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Order of convergence of splitting schemes for both deterministic and - - PowerPoint PPT Presentation

1 Order of convergence of splitting schemes for both deterministic and stochastic nonlinear Schr odinger equations Jie Liu National University of Singapore, Singapore Numerics for Stochastic Partial Differential Equations and their


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Order of convergence of splitting schemes for both deterministic and stochastic nonlinear Schr¨

  • dinger

equations

Jie Liu National University of Singapore, Singapore Numerics for Stochastic Partial Differential Equations and their Applications, RICAM, Linz, Dec. 2016.

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Outline

  • The second order convergence of Strang-type splitting scheme for

nonlinear Schr¨

  • dinger equation.
  • Mass preserving splitting scheme for stochastic nonlinear Schr¨
  • dinger

equation with multiplicative noise ⋆ Explicit formula for the nonlinear step ⋆ first order strong convergence

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Strang-type splitting scheme for nonlinear Schr¨

  • dinger

equation

Let i = √−1 and V be a real-valued function. Consider the following nonlinear Schr¨

  • dinger equation

idu = ∆udt + V (x, |u|)udt in Rd. (1) Note three things:

  • If a ∈ R, idu

dt = au ⇒ u(t) = e−iatu(0). Hence |u(t)| = |u(0)|.

  • The exact solution of idu = V (x, |u|)udt, u(0) = u0 satisfies |u(t)| =

|u(0)| and therefore u(x, t) = exp {−itV (x, |u0(x)|)} u0(x).

  • Recall the Strang splitting for du = (Au + Bu)dt:

u(δt) = eδt(A+B)u(0) ≈ e

δt 2 BeδtAe δt 2 Bu(0).

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We will study the following scheme 1 un−1 → ˜ un−1

2 →

  • un−1

2 → un → ˜

un+1

2 →

  • un+1

2 → un+1 → · · · :

˜ un−1

2 = exp

  • −iδt

2 V (x, |un−1|)

  • un−1,

(2)

  • un−1

2 = exp {−iδt∆} ˜

un−1

2,

(3) un = exp

  • −iδt

2 V (x, |

  • un−1

2|)

  • un−1

2.

(4) It can be implemented as

  • un−1

2 → ˜

un+1

2 →

  • un+1

2 (skip un) because

˜ un+1

2 = exp

  • −iδt

2 V (x, |un|)

  • un = exp
  • −iδtV (x, |
  • un−1

2|)

  • un−1

2.

The second order convergence in L2 norm has been proved by Lubich2.

1Hardin & Tappert 1973, Taha & Ablowitz 1984.

  • 2C. Lubich, On splitting methods for Schr¨
  • dinger-Poisson and cubic nonlinear Schr¨
  • dinger equations.
  • Math. Comp., 77 (2008) 2141–2153.
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Second order convergence

Theorem 1. Consider (1) and its numerical scheme (2)–(4) in R3. Assume V (x, |u|) = |u|2, and take any γ > 3/2 and any σ ∈ {0, 1, 2, 3, ...}. If u0γ = Mγ < ∞, then there are constants T and C1 depending on Mγ such that for any δt > 0, max

n=0,1,...,[T /δt] unγ ≤ C1.

(5) If u0σ+4 = Mσ+4 < ∞, then there are constants T and C2 depending

  • n Mσ+4 such that for any δt > 0,

max

n=0,1,...,[T /δt] u(tn) − unσ ≤ C2δt2.

(6) Assume in addition that there are constants ¯ T and ¯ Mσ+4 so that sup0≤t≤ ¯

T u(s)σ+4 =

¯ Mσ+4 < ∞, then there is a constant δt0 > 0 so that when δt ≤ δt0, the T in (6) can be taken as ¯ T.

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Integral formulation of the scheme

Fix T, δt, and N = [T/δt]. Define a right continuous function φN(x, t) with

  • φN(x, 0) = u0(x).
  • φN(t) = e{−i[tV (x,|φN(0)|)]}φN(0) when t ∈ [0, δt

2 )

  • On any interval [tn−1

2, tn+1 2) (n = 1, 2, ...),

φN(t) =      e{−iδt∆} lim

t↑tn−1

2 φN(t)

when t = tn−1

2,

e

{−i

  • (t−tn−1

2)V (x,|φN(tn−1 2)|)

  • }φN(tn−1

2)

when t ∈ [tn−1

2, tn+1 2).

