"Non-1/r" Newtonian gravitation and stellar structure

Details "Non-1/r" Newtonian gravitation and stellar structure "Non-1/r" Newtonian gravitation and stellar structure

1999-07-12

arxiv.org/abs/astro-ph/9907136v1

Astronomy and Astrophysics

Astrophysics

5 pages, 2 figures

Scientific paper

Some analytical spherical-symmetric equilibrium solutions are cosidered in
the Newtonian theory of gravitation with deviations from 1/r law. Stability of
star against a first-order phase-transition is shown to be particularly
influenced by the deviations of degree in the power-law potential.

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