An Algorithm for the Simulation of the Magnetized Neutron Star Cooling

An Algorithm for the Simulation of the Magnetized Neutron Star Cooling

A model and algorithm for the cooling of the magnetized neutron stars are presented. The cooling evolution described by a system of parabolic partial differential equations with non-linear coeffcients is solved using the Alternating Direction Implicit method. A difference scheme and the preliminary...

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Bibliographic Details
Main Authors: Grigorian H., Ayriyan A., Chubarian E., Piloyan A., Rafayelyan M.
Format: Article
Language:English
Published: EDP Sciences 2016-01-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/201610802025

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