Kolmogorov-Arnold-Moser Theorem

A theorem outlined by Kolmogorov (1954) which was subsequently proved in the 1960s by Arnol'd (1963) and Moser (1962; Tabor 1989, p. 105). It gives conditions under which chaos is restricted in extent. Moser's 1962 proof was valid for twist maps

theta^'=theta+2pif(I)+g(theta,I)
(1)
I^'=I+f(theta,I).
(2)

Arnol'd (1963) produced a proof for Hamiltonian systems

 H=H_0(I)+epsilonH_1(I).
(3)

The original theorem required perturbations epsilon∼10^(-48), although this has since been significantly increased. Arnol'd's proof required C^infty, and Moser's original proof required C^(333). Subsequently, Moser's version has been reduced to C^6, then C^(2+epsilon), although counterexamples are known for C^2. Conditions for applicability of the KAM theorem are:

1. small perturbations,

2. smooth perturbations, and

3. sufficiently irrational map winding number.

Moser considered an integrable Hamiltonian function H_0 with a torus T_0 and set of frequencies omega having an incommensurate frequency vector omega^* (i.e., omega·k!=0 for all integers k_i). Let H_0 be perturbed by some periodic function H_1. The KAM theorem states that, if H_1 is small enough, then for almost every omega^* there exists an invariant torus T(omega^*) of the perturbed system such that T(omega^*) is "close to" T_0(omega^*). Moreover, the tori T(omega^*) form a set of positive measures whose complement has a measure which tends to zero as |H_1|->0. A useful paraphrase of the KAM theorem is, "For sufficiently small perturbation, almost all tori (excluding those with rational frequency vectors) are preserved." The theorem thus explicitly excludes tori with rationally related frequencies, that is, n-1 conditions of the form

 omega·k=0.
(4)

These tori are destroyed by the perturbation. For a system with two degrees of freedom, the condition of closed orbits is

 sigma=(omega_1)/(omega_2)=r/s.
(5)

For a quasiperiodic map orbit, sigma is irrational. KAM shows that the preserved tori satisfy the irrationality condition

 |(omega_1)/(omega_2)-r/s|>(K(epsilon))/(s^(2.5))
(6)

for all r and s, although not much is known about K(epsilon).

The KAM theorem broke the deadlock of the small divisor problem in classical perturbation theory, and provides the starting point for an understanding of the appearance of chaos. For a Hamiltonian system, the isoenergetic nondegeneracy condition

 |(partial^2H_0)/(partialI_jpartialI_j)|!=0
(7)

guarantees preservation of most invariant tori under small perturbations epsilon<<1. The Arnol'd version states that

 |sum_(k=1)^nm_komega_k|>K(epsilon)(sum_(k=1)^n|m_k|)^(-n-1)
(8)

for all m_k in Z. This condition is less restrictive than Moser's, so fewer points are excluded.

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