Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Analyzing Black Hole X-Rays with Simulations

Technical Report ·
DOI:https://doi.org/10.2172/1768430· OSTI ID:1768430
We generate synthetic X-ray spectra of black holes from large-scale 3D GRMHD simulations performed on HPC machines. Here are a sampling of model spectra, characterized by the parameters indicated in the diagram below. The dashed red lines show power law fits to the parts of the spectrum observed by the X-ray telescope NuSTAR. How well these model spectra compare to real data helps us to characterize the physical realism of the underlying simulation techniques.
Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE National Nuclear Security Administration (NNSA)
DOE Contract Number:
89233218CNA000001
OSTI ID:
1768430
Report Number(s):
LA-UR--21-21877
Country of Publication:
United States
Language:
English

Similar Records

Black Holes: Connecting Theory and Simulation to Observation [Slides]
Technical Report · Wed Feb 10 23:00:00 EST 2021 · OSTI ID:1765857

Inverse Compton Cooling in the Coronae of Simulated Black Hole Accretion Flows
Journal Article · Wed Nov 25 19:00:00 EST 2020 · The Astrophysical Journal (Online) · OSTI ID:1774453