GRMHD simulations of low-angular-momentum accretion onto rapidly spinning black holes show quasi-steady standing shocks in the weakly magnetized SANE regime, with shock position shifting outward for higher spin.
Title resolution pending
1 Pith paper cite this work, alongside 47 external citations. Polarity classification is still indexing.
1
Pith paper citing it
47
external citations · OpenAlex
citation-role summary
background 1
citation-polarity summary
fields
astro-ph.HE 1years
2025 1verdicts
CONDITIONAL 1roles
background 1polarities
unclear 1representative citing papers
citing papers explorer
-
Low Angular Momentum Black Hole Accretion: First GRMHD Evidence of Standing Shocks
GRMHD simulations of low-angular-momentum accretion onto rapidly spinning black holes show quasi-steady standing shocks in the weakly magnetized SANE regime, with shock position shifting outward for higher spin.