Radiative GRMHD simulations of accretion disks
W{\l}odek Klu\'zniak, David Abarca, and Bhupendra Mishra
TL;DR
This paper presents recent results from general relativistic magnetohydrodynamic simulations of accretion disks around black holes and neutron stars, incorporating radiation effects to better understand their evolution.
Contribution
It introduces advanced GRRMHD simulation techniques to study accretion disk dynamics with radiation, enhancing previous models by including radiative processes.
Findings
Insights into accretion disk behavior around compact objects
Improved modeling of radiative effects in GRMHD simulations
Enhanced understanding of black hole and neutron star environments
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).
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