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. 
Neven Bilic (Rudjer Boskovic Institute, Zagreb, Croatia), Faustin   Munyaneza, Raoul D. Viollier (University of Cape Town, S...