Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2009-09-22
Nucl.Phys.Proc.Suppl.188:264-266,2009
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Belated posting of contribution to NOW 2008 proceedings. 3 pages
Scientific paper
10.1016/j.nuclphysbps.2009.02.06
The calculation of neutrino decoupling from nuclear matter requires a transport formalism capable of handling both collisions and flavor mixing. The first steps towards such a formalism are the construction of neutrino and antineutrino "distribution matrices," and a determination of the Liouville equations they satisfy in the noninteracting case. These steps are accomplished through study of a Wigner-transformed "density function," the mean value of paired neutrino quantum field operators.
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