REVIEW 2 cited by
Description of Pseudo-Newtonian Potential for the Relativistic Accretion Disk around Kerr Black Holes
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Signed reviews
read the original abstract
We present a pseudo-Newtonian potential for accretion disk modeling around the rotating black holes. This potential can describe the general relativistic effects on accretion disk. As the inclusion of rotation in a proper way is very important at an inner edge of disk the potential is derived from the Kerr metric. This potential can reproduce all the essential properties of general relativity within 10% error even for rapidly rotating black holes.
Forward citations
Cited by 2 Pith papers
-
Simulation based parameter space for shock in transonic, sub-Keplerian accretion flow onto non-rotating black holes
Multi-dimensional simulations show that the parameter space for shocks in non-dissipative transonic sub-Keplerian accretion flows is substantially larger than the analytic prediction, with dynamic boundary layers prod...
-
Threshold Drop in Accretion Density if Dark Energy is Accreting onto a Supermassive Black Hole
Viscous, rotating accretion of modified Chaplygin gas dark energy onto a supermassive black hole produces a threshold drop in accretion density and a stronger wind.
Discussion (0). Continue with ORCID to comment.