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Exponential convergence to the equilibrium for the stochastic Gross-Pitaevskii equation€¦ ·...

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Page 1: Exponential convergence to the equilibrium for the stochastic Gross-Pitaevskii equation€¦ ·  · 2016-11-14Exponential convergence to the equilibrium for the stochastic Gross-Pitaevskii

Exponential convergence to the equilibrium for thestochastic Gross-Pitaevskii equation

R. Fukuizumi 1

A. de Bouard 2 and A. Debussche 3

1RCPAM, GSIS, Tohoku University, Japan2CMAP, Ecole Polytechnique, France

3IRMAR, ENS Cachan Bretagne, France

Mathematical and Physical models of Nonlinear Optics @ IMA

R. Fukuizumi (Tohoku Univ.) October 31, 2016 1 / 29

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Outline

1 IntroductionPhysical Motivation

2 Gibbs equilibriumGibbs measureMain resultsGibbs measure and the stationary solutionInvariance of the Gibbs measure

3 Local existence

4 Global existence for ρ a.e. initial data

5 Convergence to the Gibbs equilibriumPoincaré inequality

6 Final remarks

R. Fukuizumi (Tohoku Univ.) October 31, 2016 2 / 29

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Introduction Physical Motivation

Outline

1 IntroductionPhysical Motivation

2 Gibbs equilibriumGibbs measureMain resultsGibbs measure and the stationary solutionInvariance of the Gibbs measure

3 Local existence

4 Global existence for ρ a.e. initial data

5 Convergence to the Gibbs equilibriumPoincaré inequality

6 Final remarks

R. Fukuizumi (Tohoku Univ.) October 31, 2016 3 / 29

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Introduction Physical Motivation

Bose-Einstein Condensation (BEC)

A state of matter of a dilute gas of bosons cooled to temperatures veryclose to absolute zero; a large amount of bosons occupy the lowestquantum state, where macroscopic quantum phenomena can be observed.Predicted in 1924-25, Realization in 1995.

87Rb, 23Na, 7Li, 1H, 85Rb, 41K, 4He, 133Cs, 174Yb,

52Cr, 40Ca, 84Sr : Example of the dilute gases of bosons

R. Fukuizumi (Tohoku Univ.) October 31, 2016 4 / 29

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Introduction Physical Motivation

Dynamics of BEC at nite temperature

At the zero temperature T = 0, all the atoms are well-presented by asingle condensate function and the coherent evolution of the wavefunction is described by the standard GP equation

At higher temperature, all spontaneous and incoherent process (for ex.interaction with thermal cloud) may not be neglected

The eect of such incoherent elements are implemented by adding adisspation and a noise to the GP equation, called 'Stochastic GPequation,' which is well suited for vortex formulation in BEC (Weileret al. Nature (2008))

dψ = P− i

~LGPψdt +

G (x)

kBT(µ− LGP)ψdt + dWG (x , t)

where

LGP = − ~2

2m∇2 + V (x) + g |ψ|2, 〈dW ∗G (s, y), dWG (t, x)〉 = 2G (x)δt−sδx−y

R. Fukuizumi (Tohoku Univ.) October 31, 2016 5 / 29

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Introduction Physical Motivation

P.B. Blakie et al., Advanced in Physics (2008); introduce moredetailed energy cut-o

The equation evolves the system to the grand-canonical equilibriumdistribution.

M.Kobayashi-L.Cugliandolo (arXiv:1606.03262); interested in a quenchdynamics in BEC

Phase transition leads to the formation of topological defects (i.e.vortices)Investigation of the thermal equilibrium (Gibbs equilibrium) gives theclassication (Universality class) of the type of phase transitionsStudy of the equilibrium properties around the phase transition pointsusing, as a model, Stochastic GP equation with V (x) = 0, G (x) = 1under a periodic boundary condition

Remark that essentially, nite dimension models are analyzed in Physics.Our aim: Study these models from a mathematical point of view, (i.e., ininnite dimension). In particular, interested in the Gibbs equilibrium (thecase of a space-time white noise).

R. Fukuizumi (Tohoku Univ.) October 31, 2016 6 / 29

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Introduction Physical Motivation

We consider mathematically (for the moment in 1d):

(Ω,F ,P) : propability space endowed with ltration (Ft)t≥0The equation :

dX = (i + γ)(∂2xX − V (x)X − λ|X |2X )dt +√γdW ,

X (0) = X0, t > 0, x ∈ R

where γ > 0. Assume V (x) = x2 and λ = 1 (defocusing).

