Novel Scenarios for Majorana Neutrino Mass Generation and Leptogenesis from Kalb-Ramond Torsion

TL;DR

This paper explores how Kalb-Ramond antisymmetric tensor fields, arising in string theory, can generate Majorana neutrino masses and induce leptogenesis through torsion backgrounds, with implications for dark matter and early universe physics.

Contribution

It introduces novel scenarios where Kalb-Ramond torsion backgrounds lead to neutrino mass generation and leptogenesis, connecting string theory fields to cosmological phenomena.

Findings

KR axion fluctuations can generate Majorana neutrino masses.

Constant KR torsion backgrounds can induce leptogenesis via CP violation.

Potential realization of these scenarios in D-brane string models.

Abstract

The Kalb-Ramond (KR) antisymmetric tensor field arises naturally in the gravitational multiplet of string theory. Nevertheless, the respective low-energy field theory action, in which, for reasons of gauge invariance, the only dependence on the KR field is through its field strength, constitutes an interesting model \emph{per se}. In this context, the KR field strength also acts as a totally antisymmetric torsion field, while in four space-time dimensions is \emph{dual} to an (KR) axion-like pseudoscalar field. In this context, we review here first the r\^ole of quantum fluctuations of the KR axion on the generation of Majorana mass for neutrinos, via a mixing with ordinary axions that may exist in the theory as providers of dark matter candidates. Then we proceed to discuss the r\^ole of constant in time (thus Lorentz violating) KR torsion backgrounds, that may exist in the early Universe but are completely negligible today, on inducing Leptogenesis by means of \emph{tree-level} CP violating decays of Right Handed Massive Majorana neutrinos in the presence of such H-torsion backgrounds. Some speculations regarding microscopic D-brane world models, where such scenarios may be realised, are also given.