Cosmological abundances of right-handed Dirac neutrinos

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

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Talk given at the Neutrino '96 Conference. 5 pages, LaTeX, 3 ps figures included

Scientific paper

The equilibration of the right-helicity states $\nu_+$ of light Dirac-neutrinos is discussed. I point out that the $\nu_+$ production rate is enhanced by weak gauge boson pole effects so that the right-helicity component of $\nu_\tau$ is brought into equilibrium at $T\simeq 10$ GeV independently of the initial abundance, provided $m_{\nu_{\tau}}\gsim 10$ keV. Neutrino spin flip in primordial magnetic fields and the resulting bound on $\mu_\nu$ is also discussed.

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