Neutron Stars Properties and Crust Movements in Post-glitch Epoch

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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

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General Relativity and Quantum Cosmology

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http://salesiana.dossiersoluciones.com/handle/123456789/219068

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/0902.1238
 http://arxiv.org/abs/0902.1238

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arXiv