Proof of Theorem 1 getdoc8616. 297KB Jun 04 2011 12:04:37 AM

Secondly, using Cauchy-Schwarz, I I = L E   I Ω t E   Z R e −η|x| |ut + t ∗ , x − Y t+t ∗ | d x F t     ≤ L r 2 η E    I Ω t E   Z R e −η|x| |ut + t ∗ , x − Y t+t ∗ | 2 d x F t   1 2    ≤ L c 1 r 2 η E    I Ω t Z R e −η|x| |ut, x − a| 2 d x 1 2    by Lemma 14 ≤ L c 1 r 2 η E[I Ω t ] by the choice of Ω t = L c 1 r 2 η δ 1 2 . Thus, substituting these estimates into 22, we find for t ≥ T η Z R E ˜ u |1 − ˜u| |˜u − a|t + t ∗ , x d x = Z R E u|1 − u| |u − a|t + t ∗ , x d x ≥ a1 − aδ 1 δ 2 δ 3 4 η − L c 1 r 2 η δ 1 2 . By taking η small this bound can be made arbitrarily large, which contradicts 17.

3.3 Proof of Theorem 1

Let ν c be the limit law constructed from u in Proposition 10. We let ν be the restriction of ν c to D. Proposition 13 shows that in all cases ν is a probability. Moreover the fact that L ˜ut → ν c in M D c implies that L ˜ut → ν in M D. We first check that the centered solutions are still a Markov process. This can be done, as follows, by using the Dynkin criterion see [10] Theorem 13.5 which gives a simple transition kernel condition for when a function of a Markov process remains Markov. Let D = {φ ∈ D : Γφ = 0} with the induced topology. Define the centering map J : D → D by J φ = ˜ φ. Let P t φ, dψ : t ≥ 0 be the Markov transition kernels for solutions to 1. Then the Dynkin criterion is that for all measurable A ⊆ D and all ψ ∈ D the values P t φ, J −1 A are equal for all φ ∈ J −1 ψ. By Lemma 5 ii, elements of J −1 ψ are translates of each other and the Dynkin criterion follows from translation invariance of solutions. As a consequence, there are transition kernels ˜ P t φ, dψ for the centered process on D . We write P t respectively ˜ P t for the associated semigroups generated by these kernels and acting on measurable F : D → R respectively F : D → R, and we write P ∗ t and ˜ P ∗ t for the dual semigroups acting on M D respectively M D . We aim to show that ν is the law of a stationary travelling wave by applying Markov semigroup ar- guments applied to the centered solutions ˜ ut : t ≥ 0. Some difficulties arise since the wavefront marker Γ is only semi-continuous on D, and hence D is a measurable but not a closed subset of D. 459 For example, we do not yet know that Γ φ = 0 for ν almost all φ though we will see that this is true. The centered law ˜ ν charges only D and we will therefore consider it with a slight abuse of notation as an element of M D , where it is the image of ν under the centering map J. Take F : D → R that is bounded, continuous and translation invariant that is F φ = F τ a φ for all a. Then the Feller property and translation invariance of solutions imply that P t F remains bounded, continuous and translation invariant. Let F be the restriction of F to D . The translation invariance of F implies that ˜ P t F φ = P t F φ. Write Q H t and ˜ Q H t for the law of ut and ˜ ut on D, when u is started at H. Then Z D F d˜ P ∗ s ˜ ν = Z D ˜ P s F d ˜ ν = Z D P s F d ν by translation invariance of P s F = lim t →∞ Z D P s F d ˜ Q H t by the convergence ˜ Q H t → ν = lim t →∞ Z D P s F dQ H t by translation invariance of P s F = lim t →∞ Z D F dQ H t+s by the Markov property of u = lim t →∞ Z D F d ˜ Q H t+s by translation invariance of F = Z D F d ν = Z D F d ˜ ν. This equality may now be extended, by a monotone class argument, to hold for all bounded functions that are measurable with respect to the sigma field generated by continuous translation invarinat F . Lemma 15 below shows that this includes all bounded measurable translation invariant F : D → R. Then taking F φ = I ˜ φ ∈ A for a measurable A ⊆ D we find ˜ P ∗ s ˜ νA ∩ D = ˜ P ∗ s ˜ νφ ∈ D : ˜ φ ∈ A = Z D I ˜ φ ∈ Ad˜P ∗ s ˜ ν = Z D I ˜ φ ∈ Ad ˜ ν = ˜ νA ∩ D . This yields ˜ P ∗ s ˜ ν = ˜ ν showing that ˜ ν is the law of a stationary travelling wave. Finally we check that ν was already centered. By the regularity of solutions at any time t 0 we know that φ ∈ C 1 and φ x 0 for ˜ P ∗ t ˜ ν almost all φ, and hence for ˜ ν almost all φ or indeed for ν 460 almost all φ. But the construction of ν showed that φx ≤ a for x 0 and φx ≥ a for x 0 for ν almost all φ. Combining these shows that Γφ = 0 for ν almost all φ and thus ν charges only D . Thus ˜ ν = ν and this completes the proof. Remark. We have fixed the centering height a throughout and supressed its dependence in the notation. However, we wish to show that the choice of height is unimportant and, in this remark only, we shall now indicate this dependence. The construction in Proposition 10 of the stretched limit ν c held for any centering height. We write ν a c for this law when centered at