(∂2x − x2)hk = −λ2khk with λk =√2k + 1, k ∈ N. The eigenfunctions

hk(x) are known as the Hermite functions.

W (t) : cylindrical Wiener pocess on L2(R,C), i.e.

W (t, x) =∑k∈N

βk(t)hk(x), t > 0, x ∈ R

where βk(t)k∈N : a sequence of C-valued independent Brownianmotions.

R. Fukuizumi (Tohoku Univ.) October 31, 2016 7 / 29

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Gibbs equilibrium Gibbs measure

Outline

1 IntroductionPhysical Motivation

2 Gibbs equilibriumGibbs measureMain resultsGibbs measure and the stationary solutionInvariance of the Gibbs measure

3 Local existence

4 Global existence for ρ a.e. initial data

5 Convergence to the Gibbs equilibriumPoincaré inequality

6 Final remarks

R. Fukuizumi (Tohoku Univ.) October 31, 2016 8 / 29

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Gibbs equilibrium Gibbs measure

Hamiltonian for the case of γ = 0:

H(u) =1

2

∫R|(−∂2x + x2)1/2u|2dx +

1

4

∫R|u|4dx

The Gibbs measure:

ρ(du) = Γe−H(u)du

= Γe−14

∫R |u|

4dxe−12((−∂2x+x2)u,u)L2du = Γe−

14

∫R |u|

4dxµ(du)

where Γ is the normalizing constant, may be justied in Lp(R), p > 2(see later) taking the limit N →∞ of the Gaussian measure onR2(N+1) dened by

dµN :=N∏k=0

λ2k2π

e−λ2k2(a2

k+b2

k)dakdbk

if we write u =∑

k(ak + ibk)hk with (ak , bk) ∈ R2.

µ := limN→∞ µN can be interpreted as the law of random variable∑k∈N

√2

λkgk(ω)hk(x) with L(gk) = NC(0, 1)

R. Fukuizumi (Tohoku Univ.) October 31, 2016 9 / 29

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Gibbs equilibrium Gibbs measure

Known results

Burq, Tzvetkov and Thomann, (γ = 0, λ = ±1, V (x) = x2, 1d)Ann. Inst. Fourier (Grenoble) (2013)

Construction of Gibbs measure, Global Cauchy theory in the negativeSobolev space.

Barton-Smith, (γ 6= 0, λ = ±1, V (x) = 0, bounded domain D, any d)Nonlinear dier. equ. appl.(2004)

Existence and Uniqueness of invariant measure on Lp(D) (p ∈ [2,∞))for a not too small γ 6= 0

E.A. Carlen, J. Fröhlich and J. Lebowitz, (regular noise, λ = −1,V (x) = 0, periodic boundary condi., 1d) (arXiv:1409.2327)

Construction of the grand-canonical Gibbs measure (i.e. with amodied Hamiltonian) and exponential convergence by Dirichlet formapproach under some assumptions on the noise

Our result is new on the points/no restriction on γ, the exp-convergencewith a space-time white noise

R. Fukuizumi (Tohoku Univ.) October 31, 2016 10 / 29

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Gibbs equilibrium Main results

Outline

1 IntroductionPhysical Motivation

2 Gibbs equilibriumGibbs measureMain resultsGibbs measure and the stationary solutionInvariance of the Gibbs measure

3 Local existence

4 Global existence for ρ a.e. initial data

5 Convergence to the Gibbs equilibriumPoincaré inequality

6 Final remarks

R. Fukuizumi (Tohoku Univ.) October 31, 2016 11 / 29

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Gibbs equilibrium Main results

Recall that our equation isdX = (i + γ)(∂2xX − x2X − |X |2X )dt +

√γdW ,

X (0) = X0, t > 0, x ∈ R.

Let p ≥ 3, X0 ∈ Lp(R), and γ > 0.

Theorem

There exists a set O ⊂ Lp(R) such that ρ(O) = 1, and such that for

X0 ∈ O there exists a unique solution X (·) ∈ C ([0,∞), Lp(R)) a.s.

Let Pt be the transition semigroup for the equation, i.e.Ptφ(y) = E(φ(X (t, y))), y ∈ O, t ≥ 0.

Theorem

Let φ ∈ L2((Lp, dρ),R), and φ =∫Lpφ(y)dρ(y). Then Ptφ(·) converges

exponentially to φ in L2((Lp, dρ),R), as t →∞ ; more precisely,∫Lp|Ptφ(y)− φ|2dρ(y) ≤ e−γt

∫Lp|φ(y)− φ|2dρ(y).

