MC Simulations of the Broadband Spectra of Sagittarius A* through the use of GRMHD

Abstract

We present results of simulations of the spectrum of the accretion flow onto the supermassive black hole in our Galactic Centre, Sagittarius A*, generated with a coupling of Monte-Carlo (MC) radiation and general relativistic magnetohydrodynamic (GRMHD) codes. In our modeling, we use the 2D HARM GRMHD code to first model the physical parameters of the disk, then feed its results into our 2D MC photon transport code. We will discuss results obtained which fit radio, IR, and Chandra-obtained flaring or quiescent x-ray data points, as well as the validity of the amount of scaling of input parameters (density, temperature, and magnetic field) required to fit these points. HARM output will be used to suggest whether the scaling is within reasonable limits.

8 pages with 11 figures

References in corpus (2)

• Evidence for X-ray synchrotron emission from simultaneous mid-IR to X-ray observations of a strong Sgr A* flare
• A Testable the Stochastic Acceleration Model for Flares in Sagittarius A*

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• Spectral and Imaging properties of Sgr A* from High-Resolution 3D GRMHD Simulations with Radiative Cooling
• Modelling the black hole silhouette in Sgr A* with ion tori
• Near-infrared polarimetry as a tool for testing properties of accreting super-massive black holes
• Nonthermal processes in hot accretion flows onto supermassive black holes: An inhomogeneous model
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• Numerical Modeling of Multi-wavelength Spectra of M87 Core Emission
• The Jet in the Galactic Center: An Ideal Laboratory for Magnetohydrodynamics and General Relativity
• Constraining the Accretion Flow in Sgr A* by General Relativistic Dynamical and Polarized Radiative Modeling
• General Relativistic Magnetohydrodynamic and Monte Carlo Modeling of Sagittarius A*