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An Algorithm for the Simulations of the Magnetized Neutron Star Cooling

Authors
Type
Published Article
Publication Date
Submission Date
Identifiers
DOI: 10.1051/epjconf/201610802025
Source
arXiv
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Abstract

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

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