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Metastable and interface dynamics for the hyperbolic Jin-Xin system - PowerPoint PPT Presentation

Metastable and interface dynamics for the hyperbolic Jin-Xin system in one space dimension Marta Strani, Sapienza Universit` a di Roma, Dipartimento di Matematica 14th International Conference on Hyperbolic Problems: Theory, Numerics,


  1. Metastable and interface dynamics for the hyperbolic Jin-Xin system in one space dimension Marta Strani, Sapienza Universit` a di Roma, Dipartimento di Matematica 14th International Conference on Hyperbolic Problems: Theory, Numerics, Applications Universit` a di Padova, June 25-29 2012

  2. Outline Slow motion of internal shock layers for the Jin-Xin system in one space 1 dimension Overview of the problem Spectral analysis Main results

  3. The main problem We describe slow motion for the Jin-Xin system, with Dirichlet boundary conditions in the bounded interval I = ( − ℓ, ℓ ), that is  ∂ t u + ∂ x v = 0    ∂ t v + a 2 ∂ x u = 1   ε ( f ( u ) − v )  (1) u ( ± ℓ, t ) = u ± t ≥ 0       u ( x , 0) = u 0 ( x ) , v ( x , 0) = v 0 ( x ) ≡ f ( u 0 ( x )) x ∈ I for some ε, ℓ, a > 0, u ± ∈ R and flux function f that satisfies f ′′ ( s ) ≥ c 0 > 0 , f ′ ( u + ) < 0 < f ′ ( u − ) , f ( u + ) = f ( u − ) In vector form ∂ t Z = F ε [ Z ] , � Z t =0 = Z 0 � where   − ∂ x v � P ε � 1 [ Z ] F ε [ Z ] := = − a 2 ∂ x u + 1 P ε   2 [ Z ] ε ( f ( u ) − v )

  4. The main problem We describe slow motion for the Jin-Xin system, with Dirichlet boundary conditions in the bounded interval I = ( − ℓ, ℓ ), that is  ∂ t u + ∂ x v = 0    ∂ t v + a 2 ∂ x u = 1   ε ( f ( u ) − v )  (1) u ( ± ℓ, t ) = u ± t ≥ 0       u ( x , 0) = u 0 ( x ) , v ( x , 0) = v 0 ( x ) ≡ f ( u 0 ( x )) x ∈ I for some ε, ℓ, a > 0, u ± ∈ R and flux function f that satisfies f ′′ ( s ) ≥ c 0 > 0 , f ′ ( u + ) < 0 < f ′ ( u − ) , f ( u + ) = f ( u − ) In vector form ∂ t Z = F ε [ Z ] , � Z t =0 = Z 0 � where   − ∂ x v � P ε � 1 [ Z ] F ε [ Z ] := = − a 2 ∂ x u + 1 P ε   2 [ Z ] ε ( f ( u ) − v )

  5. Metastable dynamics First time scale where solutions are close to some non stationary state. Exponentially long time convergence to the asymptotic limit. Presence of a first small eigenvalue of the linearized operator. Allen-Cahn: Carr, Pego, Comm. Pure Appl. Math. 1989 Fusco, Hale, J. Dyn. Diff. Eq. 1989 Cahn-Hilliard: Pego, Proc. Roy. Soc. London Ser. A 1989 Alikakos, Bates, Fusco, J. Diff. Eq. 1991 Burgers: Reyna, Ward, Comm. Pure Appl. Math. 1995 Laforgue, O’Malley, SIAM J. Appl. Math 1995 Mascia, S., submitted

  6. Metastable dynamics First time scale where solutions are close to some non stationary state. Exponentially long time convergence to the asymptotic limit. Presence of a first small eigenvalue of the linearized operator. Allen-Cahn: Carr, Pego, Comm. Pure Appl. Math. 1989 Fusco, Hale, J. Dyn. Diff. Eq. 1989 Cahn-Hilliard: Pego, Proc. Roy. Soc. London Ser. A 1989 Alikakos, Bates, Fusco, J. Diff. Eq. 1991 Burgers: Reyna, Ward, Comm. Pure Appl. Math. 1995 Laforgue, O’Malley, SIAM J. Appl. Math 1995 Mascia, S., submitted

  7. Metastable dynamics First time scale where solutions are close to some non stationary state. Exponentially long time convergence to the asymptotic limit. Presence of a first small eigenvalue of the linearized operator. Allen-Cahn: Carr, Pego, Comm. Pure Appl. Math. 1989 Fusco, Hale, J. Dyn. Diff. Eq. 1989 Cahn-Hilliard: Pego, Proc. Roy. Soc. London Ser. A 1989 Alikakos, Bates, Fusco, J. Diff. Eq. 1991 Burgers: Reyna, Ward, Comm. Pure Appl. Math. 1995 Laforgue, O’Malley, SIAM J. Appl. Math 1995 Mascia, S., submitted

  8. Metastable dynamics First time scale where solutions are close to some non stationary state. Exponentially long time convergence to the asymptotic limit. Presence of a first small eigenvalue of the linearized operator. Allen-Cahn: Carr, Pego, Comm. Pure Appl. Math. 1989 Fusco, Hale, J. Dyn. Diff. Eq. 1989 Cahn-Hilliard: Pego, Proc. Roy. Soc. London Ser. A 1989 Alikakos, Bates, Fusco, J. Diff. Eq. 1991 Burgers: Reyna, Ward, Comm. Pure Appl. Math. 1995 Laforgue, O’Malley, SIAM J. Appl. Math 1995 Mascia, S., submitted

  9. The relaxation limit In the relaxation limit ( ε → 0 + ), system (1) can be approximated to leading order by ∂ t u + ∂ x f ( u ) = 0 , v = f ( u ) (2) The first equation is a quasi-linear equation of hyperbolic type, whose standard setting is given by the entropy formulation , hence possessing discontinuous solutions with speed of propagation s given by the Rankine–Hugoniot relation s [ [ u ] ] = [ [ f ( u )] ] together with appropriate entropy conditions. Concerning the stationary solutions From the entropy conditions follows that only a single jump from the value u − ≥ u + is admitted, with speed s = 0.

