An Algorithm for the Simulations of the Magnetized Neutron Star Cooling

Published 17 Nov 2015 in physics.comp-ph | (1511.05380v1)

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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