EPJ Web of Conferences
Volume 108, 2016Mathematical Modeling and Computational Physics (MMCP 2015)
|Number of page(s)||6|
|Published online||09 February 2016|
An Algorithm for the Simulation of the Magnetized Neutron Star Cooling
1 Joint Institute for Nuclear Research, Joliot-Curie 6, 141980 Dubna, Moscow Region, Russia
2 Yerevan State University, Alek Manyukyan 1, 0025 Yerevan, Republic of Armenia
3 Yerevan Physics Institute, A. Alikhanian Brothers 2, 0036 Yerevan, Republic of Armenia
4 University of Bordeaux, 351 Cours de la Libération, F-33400 Talence, France
a e-mail: firstname.lastname@example.org
Published online: 9 February 2016
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 results of simulations are presented.
© Owned by the authors, published by EDP Sciences, 2016
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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