arXiv:astro-ph/9801262·v1·Astrophysics
Stars and Halos of Degenerate Relativistic Heavy-Neutrino and Neutralino Matter
Neven Bilic (Rudjer Boskovic Institute, Zagreb, Croatia)🇿🇦 · Faustin Munyaneza🇿🇦 · Raoul D. Viollier (University of Cape Town, South Africa)🇿🇦
Abstract
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.
Comments: 10 pages, 5 ps-figures, RevTex