Floquet theory

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Floquet theory is a branch of the theory of ordinary differential equations relating to the class of solutions to linear differential equations of the form,

\dot{x} = A(t) x,\,

with \displaystyle A(t) a continuous periodic function with period T.

The main theorem of Floquet theory, Floquet's theorem (named after Gaston Floquet), gives a canonical form for each fundamental matrix solution of this common linear system. It gives a coordinate change \displaystyle y=Q^{-1}(t)x with \displaystyle Q(t+2T)=Q(t) that transforms the periodic system to a traditional linear system with constant, real coefficients.

In solid-state physics, the analogous result (generalized to three dimensions) is known as Bloch's theorem.

Note that the solutions of the linear differential equation form a vector space. A Matrix φ(t) is called a fundamental matrix solution if all columns are linearly independent solutions. It is called a principal fundamental matrix at t0 if φ(t0) is the identity. Because of existence and uniqueness of the solutions there is a principal fundamental matrix Φ(t0) = φ(t− 1(t0) for each t0. The solution of the linear differential equation with the initial condition x(0) = x0 is x(t) = φ(t− 1(0)x0 where φ(t) is any fundamental matrix solution.

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[edit] Floquet's theorem

If φ(t) is a fundamental matrix solution of the periodic system \dot{x}= A(t) x, with A(t) a periodic function with period T then, for all t \in \mathbb{R},

φ(t + T) = φ(t− 1(0)φ(T).

In addition, for each matrix B (possibly complex) such that:

eTB = φ − 1(0)φ(T),

there is a periodic (period T) matrix function t \to P(t) such that

φ(t) = P(t)etB for all t \in \mathbb{R}.

Also, there is a real matrix R and a real periodic (period 2T) matrix function t \to Q(t) such that

φ(t) = Q(t)etR for all t \in \mathbb{R}.

[edit] Consequences and applications

This mapping φ(t) = Q(t)etR gives rise to a time-dependent change of coordinates (y = Q − 1(t)x), under which our original system becomes a linear system with real constant coefficients \dot{y} = R y. Since Q(t) is continuous and periodic it must be bounded. Thus the stability of the zero solution for y(t) and x(t) is determined by the eigenvalues of R.

The representation φ(t) = P(t)etB is called a Floquet normal form for the fundamental matrix φ(t).

The eigenvalues of eTB are called the characteristic multipliers of the system. They are also the eigenvalues of the (linear) Poincaré maps x(t) \to x(t+T). A Floquet exponent (sometimes called a characteristic exponent), is a complex μ such that eμT is a characteristic multiplier of the system. Notice that Floquet exponents are not unique, since e^{(\mu + \frac{2 \pi i k}{T})T}=e^{\mu T}, where k is an integer. The real parts of the Floquet exponents are called Lyapunov exponents. The zero solution is asymptotically stable if all Lyapunov exponents are negative, Lyapunov stable if the Lyapunov exponents are nonpositive and unstable otherwise.

[edit] Floquet's theorem applied to Mathieu equation

Mathieu's equation is related to the wave equation for the elliptic cylinder.

Given a \in \mathbb{R}, q \in \mathbb{C}, the Mathieu equation is given by

\frac {d^2 y} {dw^2} +(a-2q \cos 2w )y=0.

The Mathieu equation is a linear second-order differential equation with periodic coefficients.

One of the most powerful results of Mathieu's functions is the Floquet's Theorem [1, 2]. It states that periodic solutions of Mathieu equation for any pair (a, q) can be expressed in the form

y(w) = Fν(w) = ejwνP(w) or
y(w) = Fν( − w) = e jwνP( − w),

where ν is a constant depending on a and q and P(.) is π-periodic in w.

The constant ν is called the characteristic exponent.

If ν is an integer, then Fν(w) and Fν( − w) are linear dependent solutions. Furthermore,

y(w + kπ) = ejνkπy(w) or y(w + kπ) = e jνkπy(w), for the solution Fν(w) or Fν( − w), respectively.

We assume that the pair (a, q) is such that | coshjνπ | < 1 so that the solution y(w) is bounded on the real axis. General solution of Mathieu's equation (q \in \mathbb{R}, ν non-integer) is the form

y(w) = c1ejwνP(w) + c2e jwνP( − w),

where c1 and c2 are arbitrary constants.

All bounded solutions --those of fractional as well as integral order-- are described by an infinite series of harmonic oscillations whose amplitudes decrease with increasing frequency.

Another very important property of Mathieu's functions is the orthogonality [3]:

If a(ν + 2p,q) and a(ν + 2s,q) are simple roots of cosπν – y(π) = 0, then:

\int_0^{\pi} F_{\nu+2p} (w).F_{\nu+2s}(-w) dw=0,  p \ne s, i.e.,

\langle F_{\nu +2p} (w),F_{\nu +2s} (w)\rangle,  p \ne s, where <.,.> denote an inner product defined from 0 to π.

[edit] References

  • Chicone, Carmen. Ordinary Differential Equations with Applications. Springer-Verlag, New York 1999
  • Gaston Floquet, "Sur les équations différentielles linéaires à coefficients périodiques," Ann. École Norm. Sup. 12, 47-88 (1883).
  • N.W. McLachlan, Theory and Application of Mathieu Functions, New York: Dover, 1964.
  • Gerald Teschl, Ordinary Differential Equations and Dynamical Systems, http://www.mat.univie.ac.at/~gerald/ftp/book-ode/