The Neutrino Ball Model of a Quasar

Details The Neutrino Ball Model of a Quasar The Neutrino Ball Model of a Quasar

1993-04-07

arxiv.org/abs/astro-ph/9304007v1

Astronomy and Astrophysics

Astrophysics

10, Latex, psbox, 3 figures, USL-TH-93-01

Scientific paper

It is suggested that the nonorthodox model of a quasar as a neutrino ball described in terms of the standard model extended by adding right-handed neutrinos and the Majorana scalar field can be presented in order to explain a quasar as a body of weak interacting neutrinos. Neutrino interaction with the scalar Majorana field violates the lepton number and produces the mass splitting of the neutrino due to the sea-saw mechanism. In this model a quasar is an object which appears in the result of the first order cosmological phase transition. In this interpretation a quasar may be regarded as a ball filled with Dirac neutrinos and can be treated as a remnant of phase transition with unbroken global lepton symmetry. In this paper we study the macroscopic parameters of such a configuration. In the result the mass-radius curve M(R) for the quasar is obtained.

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