R. Fukuizumi (Tohoku Univ.) October 31, 2016 12 / 29

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Gibbs equilibrium Gibbs measure and the stationary solution

Outline

1 IntroductionPhysical Motivation

2 Gibbs equilibriumGibbs measureMain resultsGibbs measure and the stationary solutionInvariance of the Gibbs measure

3 Local existence

4 Global existence for ρ a.e. initial data

5 Convergence to the Gibbs equilibriumPoincaré inequality

6 Final remarks

R. Fukuizumi (Tohoku Univ.) October 31, 2016 13 / 29

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Gibbs equilibrium Gibbs measure and the stationary solution

Gibbs measure and the stationary solution

Let us denote by

Z∞(t) =√γ

∫ t

−∞e−(t−s)(i+γ)(−∂

2x+x

2)dW (s),

the solution of

dZ = (i + γ)(∂2x − x2)Zdt +√γdW

which is stationary, i.e. such that L(Z∞(t)) = L(Z∞(0)).

Write Z∞(t) using the basis hkk ,

Z∞(t) =√γ∑k∈N

(∫ t

−∞e−(t−s)(i+γ)λ

2kdβk(s)

)hk

The law of Z∞(t) equals to the Gaussian measure µ, since

L(√

γ

∫ 0

−∞es(i+γ)λ

2kdβk(s)

)= NC

(0,

2

λ2k

)R. Fukuizumi (Tohoku Univ.) October 31, 2016 14 / 29

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Gibbs equilibrium Gibbs measure and the stationary solution

Support of the measure

Let p > 2. Note that by Minkowski inequality, for q ≥ p, one has

|Z∞(t)|Lqω(Lpx ) ≤ |Z∞(t)|Lpx (Lqω).

Since Z∞ is Gaussian, to compute |Z∞|Lqω when q = 2m, it suces tocompute the L2ω norm:

E(|Z∞(t, x)|2) ≤ γ∑k∈N

E∣∣∣ ∫ t

−∞e−λ

2k(t−s)(i+γ)dβk(s)

∣∣∣2|hk(x)|2

≤ 2γ∑k∈N

∫ t

−∞e−2λ

2kγ(t−s)ds |hk(x)|2 ≤

∑k∈N

|hk(x)|2

λ2k.

R. Fukuizumi (Tohoku Univ.) October 31, 2016 15 / 29

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Gibbs equilibrium Gibbs measure and the stationary solution

For q = 2m with 2m ≥ p, we have

E(|Z∞(t, x)|2m) ≤ CmE(|Z∞(t, x)|2)m ≤ Cm

(∑k

|hk(x)|2

λ2k

)mand

|Z∞(t)|L2mω (Lpx )≤ Cm

∣∣∣∑k∈N

|hk(x)|2

λ2k

∣∣∣1/2Lp/2x

≤ Cm

(∑k

|hk(x)|2Lpx

λ2k

)1/2It is known the decay of hk in Lp (Yajima-Zhang, CMP 2001): for

p ≥ 4, |hk |Lp(R) ≤ Cpλ−1/6k , and by interpolation,

if 2 ≤ p ≤ 4, |hk |Lp(R) ≤ Cpλ− 1

3(1− 2

p)

k .

Remind that λ2k = 2k + 1 and the series converges for p > 2, i.e.,Z∞ ∈ L2m(Ω; Lp) for any m ≥ p/2 > 1;i.e. Z∞ ∈ Lp a.s. i.e. ρ(Lp) = 1 for p > 2.

R. Fukuizumi (Tohoku Univ.) October 31, 2016 16 / 29

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Gibbs equilibrium Invariance of the Gibbs measure

Outline

1 IntroductionPhysical Motivation

2 Gibbs equilibriumGibbs measureMain resultsGibbs measure and the stationary solutionInvariance of the Gibbs measure

3 Local existence

4 Global existence for ρ a.e. initial data

5 Convergence to the Gibbs equilibriumPoincaré inequality

6 Final remarks

R. Fukuizumi (Tohoku Univ.) October 31, 2016 17 / 29

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Gibbs equilibrium Invariance of the Gibbs measure

Formal proof for the invariance of the Gibbs measure

We write the equation under the form

dX = −J∇xH(X )dt − γ∇xH(X )dt +√γdW , X (0) = y ∈ Lpx

where

J =

(0 −11 0

): R2 → R2.

Let Pt be the transition semigroup, i.e,Ptφ(y) = E(φ(X (t, y))) = 〈φ, µt,x〉 for φ ∈ Cb(Lp) withµt,x = L(X (t, y)).

