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Spectrum generating algebras for the classical Kepler problem

Aidan J Keane

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It is shown that the so(4, 2) spectrum generating algebra for the classical Kepler problem for non-zero energies can be obtained from the generators of the spacetime conformal group SO(4, 2). This is achieved by exploiting the equivalence of Kepler motion and null geodesic motion in conformally flat Einstein static spacetimes. We show that it is the existence of a time-dependent representation of the so(4, 2) spectrum generating algebra for null geodesic motion in the Einstein static spacetimes (originating from the so(4, 2) algebra of first integrals) which determines the corresponding spectrum generating algebra structure in the classical Kepler problem. Further, for the zero energy state, it is shown that only the iso(3) invariance subalgebra has a direct physical significance.


PACS

45.50.Pk Celestial mechanics

02.10.De Algebraic structures and number theory

02.20.Sv Lie algebras of Lie groups

02.40.Hw Classical differential geometry

MSC

22E60 Lie algebras of Lie groups (For the algebraic theory of Lie algebras, see 17Bxx)

70F15 Celestial mechanics

Subjects

Mathematical physics

Astrophysics and astroparticles

Dates

Issue 38 (27 September 2002)

Received 1 May 2002

Published 12 September 2002



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