Other
Scientific paper
Jun 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984cemec..33..159s&link_type=abstract
Celestial Mechanics (ISSN 0008-8714), vol. 33, June 1984, p. 159-167.
Other
Equilibrium Methods, Hamiltonian Functions, Linear Systems, Systems Stability, Celestial Mechanics, Degrees Of Freedom, Perturbation Theory, Resonance
Scientific paper
The equilibrium point O of an autonomous Hamiltonian system of two degrees of freedom is considered for small-oscillation frequencies related as ω2 = 2ω1+ɛ. If under the precise resonance (ɛ = 0) the equilibrium is unstable, the inner diameter η(ɛ) of the domain of stability containing the point O is estimated. It is shown that for the normalized variables η(ɛ) ≤ ɛ/b where b is the corresponding resonance coefficient. The estimates of η(ɛ) for other main resonances are reported.
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