〈Ptφ, ρ〉 = Ptφ(y) provided L(y) = ρ. Thus P∗t ρ = µt,x .i.e. ρ is invariant i P∗t ρ = ρ.

R. Fukuizumi (Tohoku Univ.) October 31, 2016 18 / 29

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Gibbs equilibrium Invariance of the Gibbs measure

Let L be the generater for the semigroup Pt :

Lφ(y) = limt→0

Ptφ(y)− φ(y)

t.

For the invariance of ρ it is enough to show∫Lp

(Lφ)(y)ρ(dy) = 0

On the other hand, the generator L is given by (cf. Kolmogorovequation)

(Lφ)(y) = γ∆yφ(y)−γ(∇yφ(y),∇yH(y))L2x − (∇yφ(y), J∇yH(y))L2x

R. Fukuizumi (Tohoku Univ.) October 31, 2016 19 / 29

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Gibbs equilibrium Invariance of the Gibbs measure

∫Lp

(Lφ)(y)ρ(dy) =

∫Lp

[γ∆yφ(y)− γ(∇yφ(y),∇yH(y))L2

−(∇yφ(y), J∇yH(y))L2]e−H(y)dy

= γ

∫Lp

∆yφ(y)e−H(y)dy + γ

∫Lp

(∇yφ(y),∇y (e−H(y))

)L2dy

−∫Lp

(∇yφ(y), J∇y (e−H(y))

)L2dy = 0.

The last term is zero, and the second term is the opposite sign of therst term by I/P.

This calculation can be justied using a nite dimensionalapproximation.

This invariance holds for both purely dissipative case and mixed case.

R. Fukuizumi (Tohoku Univ.) October 31, 2016 20 / 29

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Local existence

Local existence

Write X = v + Z∞ with v satisfying the deterministic PDE:

∂tv = (i + γ)(∂2xv − x2v − |v + Z∞|2(v + Z∞)), t > 0, x ∈ R

Solve locally, then obtain a sol. X in C ([0,T ∗), Lp), p ≥ 3(Ginibre-Velo, CMP. 1997) using the estimates on the linear semigroupobtained by Mehler's formula:

|et(i+γ2)(∂2x−x2)f |Lr (R) ≤ Ct−12l |f |Ls , t > 0 small,

0 ≤ 1

r=

1

s− 1

l, 1 ≤ s, l ≤ ∞.

Energy methods give a global bound in Lp, but it requires somerestriction on the parameter γ. (not too small γ 6= 0)

R. Fukuizumi (Tohoku Univ.) October 31, 2016 21 / 29

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Global existence for ρ a.e. initial data

ρ-a.e. Global existence (formal)

Let T ≥ T ∗, and p ≥ 3. Wish to show that there exists CT such that∫Lp

E(

supt∈[0,T∗)

|X (t,X0)|Lp)ρ(dX0) ≤ CT .

Mild form for X :

X (t) = et(i+γ)(∂2x−x2)X0 − et(i+γ)(∂

2x−x2)Z∞(0)

+

∫ t

0

e(t−s)(i+γ)(∂2x−x2)(|X |2X )(s)ds + Z∞(t).

By the regularity of Z∞: supt |Z∞(t)|Lp ≤ MT , we have∫Lp

E(

supt∈[0,T∗)

|X (t,X0)|Lp)dρ(X0)

≤ C

∫Lp

E|X0|Lpdρ(X0) + CE∫Lp

∫ T

0

|X (s)|3L3pdsdρ(X0) + MT .

R. Fukuizumi (Tohoku Univ.) October 31, 2016 22 / 29

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Global existence for ρ a.e. initial data

Here the invariance of ρ implies∫LpPtφ(X0)dρ =

∫Lpφ(X0)dρ

with φ(X0) = |X0|3L3p . Therefore∫ T

0

∫Lp

E|X (s,X0)|3L3pdρ(X0)ds =

∫ T

0

∫LP|X0|3L3pdρ(X0)ds

≤∫ T

0

∫LP|X0|3L3pdµ(X0)ds

which is equivalent to∫ T0

E(|Z∞(s)|3L3p

)ds since L(Z∞(s)) = µ, andis bounded by CT .

Thusρ(X0 ∈ Lp; sup

t∈[0,T∗)|X (t,X0)|Lp < +∞) = 1.

This formal argument can be justied by an nite dimensionalapproximation.

