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

Preprint

27 January 1998

preprint
Published by arXiv in arXiv

https://doi.org/10.48550/arXiv.astro-ph/9801262

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.

Keywords

DEGENERATE RELATIVISTIC
NEUTRINO AND NEUTRALINO
HYDROSTATIC EQUILIBRIUM
RELATIVISTIC HEAVY
NEUTRALINO MATTER
HEAVY NEUTRINO
HALOS
STARS

All Related Versions

Version 1, 1998-01-27, ArXiv
Published version: Physical Review D, 59 (2), 024003.

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