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pro vyhledávání: '"Kinch, Brooks E."'
Data derived from general relativistic MHD simulations of accretion onto black holes can be used as input to a post-processing scheme that predicts the radiated spectrum. Combining a relativistic Compton-scattering radiation transfer solution in the
Externí odkaz:
http://arxiv.org/abs/2412.01984
Autor:
Kinch, Brooks E., Schnittman, Jeremy D., Noble, Scott C., Kallman, Timothy R., Krolik, Julian H.
We present a survey of how the spectral features of black hole X-ray binary systems depend on spin, accretion rate, viewing angle, and Fe abundance when predicted on the basis of first principles physical calculations. The power law component hardens
Externí odkaz:
http://arxiv.org/abs/2105.09408
We present a formulation for a local cooling function to be employed in the diffuse, hot corona region of 3D GRMHD simulations of accreting black holes. This new cooling function calculates the cooling rate due to inverse Compton scattering by consid
Externí odkaz:
http://arxiv.org/abs/2009.01914
We describe results from a new technique for the prediction of complete, self-consistent X-ray spectra from three-dimensional General Relativistic magnetohydrodynamic (GRMHD) simulations of black hole accretion flows. Density and cooling rate data fr
Externí odkaz:
http://arxiv.org/abs/1810.13099
We present first results from a new technique for the prediction of Fe K$\alpha$ profiles directly from general relativistic magnetohydrodynamic (GRMHD) simulations. Data from a GRMHD simulation are processed by a Monte Carlo global radiation transpo
Externí odkaz:
http://arxiv.org/abs/1604.01126
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