Nonlinear perturbations of transonic spherical accretion onto compact objects produce a dynamical effective acoustic geometry whose horizon shifts with the amplitudes of density, temperature, and mass-accretion-rate fluctuations.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
years
2026 2verdicts
UNVERDICTED 2representative citing papers
Acoustic horizons in spinning black-hole accretion with spatially varying adiabatic index have surface gravities that depend on the black-hole spin parameter.
citing papers explorer
-
Emergent gravity from nonlinear perturbation of spherical accretion with variable adiabatic index
Nonlinear perturbations of transonic spherical accretion onto compact objects produce a dynamical effective acoustic geometry whose horizon shifts with the amplitudes of density, temperature, and mass-accretion-rate fluctuations.
-
On the spin dependence of the emergent gravity phenomena as observed in axially symmetric black hole accretion with spatially varying adiabatic index
Acoustic horizons in spinning black-hole accretion with spatially varying adiabatic index have surface gravities that depend on the black-hole spin parameter.