Can I read Core-crust transition pressure evolution in post-glitch epoch for a Vela-type pulsar on EtoBox?

Core-crust transition pressure evolution in post-glitch epoch for a Vela-type pulsar by González-Romero, L. M.; Blázquez-Salcedo, J. L. is a scholarly article available to read on EtoBox.

What is Core-crust transition pressure evolution in post-glitch epoch for a Vela-type pulsar about?

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,...).

Author

González-Romero, L. M.; Blázquez-Salcedo, J. L.

Published

2009

Language

EN