Magnetised Neutron Stars : An Overview
| dc.creator | Goyal, Ashok | |
| dc.date | 2003-06-13 | |
| dc.date.accessioned | 2026-07-07T03:49:49Z | |
| dc.date.available | 2026-07-07T03:49:49Z | |
| dc.description | In the presence of strong magnetic field reported to have been observed on the surface of some neutron stars and on what are called Magnetars, a host of physical phenomenon from the birth of a neutron star to free streaming neutrino cooling phase will be modified. In this review I will discuss the effect of magnetic field on the equation of state of high density nuclear matter by including the anomalous magnetic moment of the nucleons into consideration. I would then go over to discuss the neutrino interaction processes in strong as well as in weak magnetic fields. The neutrino processes are important in studying the propagation of neutrinos and in studying the energy loss, Their study is a prerequisite for the understanding of actual dynamics of supernova explosion and on the stabilization of radial pulsation modes through the effect on bulk viscosity. The anisotropy introduced in the neutrino emission and through the modification of the shape of the neutrino sphere may explain the observed pulsar kicks. | |
| dc.description | 20 pages (latex file) including 8 figures (style file included). Talk given at Workshop on High magnetic field ane neutron star at Havana April 2003 (to be published in the proceedings) | |
| dc.identifier | https://arxiv.org/abs/hep-ph/0306116 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/0306116 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/42555 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Magnetised Neutron Stars : An Overview | |
| dc.type | text |