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: email@example.com
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
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