  10. The relaxation limit In the relaxation limit ( ε → 0 + ), system (1) can be approximated to leading order by ∂ t u + ∂ x f ( u ) = 0 , v = f ( u ) (2) The first equation is a quasi-linear equation of hyperbolic type, whose standard setting is given by the entropy formulation , hence possessing discontinuous solutions with speed of propagation s given by the Rankine–Hugoniot relation s [ [ u ] ] = [ [ f ( u )] ] together with appropriate entropy conditions. Concerning the stationary solutions From the entropy conditions follows that only a single jump from the value u − ≥ u + is admitted, with speed s = 0.

  11. The relaxation limit In the relaxation limit ( ε → 0 + ), system (1) can be approximated to leading order by ∂ t u + ∂ x f ( u ) = 0 , v = f ( u ) (2) The first equation is a quasi-linear equation of hyperbolic type, whose standard setting is given by the entropy formulation , hence possessing discontinuous solutions with speed of propagation s given by the Rankine–Hugoniot relation s [ [ u ] ] = [ [ f ( u )] ] together with appropriate entropy conditions. Concerning the stationary solutions From the entropy conditions follows that only a single jump from the value u − ≥ u + is admitted, with speed s = 0.

  12. Stationary solutions for ε = 0 Stationary solutions We have a one-parameter family of stationary solutions U hyp ( x ; ξ ) = u − χ ( − ℓ,ξ ) ( x ) + u + χ ( ξ,ℓ ) ( x ) V hyp ( x ; ξ ) = f ( u − ) χ ( − ℓ,ξ ) ( x ) + f ( u + ) χ ( ξ,ℓ ) ( x ) The dynamics determined by initial-value problem for (2) is very simple. Hypotheses: If f ( u ) is convex and such that f ( u − ) = f ( u + ), where u + ≤ u − every entropy solution converges in finite time to an element of the family { U hyp ( · ; ξ ) , V hyp ( · ; ξ ) } .

  13. Stationary solutions for ε = 0 Stationary solutions We have a one-parameter family of stationary solutions U hyp ( x ; ξ ) = u − χ ( − ℓ,ξ ) ( x ) + u + χ ( ξ,ℓ ) ( x ) V hyp ( x ; ξ ) = f ( u − ) χ ( − ℓ,ξ ) ( x ) + f ( u + ) χ ( ξ,ℓ ) ( x ) The dynamics determined by initial-value problem for (2) is very simple. Hypotheses: If f ( u ) is convex and such that f ( u − ) = f ( u + ), where u + ≤ u − every entropy solution converges in finite time to an element of the family { U hyp ( · ; ξ ) , V hyp ( · ; ξ ) } .

  14. Stationary solutions for ε = 0 Stationary solutions We have a one-parameter family of stationary solutions U hyp ( x ; ξ ) = u − χ ( − ℓ,ξ ) ( x ) + u + χ ( ξ,ℓ ) ( x ) V hyp ( x ; ξ ) = f ( u − ) χ ( − ℓ,ξ ) ( x ) + f ( u + ) χ ( ξ,ℓ ) ( x ) The dynamics determined by initial-value problem for (2) is very simple. Hypotheses: If f ( u ) is convex and such that f ( u − ) = f ( u + ), where u + ≤ u − every entropy solution converges in finite time to an element of the family { U hyp ( · ; ξ ) , V hyp ( · ; ξ ) } .

  15. Metastable dynamics for ε > 0 Stationary solution For ε > 0, the presence of the Laplace operator has the effect of a drastic reduction of the number of stationary solutions: in this case there exists a unique stationary solution that is asymptotically stable. Such solution, denoted here by (¯ rel ( x ) , ¯ U ε V ε rel ( x )), converges in the limit ε → 0 + to a specific element of the family { U hyp ( · ; ξ ) , V hyp ( · ; ξ ) } . Question What happens to the dynamics generated by an initial datum localized that still presents a sharp transition from u − to u + , but it is localized far from the equilibrium solution?

  16. Metastable dynamics for ε > 0 Stationary solution For ε > 0, the presence of the Laplace operator has the effect of a drastic reduction of the number of stationary solutions: in this case there exists a unique stationary solution that is asymptotically stable. Such solution, denoted here by (¯ rel ( x ) , ¯ U ε V ε rel ( x )), converges in the limit ε → 0 + to a specific element of the family { U hyp ( · ; ξ ) , V hyp ( · ; ξ ) } . Question What happens to the dynamics generated by an initial datum localized that still presents a sharp transition from u − to u + , but it is localized far from the equilibrium solution?

  17. Metastable dynamics for ε > 0 Stationary solution For ε > 0, the presence of the Laplace operator has the effect of a drastic reduction of the number of stationary solutions: in this case there exists a unique stationary solution that is asymptotically stable. Such solution, denoted here by (¯ rel ( x ) , ¯ U ε V ε rel ( x )), converges in the limit ε → 0 + to a specific element of the family { U hyp ( · ; ξ ) , V hyp ( · ; ξ ) } . Question What happens to the dynamics generated by an initial datum localized that still presents a sharp transition from u − to u + , but it is localized far from the equilibrium solution?

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