Neutrino-electron scattering in dense magnetized plasma

1996/08/14 by V. G. Bezchastnov, Victor G. Bezchastnov, P. Haensel · 6 citations
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Neutrino Physics Research #Quantum, superfluid, helium dynamics #astro-ph

paper · pdf · doi:10.1103/physrevd.54.3706

published as Phys.Rev. D54 (1996) 3706-3721 · Physical Review D, to be published, 18 pages, using REVTEX, without figures. Figures (hardcopy) available upon request from one of the authors ([email protected])

arxiv created 1996/08/14 · openalex publication_date 1996/09/15 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

We derive exact expressions for the cross section of neutrino scattering on electrons in dense, hot stellar matter, in the presence of strong magnetic fields. Numerical calculations of the scattering cross sections at various densities, temperatures and magnetic fields, are performed. Strong, quantizing magnetic fields modify significantly the angular and energy dependence of the scattering cross section.

Citations

• Stellar core collapse - Numerical model and infall epoch

Cited by

• Neutron star equation of state and the possibility of complex self-energy in Landau theory of a Fermi liquid in the presence of a strong, quantizing magnetic field
• Energy and momentum losses in the process of neutrino scattering on plasma electrons in the presence of a magnetic field
• NEUTRINO–ELECTRON PROCESSES IN A STRONG MAGNETIC FIELD AND PLASMA
• Neutron matter under strong magnetic fields: A comparison of models
• The study of relatively low density stellar matter in presence of strong quantizing magnetic field
• Neutrino Transport in Strongly Magnetized Proto–Neutron Stars and the Origin of Pulsar Kicks: The Effect of Asymmetric Magnetic Field Topology