Neutrino-nucleon scattering rate in the relativistic random phase approximation

Abstract

The in-medium modification to the neutrino-nucleon scattering rate is calculated in the relativistic random phase approximation in the framework of a hadronic meson exchange model, in view of applications to neutrino transport in supernovae and protoneutron stars

4 pages, 2 figures, to appear in the Proceedings of the PANIC02 conference, 30 sept - 4 oct 2002, Osaka, Japan

References in corpus (1)

• Collective multipole excitations in a microscopic relativistic approach

Cited by in corpus (5)

• Neutrinos and nucleosynthesis of elements
• Neutrino mean free path in neutron stars
• Isovector Channel Role of Relativistic Mean Field Models in the Neutrino Mean Free Path
• Neutrino Electromagnetic Form Factors Effect on the Neutrino Cross Section in Dense Matter
• Neutron Fraction and Neutrino Mean Free Path Predictions in Relativistic Mean Field Models