On the angular momentum of the neutron star
Astrophysics
2007-05-23 v1
Abstract
It is shown that the mass loss due to rotation-driven hydrodynamical instability during the catastrophic collapse of the star is small. Neutron star is formed with a large rotational kinetic energy and the spin-down takes place in the following life of neutron star as a pulsar.
Keywords
Cite
@article{arxiv.astro-ph/0310573,
title = {On the angular momentum of the neutron star},
author = {Zakir F. Seidov},
journal= {arXiv preprint arXiv:astro-ph/0310573},
year = {2007}
}
Comments
3 pages