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arXiv · astro-ph/9801262

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

Neven Bilic·Faustin Munyaneza·Raoul D. Viollier
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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.

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Neven Bilic, Faustin Munyaneza, Raoul D. Viollier. 1998-01-27. Stars and Halos of Degenerate Relativistic Heavy-Neutrino and Neutralino Matter. https://doi.org/10.1103/physrevd.59.024003

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