Cooling of Neutron Stars

We introduce the theoretical basis for modeling the cooling evolution of compact stars starting from Boltzmann equations in curved space-time. We open a discussion on observational verification of different neutron star models by consistent statistics. Particular interest has the question of existe...

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Bibliographic Details
Main Author: Grigorian H.
Format: Article
Language:English
Published: EDP Sciences 2010-10-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20100703004