Self-consistent spectra from GRMHD simulations with radiative cooling A link to reality for Sgr A*

Cosmos++ (Anninos et al., 2005) is one of the rst fully relativistic magneto-hydro-dynamical (MHD) codes that can self-consistently account for radiative cooling, in the optically thin regime. As the code combines a total energy conservation formulation with a radiative cooling function, we have now the possibility to produce spectra energy density from these simulations and compare them to data. In this paper, we present preliminary results of spectra calculated using the same cooling functions from 2D Cosmos++ simulations of the accretion ow around Sgr A*. The simulation parameters were designed to roughly reproduce Sgr A*'s behavior at very low ( 10^-8_-10^-7 M_⊙/yr) accretion rate, but only via spectra can we test that this has been achieved.