GRRMHD simulations of 32 super-Eddington magnetically arrested disks show black hole spin boosts energy output super-linearly while mass has no effect over 5–30 solar masses.
Title resolution pending
1 Pith paper cite this work, alongside 52 external citations. Polarity classification is still indexing.
1
Pith paper citing it
52
external citations · OpenAlex
fields
astro-ph.HE 1years
2026 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
Strongly Magnetized Super-Eddington Accretion: How Spin and Accretion Rate Regulate Energy Output and Mass Loss
GRRMHD simulations of 32 super-Eddington magnetically arrested disks show black hole spin boosts energy output super-linearly while mass has no effect over 5–30 solar masses.