ar X iv : a st ro - p h / 99 03 18 6 v 1 1 1 M ar 1 99 9 Preprint USM - TH - 73 Neutrino Scattering Off Spin - Polarized Particles in Supernovae
نویسندگان
چکیده
We calculate neutrino and anti-neutrino scattering off electrons and nucleons in supernovae using a detailed Monte Carlo transport code incorporating realistic equations of state. The goal is to determine whether particles in a neutron star core, partially spin-aligned by the local magnetic field, can give rise to asymmetric neutrino emission via the standard parity breaking weak force. We conclude that electron scattering in a very high magnetic field does indeed give a net asymmetry, but that nucleon scattering, if present, removes the asymmetry.
منابع مشابه
ar X iv : a st ro - p h / 98 07 18 3 v 1 1 7 Ju l 1 99 8 Neutrino spin - flips in curved space - time
The general relativistic effects on spin-flavor oscillations above the core of type II supernovae are investigated. The evolution equation is derived and the relative magnitudes of the terms in the Hamiltonian, which arise from the weak, electromagnetic and gravitational interaction, are compared. The effects on the resonance position and the adiabaticity are studied. Explicit calculations are ...
متن کاملar X iv : a st ro - p h / 96 08 03 6 v 1 8 A ug 1 99 6 TABLE 1 Properties of LMC Double - Mode
متن کامل
ar X iv : a st ro - p h / 99 03 26 4 v 1 1 7 M ar 1 99 9 The Progenitors of Type
Models for Type Ia Supernovae (SNe Ia) are reviewed. It is shown that there are strong reasons to believe that SNe Ia represent thermonuclear disruptions of C–O white dwarfs, when these white dwarfs reach the Chandrasekhar limit and ignite carbon at their centers. Progenitor scenarios are reviewed critically and the strengths and weaknesses of each scenario are explicitly presented. It is argue...
متن کاملar X iv : a st ro - p h / 99 04 21 3 v 1 1 6 A pr 1 99 9 High Energy Cosmic Neutrinos Astronomy : The ANTARES Project ‡
Neutrinos may offer a unique opportunity to explore the far Universe at high energy. The ANTARES collaboration aims at building a large undersea neutrino detector able to observe astrophysical sources (AGNs, X-ray binary systems, ...) and to study particle physics topics (neutrino oscillation, ...). After a description of the research opportunities of such a detector, a status report of the exp...
متن کامل