Neutrino neutral current interactions in hot dense matter - INSPIRE

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Neutrino neutral current interactions in hot dense matter

C.J. Horowitz
(
- Indiana U.
)
,
K. Wehrberger
(
- Darmstadt, Tech. Hochsch.
)

1991

7 pages

Published in:

Phys.Lett.B 266 (1991) 236-242

Published: 1991

DOI:

10.1016/0370-2693(91)91032-Q

View in:

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Abstract: (Elsevier)

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.

neutrino electron: interaction
interaction: neutrino electron
neutrino nucleon: interaction
interaction: neutrino nucleon
neutral current
nuclear matter
finite temperature
Hartree-Fock approximation: relativistic
random phase approximation
astrophysics: supernova

References(13)

Figures(0)

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