New FNST scalar-tensor generalization of JNW spacetime is used in GR hydrodynamic simulations of BHL accretion, yielding hydrodynamically generated QPO-like frequencies overlapping observed ranges in stellar-mass compact object systems.
D¨ onmez, 2024, 006 (2024)
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
verdicts
UNVERDICTED 3representative citing papers
Numerical BHL accretion simulations in disformal Kerr spacetime produce QPO frequencies consistent with observations from GRS 1915+105, M82 X-1, NGC 5408 X-1, and RE J1034+396.
QPO frequencies in RN AdS and Kerr geometries trace distinct thermodynamic phases and their stability when plotted against Hawking temperature.
citing papers explorer
-
QPO-like Signatures and Hydrodynamical Variability in Accretion around a JNW-type Compact Spacetime in Freund-Nambu Scalar-Tensor Gravity
New FNST scalar-tensor generalization of JNW spacetime is used in GR hydrodynamic simulations of BHL accretion, yielding hydrodynamically generated QPO-like frequencies overlapping observed ranges in stellar-mass compact object systems.
-
Disformal Kerr Imprints on BHL Accretion: Shock Morphology, PSD Signatures, and Observational QPO Counterparts
Numerical BHL accretion simulations in disformal Kerr spacetime produce QPO frequencies consistent with observations from GRS 1915+105, M82 X-1, NGC 5408 X-1, and RE J1034+396.
-
Probing Black Hole Phase Transitions through Quasi-Periodic Oscillations
QPO frequencies in RN AdS and Kerr geometries trace distinct thermodynamic phases and their stability when plotted against Hawking temperature.