Neutrino neutral current interactions in hot dense matter

Details Neutrino neutral current interactions in hot dense matter Neutrino neutral current interactions in hot dense matter

Aug 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phlb..266..236h&link_type=abstract

Physics Letters B, Volume 266, Issue 3-4, p. 236-242.

Physics

24

Scientific paper

The response function for neutrino neutral current interactions are evaluated at finite temperature for a dense medium of electrons, protons and neutrons. We use real-time finite-temperature field theory. The ground state is described by the relativistic Hartree approximation to the σω model of quantum hadrodynamics. We compare the uncorrelated response with the response in random-phase approximation and discuss the influence of vacuum contributions. Results are presented for typical astrophysical scenarios in supernova collapse and neutron star cooling.

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