Early Universe Dynamos from Neutrino Oscillations Induced by Torsion
Garcia de Andrade

TL;DR
This paper explores how neutrino oscillations induced by spacetime torsion could generate primordial magnetic fields, potentially seeding galactic magnetic fields and influencing early universe magnetism.
Contribution
It presents new models linking torsion and neutrino densities to cosmological magnetic seed fields, extending previous work on neutrino-induced magnetogenesis.
Findings
Torsion can generate seed magnetic fields of order 10^{-12} G at present day.
Relic magnetic fields of order 10^{39} G can originate from primordial nucleosynthesis conditions.
Weak fields torsion can slow magnetic field decay, supporting earlier theories.
Abstract
Earlier de Sabbata and Gasperini have shown that neutrinos oscillation which gives them a mass can be induced by torsion. More recently Enqvist et al have shown that it is possible to use massive neutrinos BBN magnetic fields to seed galactic magnetic fields. Thus based on these previous investigations we present several examples of how obtaining cosmological magnetic seed fields as galactic magnetic fields from massive neutrino densities and also from the torsion obtained by Nitsch as at the present day which yields magnetic seed field of the order of . In the case we use torsion derived from massive neutrinos given by one obtains in BBN time with the primordial nucleosynthesis magnetic field given by a relic magnetic field which…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Solar and Space Plasma Dynamics · Neutrino Physics Research