R. Fukuizumi (Tohoku Univ.) October 31, 2016 23 / 29

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Convergence to the Gibbs equilibrium

Convergence to the equilibrium (formal)

The proof of the convergence is based on a Poincaré inequality: Let γ > 0.For any φ ∈ C 1

b (Lp), the following inequality is satised.∫Lp|∇yφ(y)|2L2ydρ(y) ≥ √γ

∫Lp|φ(y)− φ|2dρ(y), (1)

where φ =∫Lpφ(y)dρ(y).

Assume (1). Let u(t, y) = Ptφ(y) and φ = 0. Then, if L is thegenerator of Pt , then

dudt

= Lu.

L satises (again by the Kolmogorov equation)

Lu2(y) = 2√γ|∇yu|2L2 + 2uLu(y).

R. Fukuizumi (Tohoku Univ.) October 31, 2016 24 / 29

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Convergence to the Gibbs equilibrium

Invariance of the measure ρ implies

0 =

∫LpLu2(y)dρ(y)

= 2√γ

∫Lp|∇yu|2L2dρ(y) + 2

∫Lpu(Lu)(y)dρ(y)

= 2√γ

∫Lp|∇yu|2L2dρ(y) +

d

dt

∫Lp|u(t)|2dρ(y).

hence by (1)d

dt|u(t)|2L2(Lp ,dρ) ≤ −2γ|u|

2L2(Lp ,dρ),

from which it follows

|u(t)|L2(Lp ,dρ) ≤ e−γt |φ|L2(Lp ,dρ).

R. Fukuizumi (Tohoku Univ.) October 31, 2016 25 / 29

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Convergence to the Gibbs equilibrium Poincaré inequality

Outline

1 IntroductionPhysical Motivation

2 Gibbs equilibriumGibbs measureMain resultsGibbs measure and the stationary solutionInvariance of the Gibbs measure

3 Local existence

4 Global existence for ρ a.e. initial data

5 Convergence to the Gibbs equilibriumPoincaré inequality

6 Final remarks

R. Fukuizumi (Tohoku Univ.) October 31, 2016 26 / 29

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Convergence to the Gibbs equilibrium Poincaré inequality

Proof of Poincaré inequality (formal)

This inequality is a property of the measure only, so that we can proveit by the purely dissipative case, for which ρ is also an invariantmeasure.

dY = γ(∂2xY − x2Y − |Y |2Y )dt +√γdW

This is again a formal argument, we need a nite dimensionalapproximation

Denote ηh := DyY (t, y).h; then ηh satisesdη = γ(∂2xη − x2η − γ|Y |2Y − 2γ(Re(Y η)Y )dt,η(0) = h ∈ L2(R).

Thanks to dissipative property, ηh satises

|ηh(t)|L2 ≤ e−γt |h|L2 . (2)

R. Fukuizumi (Tohoku Univ.) October 31, 2016 27 / 29

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Convergence to the Gibbs equilibrium Poincaré inequality

let Rt be the transition semigroup, and let g(t, y) = Rtφ(y) forφ ∈ C 1

b (Lp) and y ∈ Lp. The above exp.decay of ηh and theinvariance of the measure ρ implies∫

Lp|∇yg(y)|2L2dρ(y) ≤ e−2γt

∫Lp

∣∣∣Rt |∇yφ|L2(y)∣∣∣2dρ(y)

≤ e−2γt∫LpRt(|∇yφ|2L2)(y)dρ(y)

= e−2γt∫Lp|∇yφ|2L2(y)dρ(y).

since (∇yg(t, y), h)L2 = E((∇yφ(Y (t, y)), ηh)L2)On the other hand, by the Kolmogorov equation and the invariance ofthe measure (as above),

d

dt|g(t, y)|2L2(Lp ,dρ) = −2√γ|∇yg(y)|2L2(Lp ,dρ)

Note that g(0, y) = φ(y) and that, thanks to dissipative property,|g(t)|L2(Lp ,dρ) → 0 as t →∞. Then integrating in time and tendingt →∞ concludes the Poincaré inequality.

R. Fukuizumi (Tohoku Univ.) October 31, 2016 28 / 29

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Final remarks

Final remarks

Our results may be extended to

Stochastic complex Ginzburg-Landau eq. without the harmonicpotential (but with a periodic boundary condi., or on a boundeddomain with Dirichlet condi.)

with the chemical potential

global existence for all initial data

2d or 3d case, but for the renormalized Hamiltonian

with a rotating term; Lz := −i(x∂y − y∂x),

L(u) =1

2

∫R3

|(−H)1/2u|2 + Re

∫R3

(uΩLzu) +1

4

∫R3

|u|4

The focusing case (λ = −1)

R. Fukuizumi (Tohoku Univ.) October 31, 2016 29 / 29


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