Neutron Stars Properties and Crust Movements in Post-glitch Epoch
arXiv:0902.1238
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.
Latex, 4 pages, 3 eps figures