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 (boson-dominated).
Thin accretion disk images of the black hole in symmergent gravity
1 Pith paper cite this work. Polarity classification is still indexing.
1
Pith paper citing it
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.
citation-role summary
background 1
citation-polarity summary
fields
gr-qc 1years
2026 1verdicts
CONDITIONAL 1roles
background 1polarities
background 1representative citing papers
citing papers explorer
-
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 (boson-dominated).