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M. Chandra

3 papers hereh-index 14925 citations37 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author1
  • middle author2

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.IM1

identity via Semantic Scholar / OpenAlex

most citedHow important is non-ideal physics in simulations of sub-Eddington accretion onto spinning black holes?

60 citations · 88 across the 2 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2017★ 60 cited

How important is non-ideal physics in simulations of sub-Eddington accretion onto spinning black holes?

Francois Foucart, Mani Chandra, Charles F. Gammie +2

Black holes with accretion rates well below the Eddington rate are expected to be surrounded by low-density, hot, geometrically thick accretion disks. This includes the two black h…

astro-ph.IM2017★ 28 cited

grim: A Flexible, Conservative Scheme for Relativistic Fluid Theories

Mani Chandra, Francois Foucart, Charles F. Gammie

Hot, diffuse, relativistic plasmas such as sub-Eddington black hole accretion flows are expected to be collisionless, yet are commonly modeled as a fluid using ideal general relati…

astro-ph.HE2016

Polarized Synchrotron Emissivities and Absorptivities for Relativistic Thermal, Power-Law, and Kappa Distribution Functions

Alex Pandya, Zhaowei Zhang, Mani Chandra +1

Synchrotron emission and absorption determine the observational appearance of many astronomical systems. In this paper, we describe a numerical scheme for calculating synchrotron e…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.