Then φN(tn−1

2) =

  • un−1

2

and φN(tn) = un.

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Integral formulation of the scheme

Recall φN(t) =              e{−iδt∆} lim t↑tn−1 2 φN(t) when t = tn−1 2, e {−i

  • (t−tn−1

2)V (x,|φN(tn−1 2)|)

  • }

φN(tn−1 2) when t ∈ [tn−1 2, tn+1 2).

  • When t ∈ [tn−1

2, tn+1 2),

dφN(t) = −iV (x, |φN(t)|)φN(t)dt and therefore φN(t) = φN(tn−1

2) − i

t

tn−1

2

V (x, |φN(s)|)φN(s)ds. (7)

  • When t = tn+1

2,

φN(tn+1

2) = e{−iδt∆}

 φN(tn−1

2) − i

tn+1

2

tn−1

2

V (x, |φN(s)|)φN(s)ds   . (8)

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Integral formulation of the scheme

φN satisfies φN(t) = e−itn∆φN(0) − i t SN,n,t(s)

  • V (x, |φN(s)|)φN(s)
  • ds

when t ∈ [tn−1

2, tn+1 2), where φN(0) = u(0),

SN,n,t(s) = e−inδt∆I

[0,t

1 2](s) + n−1

j=1 I [tn−1

2−j,tn+1 2−j](s)e−i(jδt)∆ + I

[tn−1

2,t](s).

Let S(t − s) = e−i(t−s)∆. The exact solution u(t) of NLS satisfies u(t) = e−it∆u(0) − i t S(t − s) (V (x, |u(s)|)u(s)) ds. Note that tn

0 SN,n,tn(s)ds is the midpoint rule approximation of

tn

0 S(tn − s)ds on the partition

t

1 2

0 + n−1 j=1

tn+1

2−j

tn−1

2−j +

t

tn−1

2

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Error equation

Let r(t) = u(t) − φN(t). We have r(t) =(e−it∆ − e−itn∆)u0 − i t (S(t − s) − SN,n,t(s)) V (x, |φN(s)|)φN(s)ds − i t S(t − s) [V (x, |u(s)|)u(s) − V (x, |φN(s)|)φN(s)] ds =:J1(t) + J2(t) + J3(t) (9) for t ∈ [tn−1

2, tn+1 2) (but n is arbitrary). Note that only at t = tn, J1(tn)

vanishes instead of being of size O(δt).

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Error estimate

  • Step 1:

(First order error estimate over a short time interval) Since fgγ ≤ cfγgγ when γ > d/2 and e−it∆wσ = wσ, (e−it∆ − I)wα = t∆wα, one immediately get supt≤T φN(t)4 < C and sup

t≤T

r(t)2 ≤ Cδt for some T > 0. Here r(t) = u(t) − φN(t), rα = rHα

  • Step 2: (Error estimate over a short time interval) There is a constant

T which depends on the initial data so that r(tn)0 ≤ C3δt

n−1

  • j=1

r(tj)0 + C5δt2 for all n ≤ [T/δt]. So, second order convergence follows from the standard discrete Gronwall inequality.

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Step 3: (Error estimate up to the blowing up time of the exact solution) Note that to prove the 2nd order convergence in L2, one has to prove the stability in H4: By Calculus inequality in the Sobolev space, |φN|2φN4 ≤ CφN2

2φN4.

(10) Hence φN(t)4 ≤φN(0)4 + C t (u(s)2 + φN(s) − u(s)2)2 φN(s)4ds.

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12

Stochastic Schr¨

  • dinger equation

Consider the stochastic Schr¨

  • dinger equation with multiplicative noise:

idv = ∆vdt + V (x, |v|)vdt + v ◦ dW in Rd, (11) where v is a complex valued function, i = √−1, W is a real valued Wiener process, ◦ means Stratonovich product, V is also real valued. Let {βk : k ∈ N} be a sequence of independent Brownian motions that are associated with {Ft : t ≥ 0}. Let {ek : k ∈ N} be an orthonormal basis

  • f L2(Rd, R). Then

ˆ W =

  • k

βk(t, ω)ek(x) and W = Φ ˆ W =

  • k

βk(t, ω)(Φek(x)). Φ is a Hilbert-Schmidt operator from L2 to Hα 3.

