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Instability of local deformations of an elastic filament

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Title: Instability of local deformations of an elastic filament


1
Instability of local deformations of an elastic
filament
  • with
  • S. Lafortune S. Madrid-Jaramillo
  • Department of Mathematics
  • University of Arizona

S. Lafortune J.L., Physica D 182, 103-124
(2003)S. Lafortune J.L., submitted to SIMA S.
Lafortune, J.L. S. Madrid-Jaramillo, submitted
to Chaos
University of Arizona
Tucson
AZ
2
Outline
  • Motivations
  • Dynamics of an elastic filament
  • The coupled Klein-Gordon equations
  • Special solutions and numerical simulations of
    pulse solutions
  • Evans function methods S. Lafortune J.L.,
    Physica D 182, 103-124 (2003)
  • Linearization about pulse solutions
  • Behavior of the Evans function at the origin
  • Behavior of the Evans function at infinity
  • Instability criterion
  • Numerical evaluation of the Evans functionS.
    Lafortune, J.L. S. Madrid-Jaramillo, submitted
    to Chaos
  • Hamiltonian formalism S. Lafortune J.L,
    submitted to SIMA
  • Hamiltonian form of the coupled Klein-Gordon
    equations
  • Spectral stability criterion
  • Conclusions

3
Dynamic of an elastic filament
  • Consider an elastic filament kept under tension
    and subject to constant twist
  • There is a critical value of the applied twist
    above which the filament undergoes a writhing
    bifurcation

4
Description of near-threshold dynamics
Reconstructionof elastic filament
Near-thresholddynamics
Envelope equations
5
The coupled Klein-Gordon equations
  • They describe the near-threshold dynamics of an
    elastic filament subject to sufficiently high
    constant twist
  • Dimensionless form of the equationsA
    complex envelope of helical modeB axial
    twistA. Goriely M. Tabor, Nonlinear dynamics
    of filaments II Nonlinear analysis, Physica D
    105, 45-61 (1997).

6
Some special solutions
  • Traveling holes
  • Traveling fronts
  • Periodic solutions
  • Traveling pulses

J.L. A. Goriely, Pulses, fronts and
oscillations of an elastic rod, Physica D 132,
373-391 (1999).
7
Traveling pulse solutions
  • Analytic expression

J.L. A. Goriely, Pulses, fronts and
oscillations of an elastic rod, Physica D 132,
373-391 (1999).
8
Numerical simulations of pulse solutions
  • Numerical simulation
  • Non-reflecting boundary conditions
  • Compact finite differences Runge-Kutta in
    time
  • J.L. A. Goriely, Pulses, fronts and
    oscillations of an elastic rod, Physica D 132,
    373-391 (1999).

9
Question
  • Numerical simulations indicate that some pulses
    are stable and some are not
  • Can one find a criterion which guarantees the
    instability of the pulse solutions? If so, this
    condition should depend on the speed of
    propagation c of each pulse
  • Below, we present two complementary ways - Evans
    function methods and Hamiltonian techniques - of
    answering this question

10
Outline
  • Motivations
  • Dynamics of an elastic filament
  • The coupled Klein-Gordon equations
  • Special solutions and numerical simulations of
    pulse solutions
  • Evans function methods S. Lafortune J.L.,
    Physica D 182, 103-124 (2003)
  • Linearization about pulse solutions
  • Behavior of the Evans function at the origin
  • Behavior of the Evans function at infinity
  • Instability criterion
  • Numerical evaluation of the Evans functionS.
    Lafortune, J.L. S. Madrid-Jaramillo, submitted
    to Chaos
  • Hamiltonian formalism S. Lafortune J.L,
    submitted to SIMA
  • Hamiltonian form of the coupled Klein-Gordon
    equations
  • Spectral stability criterion
  • Conclusions

11
Linear stability analysis of the pulse solutions
  • Coupled Klein-Gordon equations
  • Pulse solutions

12
Linearization about the pulse solutions
  • Write
    where a and b correspond to a pulse solution
  • Obtain a linearized system of the form where

    is a six-dimensional vector and L is a
    differential operator in x
  • Define an eigenfunction of L with eigenvalue l as
    a solution Y of L Y l Y such that
    (u,u,w)?(H1H1L?)?(C1C1C1) The equation L Y
    l Y can be writtenas a six-dimensional system of
    the form

13
The Evans function
  • An eigenfunction exists if the two vector spaces
    of solutions of X A(x, l) X that are bounded
    at ? and ? intersect non-trivially
  • Typically, this only happens for particular
    values of l
  • The Evans function E(l) is an analytic function
    of l, which is real-valued for l real and which
    vanishes on the point spectrum of L
  • It can be viewed as the Wronskian, calculated for
    instance at x 0, of linearly independent
    solutions of X A(x, l) X that converge at ?
    and linearly independent solutions of X
    A(x, l) X that converge at ?

