Magnetic Fields of Neutron Stars
arXiv:1709.07106 · doi:10.1007/s12036-017-9467-4
Abstract
This article briefly reviews our current understanding of the evolution of magnetic fields in neutron stars, which basically defines the evolutionary pathways between different observational classes of neutron stars. The emphasis here is on the evolution in binary systems and the newly emergent classes of millisecond pulsars.
Has appeared in Journal of Astrophysics and Astronomy special issue on 'Physics of Neutron Stars and Related Objects', celebrating the 75th birth-year of G. Srinivasan
References in corpus (15)
- A Radio Pulsar/X-ray Binary Link
- The Magnificent Seven: Magnetic fields and surface temperature distributions
- Discovery of coherent millisecond X-ray pulsations in Aql X-1
- Discovery of PSR J1227-4853: A transition from a low-mass X-ray binary to a redback millisecond pulsar
- CCOs and the hidden magnetic field scenario
- Population synthesis of radio and gamma-ray millisecond pulsars from the Galactic disk
- Burial of the polar magnetic field of an accreting neutron star. II. Hydromagnetic stability of axisymmetric equilibria
- The relevance of ambipolar diffusion for neutron star evolution
- XMM-Newton Observations of Radio Pulsars B0834+06 and B0826-34 and Implications for Pulsar Inner Accelerator
- Hall drift of axisymmetric magnetic fields in solid neutron-star matter
- MHD instabilities in accretion mounds - 1: 2D axisymmetric simulations
- Neutron Star Physics in the Square Kilometer Array Era : An Indian Perspective
- Magnetic field evolution in neutron stars
- Joule heating in high magnetic field pulsars
- Members of the double pulsar system PSR J0737-3039 : neutron stars or strange stars ?