Stars and Halos of Degenerate Relativistic Heavy-Neutrino and Neutralino Matter

Details Stars and Halos of Degenerate Relativistic Heavy-Neutrino and Neutralino Matter Stars and Halos of Degenerate Relativistic Heavy-Neutrino and Neutralino Matter

1998-01-27

arxiv.org/abs/astro-ph/9801262v1

Phys.Rev. D59 (1999) 024003

Astronomy and Astrophysics

Astrophysics

10 pages, 5 ps-figures, RevTex

Scientific paper

10.1103/PhysRevD.59.024003

Heavy-neutrino (or neutralino) stars are studied using the general relativistic equations of hydrostatic equilibrium and the relativistic equation of state for degenerate fermionic matter. The Tolman-Oppenheimer-Volkoff equations are then generalized to include a system of degenerate neutrino and neutralino matter that is gravitationally coupled. The properties and implications of such an interacting astrophysical system are discussed in detail.

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