeault Magnetic interpolation inequalities
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=−B2x1 ∀x= (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)
J. Dolbeault Magnetic interpolation inequalities
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
dx≥B c Z
R2
u2dx
J. Dolbeault Magnetic interpolation inequalities
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
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
r−B r2 2
|v|2r dr and optimality is achieved inCk
Test functionvσ(r) =e−r2/(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
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
−v00−v0 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
−v00− v0 r +
B2
4 r2+α
v=|v|p−2v
J. Dolbeault Magnetic interpolation inequalities
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 log10(µGauss/µEL), log10(µLT/µEL) and log10(µinterp/µEL) 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
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 thatkψαkp= 1, then there exists a non trivialϕα∈LLL such that
lim
α→(−B)+
kψα−ϕαkH1
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)+kχαk2= 0 and
µB(α) = (α+B)kϕαk22+ k∇Aχαk22+αkχαk22≥23k∇Aχαk22 concludes the proof
J. Dolbeault Magnetic interpolation inequalities
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=−B2x1 ∀x= (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) =Cpαdp−d−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
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
−ψ000− ψ00 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 r−B r2 2
+α
|v|2dx−p2 Z +∞
0
|ψ0|p−2v2r dr
ε2
and we have to solve the eigenvalue problem
−v00− v0 r +
1
r−B r2 2 +α
v−p2|ψ0|p−2v=µ v
J. Dolbeault Magnetic interpolation inequalities
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
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