Neutron Stars Properties and Crust Movements in Post-glitch Epoch

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dc.creatorGonzález-Romero, L. M.
dc.creatorNavarro-Lérida, F.
dc.date2009-02-07
dc.date.accessioned2026-07-07T12:39:19Z
dc.date.available2026-07-07T12:39:19Z
dc.descriptionUsing 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.
dc.descriptionLatex, 4 pages, 3 eps figures
dc.identifierhttps://arxiv.org/abs/0902.1238
dc.identifierhttp://arxiv.org/abs/0902.1238
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/219068
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleNeutron Stars Properties and Crust Movements in Post-glitch Epoch
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