14
The Evans function
  • References
  • J.W. Evans, Nerve axon equations. IV. The stable
    and unstable impulse, Indiana Univ. Math. J. 24,
    1169-1190 (1975).
  • C.K.R.T. Jones, Stability of the travelling wave
    solution to the FitzHugh-Nagumo equation, Trans.
    AMS 286, 431-469 (1984).
  • E. Yanagida, Stability of fast traveling pulse
    solutions to the FitzHugh-Nagumo equations, J.
    Math. Biol. 22, 81-104 (1985).
  • J. Alexander, R. Gardner C. Jones, A
    topological invariant arising in the stability
    analysis of travelling waves, J. Reine Angew.
    Math. 410, 167-212 (1990).
  • R. Pego M. Weinstein, Eigenvalues, and
    instabilities of solitary waves, Phil. Trans. R.
    Soc. London A 340, 47-94 (1992).
  • R.A. Gardner K. Zumbrun, The Gap Lemma and
    geometric criteria for instability of viscous
    shock profiles, Commun. Pure Appl. Math. LI,
    0797-0855 (1998).
  • T. Kapitula B. Sandstede, Stability of bright
    solitary-wave solutions to perturbed nonlinear
    Schrödinger equations, Physica D 124, 58-103
    (1998).
  • B. Sandstede, Stability of travelling waves, in
    Handbook of Dynamical Systems II Towards
    Applications, pp. 983-1055, B. Fielder Ed.,
    Elsevier, 2002.

15
The Evans function
  • As x ? ?, A(x, l) ? A0(l), where the matrix
    A0(l) has constant coefficients
  • If the deviator
    converges and if the asymptotic matrix A0(l) is
    diagonalizable, then for each (wi,ni) such that
    A0(l) wi ni wi , there is a solution Fi(x,l) to
    X A(x, l) X such that
  • Moreover, if the convergence of the deviator is
    uniform in l on compact subsets of the complex
    plane, one can find solutions Fi(x,l) which are
    analytic in l in some subset of the complex plane
  • E. Coddington N. Levinson, Theory of
    Ordinary Differential Equations, McGraw-Hill,
    New-York (1955).

16
The Evans function
  • When l gt 0, the asymptotic matrix A0(l) has 3
    positive and 3 negative eigenvalues
  • We define the Evans function E(l) bywhere
  • We look for a criterion, involving the speed of
    the traveling pulse, which guarantees that E(l)
    vanishes on the real axis. This is done by
    comparing the sign of E(l) near the origin with
    its sign for large positive values of the
    spectral parameter l

17
Behavior of E(l) near the origin
  • The Evans function, as well as its first four
    derivatives, vanish at l 0
  • The fifth derivative has to be computed by
    finding expansions of the Fi(x,l) in powers of l
  • Because of the symmetry B ? B constant of the
    original nonlinear Klein-Gordon equations, two of
    the Fi(x,l) are bounded at l 0, and singular
    expansions of the form are needed in this
    particular case
  • The fifth derivative of the Evans function at l
    0 is given by

18
Behavior of E(l) at infinity
  • The change of variable z l x, turns the system
    X A(x, l) X into X Ã(z, l) X
  • As l ? ?, Ã(z, l) converges uniformly toward a
    matrix Ã0, which has constant coefficients
  • Because X Ã(z, l) X has an exponential
    dichotomy for l large, its solutions are
    uniformly close to solutions of X Ã0 X for l
    large enough
  • The sign of E(l) for l large is therefore the
    same as the sign of the Evans function
    associated with X Ã0 X, provided the basis
    vectors are arranged in the same order
  • One finds

19
Instability criterion
  • For l positive and small,
  • For m gt 0, the asymptotic state of the pulse is
    unstable to plane waves perturbations, so we
    assume m lt 0. Then, E(l) is negative for l
    positive and large
  • Therefore, E(l) vanishes for a real positive
    value of l if

    , which can be
    rewritten as
  • In the numerical simulation shown before, T
    27.078 lt 0

20
Numerical evaluation of the Evans function
  • One can numerically evaluate the Evans function
    for l on the real axis and see how E(l) changes
    as c2 gets close to K
  • Below,

S. Lafortune, J.L. S. Madrid-Jaramillo,
Instability of local deformations of an elastic
rod numerical evaluation of the Evans function,
submitted to Chaos.
21
Numerical evaluation of the Evans function
  • Contour integration in the complex plane can also
    be used to detect the zeros of the Evans function
    in a region near the origin
  • Here, the winding number is equal to 6 for

S. Lafortune, J.L. S. Madrid-Jaramillo,
Instability of local deformations of an elastic
rod numerical evaluation of the Evans function,
submitted to Chaos.
22
Outline
  • Motivations
  • Dynamics of an elastic filament
  • The coupled Klein-Gordon equations
  • Special solutions and numerical simulations of
    pulse solutions
  • Evans function methods S. Lafortune J.L.,
    Physica D 182, 103-124 (2003)
  • Linearization about pulse solutions
  • Behavior of the Evans function at the origin
  • Behavior of the Evans function at infinity
  • Instability criterion
  • Numerical evaluation of the Evans functionS.
    Lafortune, J.L. S. Madrid-Jaramillo, submitted
    to Chaos
  • Hamiltonian formalism S. Lafortune J.L,
    submitted to SIMA
  • Hamiltonian form of the coupled Klein-Gordon
    equations
  • Spectral stability criterion
  • Conclusions

