The power of imaging: Constraining the plasma properties of grmhd simulations using eht observations of Sgr A∗

Chi Kwan Chan, Dimitrios Psaltis, Feryal Ozel, Ramesh Narayan, Aleksander Sa¸dowski

Research output: Contribution to journalArticle

62 Citations (Scopus)

Abstract

Recent advances in general relativistic magnetohydrodynamic simulations have expanded and improved our understanding of the dynamics of black-hole accretion disks. However, current simulations do not capture the thermodynamics of electrons in the low density accreting plasma. This poses a significant challenge in predicting accretion flow images and spectra from first principles. Because of this, simplified emission models have often been used, with widely different configurations (e.g., disk- versus jet-dominated emission), and were able to account for the observed spectral properties of accreting black holes. Exploring the large parameter space introduced by such models, however, requires significant computational power that exceeds conventional computational facilities. In this paper, we use GRay, a fast graphics processing unit (GPU) based ray-tracing algorithm, on the GPU cluster El Gato, to compute images and spectra for a set of six general relativistic magnetohydrodynamic simulations with different magnetic field configurations and black-hole spins. We also employ two different parametric models for the plasma thermodynamics in each of the simulations. We show that, if only the spectral properties of Sgr A∗ are used, all 12 models tested here can fit the spectra equally well. However, when combined with the measurement of the image size of the emission using the Event Horizon Telescope, current observations rule out all models with strong funnel emission, because the funnels are typically very extended. Our study shows that images of accretion flows with horizon-scale resolution offer a powerful tool in understanding accretion flows around black holes and their thermodynamic properties.

Original languageEnglish (US)
Article number1
JournalAstrophysical Journal
Volume799
Issue number1
DOIs
StatePublished - Jan 20 2015

Fingerprint

plasma
accretion
funnels
magnetohydrodynamic simulation
simulation
magnetohydrodynamics
thermodynamics
magnetic field configurations
event horizon
thermodynamic property
ray tracing
accretion disks
plasma density
horizon
thermodynamic properties
telescopes
magnetic field
electron
configurations
electrons

Keywords

  • Accretion, accretion disks
  • Black hole physics
  • Galaxy: Center
  • Radiative transfer

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

The power of imaging : Constraining the plasma properties of grmhd simulations using eht observations of Sgr A∗. / Chan, Chi Kwan; Psaltis, Dimitrios; Ozel, Feryal; Narayan, Ramesh; Sa¸dowski, Aleksander.

In: Astrophysical Journal, Vol. 799, No. 1, 1, 20.01.2015.

Research output: Contribution to journalArticle

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