On relativistic discs and rings

Details On relativistic discs and rings On relativistic discs and rings

1997-01-14

arxiv.org/abs/astro-ph/9701071v1

Astronomy and Astrophysics

Astrophysics

9 pages, requires mn.sty and epsf.sty, 12 figures included, accepted by Monthly Notices of the Royal Astronomical Society

Scientific paper

Sequences of infinitesimally thin, uniformly rotating, self-gravitating relativistic discs with internal two-dimensional pressure have been constructed. It is shown that in weaker relativistic configurations the sequences undergo a continuous bifurcation from a disc to a ring structure, while in stronger relativistic cases the sequences terminate at the mass-shed limit where gravitational forces are exactly balanced by centrifugal forces.

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