23
Hamiltonian formalism
  • The coupled nonlinear Klein-Gordon equations form
    a Hamiltonian system

J.L. A. Goriely, Pulses, fronts and
oscillations of an elastic rod, Physica D 132,
373-391 (1999)
24
Hamiltonian formalism
  • If v0 corresponds to a pulse solution, then the
    linearization of the Hamiltonian system about v0
    is of the formwhere Hc,w is self-adjoint
  • The idea is to use the fact that the spectrum of
    Hc,w is relatively simpler to analyze, to get
    information on the spectrum of J Hc,w
  • M. Grillakis, J. Shatah and W. Strauss, Stability
    theory of solitary waves in the presence of
    symmetry, I, J. Functional Analysis 74, 160-197
    (1987)
  • M. Grillakis, J. Shatah and W. Strauss, Stability
    theory of solitary waves in the presence of
    symmetry, II, J. Functional Analysis 94, 308-348
    (1990)

25
Hamiltonian formalism
  • Assume that the continuous spectrum of Hc,w is
    positive and bounded away from the origin, and
    that the Hilbert space in which perturbations
    live is the direct sum of the kernel, positive
    and negative subspaces of Hc,w.
  • Let d(c,w) E(v0) cQ1(v0)
    wQ2(v0),where v0 corresponds to the pulse
    solution, Q1(v0) is the conserved quantity
    associated with translational invariance and
    Q2(v0) is the conserved quantity associated with
    gauge invariance.
  • Let d?(c,w) be non-singular, n(Hc,w) be the
    dimension of the negative subspace of Hc,w, and
    p(d?) be the number of positive eigenvalues of
    the Hessian of d.

26
Hamiltonian formalism
  • Theorem (M. Grillakis, J. Shatah and W. Strauss)
  • If n(Hc,w) p(d?) is odd, then J Hc,w has at
    least one pair of real non-zero eigenvalues.
  • If n(Hc,w) p(d?), then pulse solutions are
    (orbitally) stable.
  • M. Grillakis, J. Shatah and W. Strauss, Stability
    theory of solitary waves in the presence of
    symmetry, II, J. Functional Analysis 94, 308-348
    (1990)

27
Hamiltonian formalism
  • Here, one can prove that n(Hc,w) 1
  • But the continuous spectrum of Hc,w touches the
    origin, so the above theorem is not directly
    applicable
  • However, one has the following result
  • Let d?(c,w) be non-singular. Then, pulses are
    spectrally stable if and only if
  • S. Lafortune J.L., Spectral stability of local
    deformations of an elastic rod Hamiltonian
    formalism, submitted to SIMA

28
Hamiltonian formalism
  • This condition reads
  • In the case w 0, this is consistent with the
    instability criterion obtained by means of Evans
    function techniques

29
Summary spectrum of linearized operator
30
Conclusions
  • Instability of pulse solutions to the coupled
    nonlinear Klein-Gordon equations
  • Numerical simulations show that both stable and
    unstable pulses exist
  • This analysis indicates that pulses propagating
    at the speed c are spectrally stable if and only
    if c2 is less than K ? c02
  • Evans function techniques
  • The Evans function as well as its first 4
    derivatives vanish at the origin
  • The spaces of solutions which are bounded at plus
    infinity and at minus infinity are 3-dimensional

31
Conclusions
  • Evans function techniques
  • Regular and singular perturbation expansions of
    the solutions in powers of l are needed to
    calculate the fifth derivative of the Evans
    function at the origin
  • The sign of the Evans function for large and
    positive values of the spectral parameter is
    found by calculating the Evans function of a
    system with constant coefficients (obtained after
    a suitable change of variable)
  • Analytical results can be complemented by a
    numerical evaluation of the Evans function

32
Conclusions
  • Hamiltonian formalism
  • Because the coupled Klein-Gordon form a
    Hamiltonian system, it is possible to obtain a
    necessary and sufficient condition for spectral
    stability
  • Classical Hamiltonian methods have to be adapted
    to this case because the continuous spectrum of
    the modified Hamiltonian touches the origin
  • It may be possible to obtain strong stability
    results provided the perturbations live in a
    different space

33
Conclusions
  • Hamiltonian formalism
  • Because the coupled Klein-Gordon form a
    Hamiltonian system, it is possible to obtain a
    necessary and sufficient condition for spectral
    stability
  • Classical Hamiltonian methods have to be adapted
    to this case because the continuous spectrum of
    the modified Hamiltonian touches the origin
  • It may be possible to obtain strong stability
    results provided the perturbations live in a
    different space

34
Symmetries
  • The coupled Klein-Gordon equations are
  • Invariant under space translations
  • Gauge invariant
  • Invariant under B ? B constant
  • Two-parameter family pulse of solutions
  • The speed c is associated with the space
    translation invariance
  • The frequency w is associated with the gauge
    invariance

35
Traveling pulse solutions
  • Analytic expression

J.L. A. Goriely, Pulses, fronts and
oscillations of an elastic rod,Physica D 132,
373-391 (1999).
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