26.12.2013 Views

Degenerate parabolic stochastic partial differential equations

Degenerate parabolic stochastic partial differential equations

Degenerate parabolic stochastic partial differential equations

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

M. Hofmanová / Stochastic Processes and their Applications 123 (2013) 4294–4336 4313<br />

These <strong>equations</strong> have smooth solutions and consequent passage to the limit gives the existence<br />

of a kinetic solution to the original equation. Nevertheless, the limit argument is quite technical<br />

and has to be done in several steps. It is based on the compactness method: the uniform energy<br />

estimates yield tightness of a sequence of approximate solutions and thus, on another probability<br />

space, this sequence converges almost surely due to the Skorokhod representation theorem. The<br />

limit is then shown to be a martingale kinetic solution to (1). Combining this fact and the pathwise<br />

uniqueness with the Gyöngy–Krylov characterization of convergence in probability, we finally<br />

obtain the desired kinetic solution.<br />

4.1. Nondegenerate case<br />

Consider a truncation (χ ε ) on R and approximations to the identity (ϕ ε ), (ψ ε ) on T N × R<br />

and R, respectively. To be more precise concerning the case of T N ×R, we make use of the same<br />

notation as at the beginning of the proof of Theorem 3.3 and define<br />

ϕ ε (x, ξ) = 1 x<br />

ξ<br />

<br />

ε N+1 ϱ ψ .<br />

ε ε<br />

The regularizations of Φ, B are then defined in the following way<br />

B ε i (ξ) = (B i ∗ ψ ε )χ ε<br />

<br />

(ξ), i = 1, . . . , N,<br />

<br />

gk ε (x, ξ) = (gk ∗ ϕ ε )χ ε (x, ξ), if k ≤ ⌊1/ε⌋,<br />

0, if k > ⌊1/ε⌋,<br />

where x ∈ T N , ξ ∈ R. Consequently, we set B ε = (B1 ε, . . . , Bε N ) and define the operator Φε by<br />

Φ ε (z)e k = gk ε(·, z(·)), z ∈ L2 (T N ). Clearly, the approximations B ε , gk ε are of class C∞ with<br />

a compact support therefore Lipschitz continuous. Moreover, the functions gk ε satisfy (2), (3)<br />

uniformly in ε and the following Lipschitz condition holds true<br />

∀x ∈ T N ∀ξ, ζ ∈ R<br />

|gk ε (x, ξ) − gε k (x, ζ )|2 ≤ L ε |ξ − ζ | 2 . (24)<br />

k≥1<br />

From (2) we conclude that Φ ε (z) is Hilbert–Schmidt for all z ∈ L 2 (T N ). Also the polynomial<br />

growth of B remains valid for B ε and holds uniformly in ε. Suitable approximation of the<br />

diffusion matrix A is obtained as its perturbation by εI, where I denotes the identity matrix.<br />

We denote A ε = A + εI.<br />

Consider an approximation of problem (1) by a nondegenerate equation<br />

du ε + div B ε (u ε ) dt = div A ε (x)∇u ε dt + Φ ε (u ε ) dW,<br />

u ε (0) = u 0 .<br />

(25)<br />

Theorem 4.1. Assume that u 0 ∈ L p (Ω; C ∞ (T N )) for all p ∈ (2, ∞). For any ε > 0, there<br />

exists a C ∞ (T N )-valued process which is the unique strong solution to (25). Moreover, it belongs<br />

to<br />

L p (Ω; C([0, T ]; W l,q (T N ))) for every p ∈ (2, ∞), q ∈ [2, ∞), l ∈ N.<br />

Proof. For any fixed ε > 0, the assumptions of [18, Theorem 2.1, Corollary 2.2] are satisfied<br />

and therefore the claim follows. □<br />

Let m ε be the <strong>parabolic</strong> dissipative measure corresponding to the diffusion matrix A + εI . To<br />

be more precise, set

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!