Radiative GRMHD simulations of accretion disks
arXiv:1712.07014 · doi:10.1002/asna.201713419
Abstract
We describe some recent results on the evolution of accretion disks around black holes and neutron stars obtained in magnetohydrodynamic (MHD) simulations in general relativity (GR) with the inclusion of radiation (GRRMHD).
arXiv comment6 pages, 4 figures, Proceeding for SMFNS2017 5th International Symposium on Strong Electromagnetic Fields and Neutron Stars, 10-13 May, 2017 Varadero, Cuba
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