Neutrino flavor transformation in the lepton-asymmetric universe

Lucas Johns, Mattia Mina, Vincenzo Cirigliano, Mark W. Paris, and George M. Fuller
Phys. Rev. D 94, 083505 – Published 4 October 2016

Abstract

We investigate neutrino flavor transformation in the early Universe in the presence of a lepton asymmetry, focusing on a two-flavor system with 1–3 mixing parameters. We identify five distinct regimes that emerge in an approximate treatment neglecting collisions as the initial lepton asymmetry at high temperature is varied from values comparable to current constraints on the lepton number down to values at which the neutrino-neutrino forward-scattering potential is negligible. The characteristic phenomena occurring in these regimes are (1) large synchronized oscillations, (2) minimal flavor transformation, (3) asymmetric (ν- or ν¯-only) MSW, (4) partial MSW, and (5) symmetric MSW. We examine our numerical results in the framework of adiabaticity, and we illustrate how they are modified by collisional damping. Finally, we point out the existence of matter-neutrino resonances in the early Universe and show that they suffer from nonadiabaticity.

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  • Received 8 August 2016

DOI:https://doi.org/10.1103/PhysRevD.94.083505

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsParticles & Fields

Authors & Affiliations

Lucas Johns1,2,*, Mattia Mina2,3, Vincenzo Cirigliano2, Mark W. Paris2, and George M. Fuller1

  • 1Department of Physics, University of California, San Diego, La Jolla, California 92093, USA
  • 2Theoretical Divison, Los Alamos National Laboratory, Los Alamos, New Mexico 87545, USA
  • 3Department of Physics, University of Torino, Via P. Giuria 1, I—10125 Torino, Italy

  • *ljohns@physics.ucsd.edu

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Issue

Vol. 94, Iss. 8 — 15 October 2016

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