Tushar Mondal

Dynamo and Jet Interconnections in GRMHD Simulations of Black Hole Accretion Disks

Abstract We present 3D general relativistic magnetohydrodynamic (GRMHD) simulations of black hole (BH) accretion disks that investigate how a magnetorotational instability (MRI)-driven dynamo regulates jet formation and evolution. Unlike typical standard and normal evolution (SAN...