lepton number survival in the cosmic neutrino background
Oleg Ruchayskiy, Vsevolod Syvolap, Robin Wursch

TL;DR
This paper investigates whether primordial lepton asymmetry in the cosmic neutrino background could survive until today, considering neutrino mass effects and helicity-flipping processes.
Contribution
It provides an analysis of helicity-flipping rates for massive neutrinos, showing that relic lepton asymmetry can persist in the current epoch under realistic conditions.
Findings
Lepton asymmetry can survive in the cosmic neutrino background.
Helicity-flipping rates are low enough to preserve asymmetry.
Massive neutrinos do not fully erase primordial asymmetries.
Abstract
The Hot Big Bang model predicts the existence of a \emph{cosmic neutrino background}. The number of particles and anti-particles in this primordial bath of neutrinos can be different -- a memory of processes that took place at very early epochs. If neutrinos were massless, this asymmetry would not change once neutrinos froze out. However, in the case of massive particles, the asymmetry is not protected by conservation laws and can get erased via helicity-flipping scatterings off matter inhomogeneities. We evaluate this helicity-flipping rate and demonstrate that if relic lepton asymmetry ever existed, it would remain largely intact in the Earth's neighborhood for realistic values of neutrino masses.
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Taxonomy
TopicsParticle physics theoretical and experimental studies · Dark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories
