REVIEW 2 cited by
Thin accretion disk images of the black hole in symmergent gravity
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
read the original abstract
In this paper, we study circular orbits, effective potential, and thin-accretion disk of a black hole in symmergent gravity within the Novikov-Thorne model in a way including the energy flux and temperature distribution. We determine bounds on symmergent gravity parameters and conclude that the accretion disk could be used as an astrophysical tool to probe symmergent gravity.
Forward citations
Cited by 2 Pith papers
-
Spinning Particle Dynamics and Observational Redshift around an Asymptotically Flat Symmergent Black Hole
For a black hole in symmergent gravity, the sign of the boson-fermion imbalance determines whether particle and photon observables deviate from Schwarzschild smoothly (fermion-dominated) or in an oscillatory pattern (...
-
Observable thin accretion disk around a self-dual black hole in loop quantum gravity
A self-dual loop quantum black hole is shown to look smaller and brighter than Schwarzschild in thin disk models, with the polymer parameter P bounded by Mercury and S2 star data.
Discussion (0). Continue with ORCID to comment.