Title of article
Quantum leptogenesis I Original Research Article
Author/Authors
A. Anisimov، نويسنده , , W. Buchmuller، نويسنده , , M. Drewes، نويسنده , , S. Mendizabal، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2011
Pages
41
From page
1998
To page
2038
Abstract
Thermal leptogenesis explains the observed matter–antimatter asymmetry of the universe in terms of neutrino masses, consistent with neutrino oscillation experiments. We present a full quantum mechanical calculation of the generated lepton asymmetry based on Kadanoff–Baym equations. Origin of the asymmetry is the departure from equilibrium of the statistical propagator of the heavy Majorana neutrino, together with CP violating couplings. The lepton asymmetry is calculated directly in terms of Green’s functions without referring to “number densities”. Compared to Boltzmann and quantum Boltzmann equations, the crucial difference are memory effects, rapid oscillations much faster than the heavy neutrino equilibration time. These oscillations strongly suppress the generated lepton asymmetry, unless the standard model gauge interactions, which cause thermal damping, are properly taken into account. We find that these damping effects essentially compensate the enhancement due to quantum statistical factors, so that finally the conventional Boltzmann equations again provide rather accurate predictions for the lepton asymmetry.
Keywords
Thermal field theory , Nonequilibrium , Particle physics , Leptogenesis , Cosmology
Journal title
Annals of Physics
Serial Year
2011
Journal title
Annals of Physics
Record number
1206494
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