The Neutrino Ball Model of a Quasar
Abstract
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.
Cite
@article{arxiv.astro-ph/9304007,
title = {The Neutrino Ball Model of a Quasar},
author = {R. Manka and I. Bednarek and D. Karczewska},
journal= {arXiv preprint arXiv:astro-ph/9304007},
year = {2019}
}
Comments
10, Latex, psbox, 3 figures, USL-TH-93-01