Defects in oscillatory media towards a classification Bjrn - - PDF document

defects in oscillatory media towards a classification
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Defects in oscillatory media towards a classification Bjrn - - PDF document

Defects in oscillatory media towards a classification Bjrn Sandstede (Ohio State University) Joint work with Arnd Scheel (U Minnesota) Modulated Waves x R , u R n u t = Du xx + f ( u ) , Defects and coherent structures:


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SLIDE 1

Defects in oscillatory media — towards a classification —

Björn Sandstede (Ohio State University) Joint work with Arnd Scheel (U Minnesota)

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SLIDE 2

Modulated Waves

ut = Duxx + f(u), x ∈ R, u ∈ Rn Defects and coherent structures:

  • time periodic in an appropriate moving frame
  • spatially asymptotic to periodic travelling waves

cd c−

p

c+

p

defect wave train wave train space time space time

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SLIDE 3

Coherent Structures in Experiments

CIMA-reaction [Perraud, De Wit, Dulos, De Kepper, Dewel, Borckmans] Heated-wire experiments [Pastur, Westra, van de Water] Period-doubled spiral wave Belousov–Zhabotinsky reaction [Yoneyama, Fujii, Maeda] Line defect [Goryachev, Kapral]

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SLIDE 4

Overview

Goals:

  • Multiplicity and robustness
  • Bifurcations from and to defects
  • Stability and interaction
  • Model-independent approach to coherent structures

Issues:

  • Defects are genuine PDE solutions
  • Essential spectrum touches the imaginary axis:

Outline:

  • Wave trains
  • Classification
  • Spatial dynamics
  • Multiplicity and robustness
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SLIDE 5

Wave Trains and Group Velocity

Reaction-diffusion system: ut = Duxx + f(u), x ∈ R, u ∈ Rn Wave trains u(x, t) = u0(kx − ωt; k) satisfy −ωuφ = k2Duφφ + f(u) Wave train u0(φ; k) = u0(φ + 2π; k) Temporal frequency ω = ωnl(k) Wave speed cp = ω/k Group velocity cg = dω/dk

cp cg phase velocity group velocity

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SLIDE 6

Spectra of Wave Trains

vt = Dvxx + f ′(u0(kx − ωt; k))v − → v(x, t) = eλt+νx vper(kx − ωt) Linear dispersion relation: λ = λ(ν) with ν ∈ iR Group velocity: cg = dω dk = −dλ dν

  • ν=0

Hypothesis: λ(iγ) Re λ Im λ Translational invariance implies that λ = 0 is contained in the spectrum: wave train u0 translation mode vper = ∂φu0

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SLIDE 7

Burgers Equation for Modulated Wave Trains

cg

Slowly-varying modulations of the wavenumber: u(x, t) = u0(kx − ωt + φ(X, T); k + ǫφX(X, T)) where X = ǫ(x − cgt), T = ǫ2t/2 and ǫ ≪ 1 Wavenumber q = φX satisfies viscous Burgers equation: ∂q ∂T = λ′′(0) ∂2q ∂X2 − ω′′

nl(k)

  • q2

X

Validity of Burgers equations over natural time scale [0, ǫ−2]: [Doelman, Sandstede, Scheel, Schneider]

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SLIDE 8

Classifi cation of Coherent Structures

  • time periodic in an appropriate moving frame
  • spatially asymptotic to wave trains

cd c−

g

c+

g

defect wave train wave train Sink c−

g > cd > c+ g

Contact defect c−

g = cd = c+ g

Transmission defect c±

g < cd

Source c−

g < cd < c+ g

  • Rankine–Hugoniot condition:

cd = ωnl(k+) − ωnl(k−) k+ − k−

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SLIDE 9

Spatial Dynamics

Reaction-diffusion system in (ξ, τ) = (x − cdt, ωdt): ωduτ = Duξξ + cduξ + f(u) Space-time plot for τ ∈ [0, 2π]:

space time

Modulated-wave equation for defects: d dξ   u v   =   v D−1[ωduτ − cdv − f(u)]   where (u, v)(ξ, ·) is time-periodic in τ with period 2π Defects are heteroclinic orbits that connect periodic orbits Key: Group velocity determines relative dimensions of stable and unstable manifolds of periodic orbits cg < cd cg = cd cg > cd 2

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Spatial Dynamics

Sinks Contact defects Transmission defects Sources

2

  • Sinks:
  • Wavenumbers (k−, k+) are free
  • Defect speed determined by Rankine–Hugoniot condition
  • Contact defects:
  • Wavenumber k− = k+ is free
  • Defect speed equal to group velocity
  • Transmission defects:
  • Wavenumber k− = k+ is free
  • Speed selected by defect

(Rankine–Hugoniot condition is violated)

  • Sources:
  • Defect speed and wavenumbers selected
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SLIDE 11

Floquet Spectra of Defects

Floquet spectra in L2(R):

Sink Contact Transmission Source

1 2 1

Floquet spectra in exponentially weighted spaces:

Sink Transmission Source Admissible functions in weighted spaces

1 2

Techniques:

  • Evans functions for waves with algebraic spatial decay
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SLIDE 12

Rigorous Justifi cation and Proofs

Modulated-wave equation: d dξ   u v   =   v D−1[ωduτ − cdv − f(u)]   Issues:

  • Spaces: (u, v) ∈ H

1 2 (S1) × L2(S1)

  • Initial-value problem is ill-posed
  • Both stable and unstable manifolds are infinite-dimensional
  • Contact defects: no asymptotic phase

− →

  • Exponential dichotomies to construct stable and unstable

manifolds for ill-posed elliptic equations

  • Relate Evans function in spatial dynamics to spectral stability
  • f defects

[Peterhof, Sandstede, Scheel], [Sandstede, Scheel]

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SLIDE 13

Comments:

  • Classifi cation extends counting arguments for complex

Ginzburg–Landau equations by [van Saarloos, Hohenberg]

  • Nonlinear stability:
  • Sinks (phase matching)
  • Transmission defects [Gallay, Schneider, Uecker]
  • Bifurcations to defects
  • Essential instabilities of standing and travelling pulses

− → sources and transmission defects

  • Small-amplitude shocks in Burgers equation −

→ sinks

  • Period doubling of homogeneous oscillations

− → sources and contact defects

  • Spatial inhomogeneities −

→ sources and contact defects

  • Bifurcations from defects:
  • Contact defects versus sinks
  • In general: homoclinic and heteroclinic bifurcations

Future Directions:

  • Nonlinear stability of sources and contact defects
  • Interactions of source-sinks pairs, transmission and contact defects:
  • Relevance of roots of Evans functions
  • Description by coupled ODEs and Burgers equations
  • First insights: Interaction on circles