Neutrino Interactions in Octet Baryon Matter

Abstract

Neutrino processes caused by the neutral current are studied in octet baryon matter. Previous confusion about the baryonic matrix elements of the neutral current interaction is excluded, and a correct table for them improved by consideration of the proton spin problem is presented instead.

6 pages

References in corpus (2)

• Neutrino Propagation in Dense Astrophysical Systems
• Neutrino emission due to Cooper pairing of nucleons in cooling neutron stars

Cited by in corpus (6)

• Hadron-quark mixed phase in hyperon stars
• The physics of dense hadronic matter and compact stars
• Baryon superfluidity and neutrino emissivity of neutron stars
• Hadron-quark mixed phase in neutron stars
• Constraining quark-hadron interface tension in the multi-messenger era
• Interface effects of strange quark matter