engleski

Stars and halos of degenerate relativistic heavy-neutrino and neutralino matter

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.

neutrino ; neutralino ; Oppenheimer-Volkoff limit ; neutrino star ; MACHO ; galactic center ; dark matter

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