The Neutrino Ball Model of a Quasar

R. Manka; I. Bednarek; D. Karczewska

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arXiv · astro-ph/9304007

The Neutrino Ball Model of a Quasar

R. Manka·I. Bednarek·D. Karczewska

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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.

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R. Manka, I. Bednarek, D. Karczewska. 1993-04-07. The Neutrino Ball Model of a Quasar. https://arxiv.org/abs/astro-ph/9304007

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