Model-Dependent Galactic Environment Effects on Multi-Transonic Accretion and Emergent Acoustic Gravity around Kerr Black Holes
astro-ph.HE, astro-ph.GA
Submitted: 2025-09-23
Updated: 2026-09-10
Comments: Accepted for publication in ApJ
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Hot Gas In and Around Elliptical Galaxies
- Powerful AGN jets and unbalanced cooling in the hot atmosphere of IC 4296
- Low radiative efficiency accretion in the nuclei of elliptical galaxies
- Isothermal Shock Formation in Non-Equatorial Accretion Flows around Kerr Black Holes
- General Relativistic Hydrodynamic Simulations and Linear Analysis of the Standing Accretion Shock Instability around a Black Hole
- The Standing Accretion Shock Instability in the Disk around the Kerr Black Hole
- Spectral properties of NGC 4151 and the Estimation of black hole mass using TCAF solution
- Shocks in relativistic viscous accretion flows around Kerr black holes
- Changing Accretion Geometry of Seyfert 1 Mrk 335 with {\it NuSTAR}: A Comparative Study
- Variable mass accretion and failed wind explain changing look phenomena in NGC 1365
- Study of accretion flows around an ultraluminous X-ray source M82 X-1 using NuSTAR data
- On the origin of core radio emissions from black hole sources in the realm of relativistic shocked accretion flow
- Ideal E/IMRI vs Real E/IMRI system : Observable signature in LISA
- Influence of flow thickness on general relativistic low angular momentum accretion around spinning black holes
- Effect of matter geometry on low angular momentum black hole accretion in the Kerr metric
- Model dependence of the multi-transonic behavior, stability properties and corresponding acoustic geometry for accretion onto a spinning black hole
- Black Hole spin dependence of general relativistic multi-transonic accretion close to the horizon
- Influence of the black hole spin on the chaotic particle dynamics within a dipolar halo
- The Cooling Flow to Accretion Flow Transition
- Dark matter in elliptical galaxies: II. Estimating the mass within the virial radius
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