3To present our scheme, we need α = 0. To prove stability and convergence, we will need larger α.

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Applications of Stochastic NLS

  • It can be used to model the wave propagation in nonhomogeneous or

random media4. (Prof. Solna’s talk on Tuesday)

  • It has been introduced by Bang etc5 as a model for molecular

monolayers arranged in Scheibe aggregates with thermal fluctuations

  • f the phonons.
  • It has also been widely used in quantum trajectory theory6, which

determines the evolution of the state of a continuously measured quantum system (e.g. the continuous monitoring of an atom by the detection of its fluorescence light).

  • 4V. Konotop, and L. V´

azquez, Nonlinear random waves, World Scientific, NJ, 1994.

  • 5O. Bang, P.L. Christiansen, F. If, K. Ø. Rasmussen and Y. B. Gaididei, Temperature effects in a

nonlinear model of monolayer Scheibe aggregates, Phys. Rev. E, 49 (1994) 4627–4636.

  • 6A. Barchielli and M. Gregoratti, Quantum trajectories and measurements in continuous time: the

diffusive case, Lecture Notes in Physics 782, Springer, Berlin, 2009.

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⎧ ⎪ ⎪ ⎨ ⎪ ⎪ ⎩ dψ(t) = ⎛ ⎝−iH(t) − 1 2

d

  • j=1

R j(t)∗R j(t) ⎞ ⎠ ψ(t) dt +

d

  • j=1

R j(t)ψ(t) dW j(t) , ψ(0) = ψ0 , ψ0 ∈ H. (2.28)

2 The Stochastic Schr¨

  • dinger Equation. . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11

2.1 Introduction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 11 2.2 Linear Stochastic Differential Equations . . . . . . . . . . . . . . . . . . . . . 12 2.2.1 An Homogeneous Linear SDE in Hilbert Space . . . . . . . . 13 2.2.2 The Stochastic Evolution Operator. . . . . . . . . . . . . . . . . . . 14 2.2.3 The Square Norm of the Solution . . . . . . . . . . . . . . . . . . . . 17 2.3 The Linear Stochastic Schr¨

  • dinger Equation . . . . . . . . . . . . . . . . . . 19

2.3.1 A Key Restriction . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 19 2.3.2 A Change of Probability . . . . . . . . . . . . . . . . . . . . . . . . . . . 21 2.4 The Physical Interpretation. . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 21 2.4.1 The POM of the Output and the Physical Probabilities . . 23 2.4.2 The A Posteriori States . . . . . . . . . . . . . . . . . . . . . . . . . . . . 25 2.4.3 Infinite Time Horizon . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 26 2.4.4 The Conservative Case . . . . . . . . . . . . . . . . . . . . . . . . . . . . 27 2.5 The Stochastic Schr¨

  • dinger Equation . . . . . . . . . . . . . . . . . . . . . . . . 28

2.5.1 The Stochastic Differential of the A Posteriori State . . . . 28 2.5.2 Four Stochastic Schr¨

  • dinger Equations . . . . . . . . . . . . . . . 30

2.5.3 Existence and Uniqueness of the Solution . . . . . . . . . . . . . 33 2.5.4 The Stochastic Schr¨

  • dinger Equation as a Starting Point

38 2.6 The Linear Approach Versus the Nonlinear One . . . . . . . . . . . . . . . 40 2.7 Tricks to Simplify the Equations . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41 2.7.1 Time-Dependent Coefficients and Unitary Transformations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 41

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Known results

  • A. de Bouard and A. Debussche, A stochastic nonlinear Schr¨
  • dinger equation with

multiplicative noise, Commun. Math. Phys. 205 (1999) 161-181.

  • A. de Bouard and A. Debussche, A semi-discrete scheme for the stochastic nonlinear

Schr¨

  • dinger equation, Numerische Math. 96 (2004) 733–770.
  • A. de Bouard and A. Debussche, Weak and strong order of convergence of a

semi discrete scheme for the stochastic nonlinear Schr¨

  • dinger equation, Applied

Mathematics and Optimization, 54 (2006) 369–399.

