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arXiv · 0912.0628

Core-crust transition pressure evolution in post-glitch epoch for a Vela-type pulsar

L. M. González-Romero·J. L. Blázquez-Salcedo
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Abstract

We propose that the \textit{post-glitch} epoch in a Vela-type pulsar corresponds to a transition time in which the broken \textit{crust} is readjusting its temperature and core-\textit{crust} transition pressure after the changes produced by the \textit{glitch}. To describe the evolution of the pulsar in this epoch we use a sequence of stationary and axisymmetric relativistic models of slowly rotating neutron stars with a surface layer \textit{crust}. Previously, we have formulated the matching conditions on the surface of the star in terms of physical properties (total mass of the star, core-\textit{crust} transition pressure,...).

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L. M. González-Romero, J. L. Blázquez-Salcedo. 2009-12-03. Core-crust transition pressure evolution in post-glitch epoch for a Vela-type pulsar. https://arxiv.org/abs/0912.0628

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