Dependence of acoustic surface gravity on geometric configuration of matter for axially symmetric background flows in the Schwarzschild metric
From MaRDI portal
Publication:2793150
DOI10.1142/S0218271815500960zbMath1332.83070arXiv1305.7134OpenAlexW2963245784MaRDI QIDQ2793150
Publication date: 15 March 2016
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1305.7134
Black holes (83C57) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Quantum hydrodynamics and relativistic hydrodynamics (76Y05) Exact solutions to problems in general relativity and gravitational theory (83C15)
Related Items (3)
Relativistic sonic geometry for isothermal accretion in the Schwarzschild metric ⋮ Multi-criticality and related bifurcation in accretion discs around non-rotating black holes: an analytical study ⋮ Relativistic sonic geometry for isothermal accretion in the Kerr metric
Cites Work
This page was built for publication: Dependence of acoustic surface gravity on geometric configuration of matter for axially symmetric background flows in the Schwarzschild metric