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Space-time propagation of neutrino wave packets at high temperature and density

C. M. Ho* and D. Boyanovsky†

  • Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania 15260, USA

  • *Electronic address: cmho@phyast.pitt.edu
  • †Electronic address: boyan@pitt.edu
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Phys. Rev. D 73, 125014 – Published 14 June, 2006

DOI: https://doi.org/10.1103/PhysRevD.73.125014

Abstract

We study the space-time evolution of “flavor” neutrino wave packets at finite temperature and density in the early Universe prior to big bang nucleosynthesis (BBN). We implement nonequilibrium field theory methods and linear response to study the space-time evolution directly from the effective Dirac equation in the medium. There is a rich hierarchy of time scales associated with transverse and longitudinal dispersion and coherence. A phenomenon of “freezing of coherence” is a result of a competition between longitudinal dispersion and the separation of wave packets of propagating modes in the medium. Near a resonance the coherence and oscillation time scales are enhanced by a factor 1/sin2θ compared to the vacuum. Collisional relaxation via charged and neutral currents occurs on time scales much shorter than the coherence time scale and for small vacuum mixing angle, shorter than the oscillation scale. Assuming that the momentum spread of the initial wave packet is determined by the large angle scattering mean free path of charged leptons, we find that the transverse dispersion time scale is the shortest and is responsible for a large suppression in both the survival and transition probabilities on time scales much shorter than the Hubble time. For small mixing angle the oscillation time scale is longer than the collisional relaxation scale. The method also yields the evolution of right-handed wave packets. Corrections to the oscillation frequencies emerge from wave-packet structure as well as from the energy dependence of mixing angles in the medium.

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Phys. Rev. D 73, 125014– Published 14 June, 2006
  • Received 5 April 2006

© 2006 American Physical Society

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