TL;DR
This paper investigates how black hole mass evolves during the universe's transition from matter dominance to dark energy dominance, highlighting a significant change in accretion rates.
Contribution
It provides a detailed analysis of black hole mass evolution in a standard cosmological model during a critical transition period.
Findings
Accretion rate of matter was about 10^{54} times higher than dark energy at transition.
Black hole mass evolution is significantly affected during the matter to dark energy transition.
The study offers insights into black hole growth in an accelerating universe.
Abstract
We have analyzed the evolution of mass of a stationary black hole in the standard FRW cosmological model. The evolution is determined specifically about the time of transition from the earlier matter to the later exotic dark energy dominated universe. It turns out that the accretion rate of matter on the black hole of mass was approximately higher than the accretion rate of exotic dark energy at the time of transition.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.