  • R. Marty, On a splitting scheme for the nonlinear Schr¨
  • dinger equation in a random
  • medium. Commun. Math. Sci., 4 (2006) 679–705.
  • Z. Brzezniak and A. Millet, On the splitting method for Schrodinger-like evolution
  • equations. Stochastic Analysis and Related Topics, 2012 57–90.
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Exact formula for the nonlinear part

Let us for the moment drop the ∆v term in stochastic NLS: idv = V (x, |v|)vdt + v ◦ dW(t). (12) For the above equation, we have the following observation: Theorem 2. The following v(x, t) is a solution of (12) v(x, t) = v(x, 0) exp {−i[tV (x, |v(x, 0)|) + W(x, t)]} . (13) In particular, |v(x, t)| = |v(x, 0)| and V (x, |v(x, t)|) = V (x, |v(x, 0)|).

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Mass preserving splitting scheme

It is now clear that we can define the following splitting scheme initialized with v0 = v(x, 0): ˜ vn = exp

  • −i
  • δtV (x, |vn−1|) +
  • W(x, tn) − W(x, tn−1)
  • vn−1, (14)

vn = exp {−iδt∆} ˜ vn. (15) It is clear vn2

L2 = ˜

vn2

L2 = vn−12

  • L2. We summarize this property

into the following Theorem: Theorem 3. The scheme (14)–(15) is unconditionally stable and is mass preserving, i.e, for any n vn2

L2 = v02 L2.

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18

First order strong convergence

Theorem 4. Consider (11) and the scheme (14)–(15) in Rd. Assume V (x, |v|) = |v|2. Take any integer γ > d/2 and assume Φ ∈ L2(L2, Hγ+2). Assume the F0-measurable initial data v0 satisfies

  • Ev0p

Hγ+2

1/p < Mγ+2 < ∞ uniformly for p ≥ 1. Then, for any L > 0 with associated stopping time τL = inf{t, v(t)γ ≥ L}, we have lim

K→∞ P

  • δt−1

max

n=0,1,...,[τL/δt] v(tn) − vnγ ≥ K

  • = 0.

(16) Moreover, for any ε > 0, there exists a random variable KL,ε with finite E|KL,ε|q for any q ≥ 1, such that max

n=0,1,...,[τL/δt] v(tn) − vnγ ≤ KL,εδt1−ε.

(17)

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Integral representation of the scheme

Fix T, δt and N = [T/δt]. Introduce a right continuous function ψN(x, t) with ψN(x, 0) = v(x, 0) = v0 and on any interval [tn−1, tn], ψN(t) =          e{−i[(t−tn−1)V (x,|ψN(tn−1)|)+(W (t)−W (tn−1))]} ×ψN(tn−1) t ∈ [tn−1, tn), e{−iδt∆} limt↑tn ψN(t) t = tn. We have ψN(tn) = vn

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Integral representation of the scheme

ψN(t) = e{−itn−1∆}ψN(0) − i t SN,n,t(s)×

  • ¯

V (x, |ψN(s)|)ψN(s)ds + ψN(s)dW(s)

  • ,

where SN,n,t(s) =

n−1

  • j=1

I[tn−1−j,tn−j](s)e−i(jδt)∆ + I[tn−1,t](s). (18)

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Truncated stochastic Schrodinger equation

Because we do not have E|X|3 ≤ C(E|X|)3, the previous argument cannot be applied here. To prove error estimate, we need to study the following truncated equation (motivated the works of Profs. de Bouard & Debussche and Prof. Gy¨

  • ngy and his co-workers)

idvR = ∆vRdt + ¯ VR(x, vR)vRdt + vRdW in Rd, (19) with initial condition vR(x, 0) = v0(x). Here θR(w) = θ wγ R

  • ,

VR(x, w) = θR(w)V (x, |w|), ¯ VR(x, w) = VR(x, w) − i 2FΦ. θ ∈ C∞(R) is a cut-off function satisfying θ(x) = 1 for x ∈ [0, 1] and θ(x) = 0 for x ≥ 2. γ is any integer > d/2.

