An Algorithm for the Simulations of the Magnetized Neutron Star Cooling
Computational Physics
2016-03-07 v1
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.
Keywords
Cite
@article{arxiv.1511.05380,
title = {An Algorithm for the Simulations of the Magnetized Neutron Star Cooling},
author = {H. Grigorian and A. Ayriyan and E. Chubarian and A. Piloyan and M. Rafayelyan},
journal= {arXiv preprint arXiv:1511.05380},
year = {2016}
}
Comments
6 pages, 4 figures, accepted to the European Physical Journal Web of Conferences as a contribution of the International Conference Mathematical Modeling and Computational Physics 2015 (High Tatra Mountains, Slovakia, July 13 - July 17, 2015, http://web.tuke.sk/mmcp/mmcp2015/)