Neutron Stars Properties and Crust Movements in Post-glitch Epoch
General Relativity and Quantum Cosmology
2009-02-10 v1
Abstract
Using a new numerical code with non-uniform adapted mesh, we study the changes produced in the global properties of neutron stars by the motion of matter in crust region during post-glitch epoch. Our numerical analysis shows that these changes may contribute to explain the observed spin-down of rotational frequency.
Cite
@article{arxiv.0902.1238,
title = {Neutron Stars Properties and Crust Movements in Post-glitch Epoch},
author = {L. M. González-Romero and F. Navarro-Lérida},
journal= {arXiv preprint arXiv:0902.1238},
year = {2009}
}
Comments
Latex, 4 pages, 3 eps figures