Magnetic Fields of Neutron Stars
arXiv:astro-ph/9911239
Abstract
The evolution of the magnetic field is investigated for isolated as well as binary neutron stars. The overall nature of the field evolution is seen to be similar for an initial crustal field and an expelled flux. The major uncertainties of the present models of field evolution and the directions in which further investigation are required are also discussed in detail.
6 pages, uses crckapb.sty and suprtab.sty, to be published in the proceedings of NATO/ASI on 'The Neutron Star - Black Hole Connection, held in Creete, Greece, 1999
References in corpus (6)
- The rp Process Ashes from Stable Nuclear Burning on an Accreting Neutron Star
- Nuclear heating and melted layers in the inner crust of an accreting neutron star
- Almost Analytic Models of Ultramagnetized Neutron Star Envelopes
- Magnetic Field Evolution of Accreting Neutron Stars - II
- Magnetic Field Evolution of Accreting Neutron Stars - III
- Evolution of Multipolar Magnetic Field in Isolated Neutron Stars