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Step 1: Stability of the truncated stochastic NLS

One can prove that even though we only truncate in the Hγ norm in vR, the solution automatically becomes Hγ+2-regular: Lemma 1. (de Bouard and Debussche) Take any integer γ > d/2 and consider (19) in Rd with ¯ VR(x, v) = θ (vγ/R) |v|2 − i

2FΦ.

Assume Φ ∈ L2(L2, Hγ+2). Take any T > 0 and any p ≥ 1, for any F0- measurable initial data v0 satisfying Ev0p

γ+2 = Mγ+2 < ∞, there is a

constant MR depending on R, such that E sup

t≤T

vR(t)p

γ+2 ≤ MR.

(20) Once again. the proof uses |vR|2vRγ+2 ≤ CvR2

γvRγ+2.

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Step 2: splitting scheme for the truncated stochastic NLS

Proposition 1. Take any integer γ > d/2 and consider the splitting scheme in Rd with VR(x, v) = θR(v)|v|2. Assume Φ ∈ L2(L2, Hγ+2). For any R, T > 0 and any p ≥ 1, for any F0-measurable initial data v0 satisfying Ev0p

γ+2 ≤ Mp,γ+2 < ∞, there is a constant CR which

depends on R, T, p, Mp,γ+2 and ΦL2(L2,Hγ+2) so that E max

n=0,1,...,[T/δt] vR(tn) − vn Rp γ ≤ CRδtp.

(21) Proof: Let r(t) = vR(t) − ψR

N(t). Then

r(t) =

7

  • k=1

Ik(t), (22)

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24

where I1(t) =

  • e{−i(t−tn−1)∆} − 1
  • e{−itn−1∆}v0,

(23) I2(t) = − i t SN,n,t(s)

  • VR(x, vR)vR(s) − VR(x, ψR

N)ψR N(s)

  • ds,

(24) I3(t) = − 1 2 t SN,n,t(s)r(s)FΦds, (25) I4(t) = − i t (S(t − s) − SN,n,t(s)) VR(x, vR)vR(s)ds, (26) I5(t) = − 1 2 t (S(t − s) − SN,n,t(s)) vR(s)FΦds, (27) I6(t) = − i t SN,n,t(s)r(s)dW(s), (28) I7(t) = − i t (S(t − s) − SN,n,t(s)) vR(s)dW(s). (29)

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25

Finally, E sup

0≤τ≤t

r(τ)p

γ ≤ C1

t

  • E sup

0≤τ≤s

r(τ)p

γ

  • ds + C2δtp.

The C1 term comes from the estimates of I2, I3, I6 and the C2 term comes from the estimates of I1, I4, I5, I7.

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26

Step 3: from truncated equation to un-truncated equation

(Follows the idea of Gy¨

  • ngy and Nualart.) Next, for any σ ≥ 0, L > 0,

we define the stopping time τL = inf{t, v(t)σ ≥ L}. We then prove that for any ε ∈ (0, 1)

  • max

0≤n≤[τL/δt] vn − v(tn)σ ≥ ε

  • sup

0≤t≤τL

v(t)σ ≥ R − 1

  • max

0≤n≤[τL/δt] vn R − vR(tn)σ ≥ ε

  • (30)

for any R > 0. This follows from A ⊂ B ∪ { ¯ B ∩ A}. (30) allows us to prove the convergence in probability before τL for the splitting scheme for the un-truncated stochastic NLS.

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27

First order strong convergence

Theorem 5. Consider (11) and the scheme (14)–(15) in Rd. Assume V (x, |v|) = |v|2. Take any integer γ > d/2 and assume Φ ∈ L2(L2, Hγ+2). Assume the F0-measurable initial data v0 satisfies

  • Ev0p

Hγ+2

1/p < Mγ+2 < ∞ uniformly for p ≥ 1. Then, for any L > 0 with associated stopping time τL = inf{t, v(t)γ ≥ L}, we have lim

K→∞ P

  • δt−1

max

n=0,1,...,[τL/δt] v(tn) − vnγ ≥ K

  • = 0.

(31) Moreover, for any ε > 0, there exists a random variable KL,ε with finite E|KL,ε|q for any q ≥ 1, such that max

n=0,1,...,[τL/δt] v(tn) − vnγ ≤ KL,εδt1−ε.

(32)