height a and also Γ a for the wavefront marker at height a and ˜ u a for the the solution started at H centered using Γ a . The moments in Proposition 13 rely on the specific properties of f and g and the distiguished point a in the definition of the three types of reaction f . But these moments imply, in any of the three cases, that the law ν a c charges only D and that the restiction ν a to D is the law of a stationary travelling wave for any centering height a. We claim, for a 1 , a 2 ∈ 0, 1, that the image of ν a 1 under the map φ → φ· + Γ a 2 φ is ν a 2 . Indeed ν a 1 s ≻ δ H and so by Corollary 9 i and the stationarity of ν a 1 we have ν a 1 s ≻ L ˜u a 2 t. Now letting t → ∞ we have ν a 1 s ≻ ν a 2 . But reversing the roles of a 1 and a 2 we find ν a 2 s ≻ ν a 1 and Lemma 6 ii implies that the centered copies at any height of ν a 1 and ν a 2 must coincide. Lemma 15. Translation invariant measurable F : D → R are measurable with respect to the sigma field generated by the continuous translation invariant functions on D. Proof. We make use of a smoother wave marker than the wave marker Γ a for the height a. Define ˆ Γ = R 1 haΓ a d a, where h : 0, 1 → R is continuous and compactly supported in 0, 1. Then Γφ is finite and Γ τ a φ = Γφ+a if we assume in addition that R h d x = 1. Then the map φ → ˆΓφ is continuous since Γ a φ is discontinuous at φ only for the countably many a where {x : φx = a} has non-empty interior. We let ˆ D = {φ ∈ D : ˆΓφ = 0}, so that D is a closed subset of D, and give it the induced subspace topology and Borel sigma field. For this proof only we let ˜ φ be the wave centered at the new wave-marker ˆ Γ. One may now check that the map D ∋ φ → Jφ = ˆΓφ, ˜ φ ∈ R × ˆ D is a homeomorphism. Also, every continuous respectively measurable translation invariant F : D → R is of the form Fφ = ˆ F ˜ φ for some continuous respectively measurable ˆ F : ˆ D → R. Using this one finds that τ := {O ⊆ D : O is open and IO is translation invariant} = {J −1 R × O : O open in ˆD } and {B ⊆ D : B is measurable and IB is translation invariant} = {J −1 R × B : B measurable in ˆD }. This implies that translation invariant measurable F : D → R are measurable with respect to the sigma field στ. But for an open O ⊆ D for which IO is translation invariant, by us- ing a translation invariant metric on D see the start of section 2.2, the continuous functions F n φ = min{ndφ, O c , 1} are translation invariant and converge to IO as n → ∞, completing the proof. 461 4 The domain of attraction Throughout this section ν is the law of the stationary travelling wave constructed in Theorem 1. The stochastic monotonicity results imply that solutions starting from a certain set of initial conditions are attracted to ν, as follows. Proposition 16. Suppose that f is of KPP, Nagumo or unstable type. In the latter two cases suppose that f a = 0 and ga 6= 0. Let u be a solution to 1 whose initial condition u0 has law µ ∈ M D. If ν s ≻ µ s ≻ δ H then L ˜ut → ν as t → ∞. Proof Since ν s ≻ µ s ≻ δ H , Corollary 9 i implies that ν s ≻ L ˜ut s ≻ ˜ Q H t 23 for all t. The simple idea is to let t → ∞ and use ˜ Q H t → ν. We face a familiar set of technical details to check. For any sequence t n → ∞ there is a subsequence t ′ n along which L ˜ut converges in M D c to a limit which we call µ c . For λ 0, the map φ → 1 − exp−λ R R φ1 − φd x is increasing on D in the stretching pre-order and lower semi- continuous on D c . Using ν s ≻ L ˜ut n ′ and L ˜ut n ′ → µ c we find Z D c ‚ 1 − exp−λ Z R φ1 − φd x Œ µ c dφ ≤ Z D ‚ 1 − exp−λ Z R φ1 − φd x Œ νdφ Proposition 13 shows that in all cases R φ1 − φd x ∞ for ν almost all φ. Therefore as λ ↓ 0 the right hand side approaches 0. This shows that µ c charges only D or the single points φ ≡ 0 or φ ≡ 1. However the construction of µ c as the limit of centered laws ensures that φx ≤ a for x 0 and φx ≥ a for x 0 for µ c almost all φ. We conclude that µ c only charges D. Let µ be the restriction of µ c to D, so that L ˜ut n ′ → µ in M D. Using Lemma 6 iii we may pass to the limit in 23 as n ′ → ∞ to find ν s ≻ µ s ≻ µ. Lemma 6 ii now gives that ˜ µ = ˜ ν. But we know that ν charges only φ for which φ ∈ C 1 R and φ x 0. Hence so does µ and ˜ µ = µ = ν. This shows that L ˜ut n ′ → ν and since t n was arbitrary the proof is finished. Checking the hypotheses of Proposition 16 does not look easy. Moreover one would expect the domain of attraction for ν to contain many other initial conditions. In the upcoming section we discuss a natural class of initial conditions that should be in the domain.

4.1 Solutions with finite initial width

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