Multi-transonic spherical-type flows around massive black holes: galactic potential induced standing isothermal shocks
DOI10.1088/1475-7516/2021/05/025zbMath1485.85017arXiv1905.08567OpenAlexW3162238026MaRDI QIDQ5028122
Partha S. Joarder, Shubhrangshu Ghosh, Sananda Raychaudhuri
Publication date: 8 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1905.08567
Black holes (83C57) Shock waves and blast waves in fluid mechanics (76L05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Classical and relativistic thermodynamics (80A10) Galactic and stellar structure (85A15) Orbital mechanics (70M20) Dark matter and dark energy (83C56)
Cites Work
- Pseudo-Newtonian and general relativistic barotropic tori in Schwarzschild–de Sitter spacetimes
- General relativistic radiative transfer in spherical flows
- Standing shocks in isothermal rotating winds and accretion
- Dark matter halos around isolated ellipticals
- COMPARISON OF GENERAL RELATIVISTIC AND PSEUDO-NEWTONIAN DESCRIPTION OF MAGELLANIC-CLOUDS MOTION IN THE FIELD OF MILKY WAY
This page was built for publication: Multi-transonic spherical-type flows around massive black holes: galactic potential induced standing isothermal shocks
