REVIEW 2 cited by
Kerr-Newman-NUT-Kiselev black holes in Rastall theory of gravity and Kerr/CFT Correspondence
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 new twisted rotating black hole solution by performing Demia{\'n}ski-Newman-Janis algorithm to the electrically and dyonically charged black hole with quintessence in Rastall theory of gravity. Using our black hole solution, we argue that Rastall gravity is not equivalent with Einstein gravity. For further explanation, the black hole properties such as the horizon and ergosphere are studied for which there are some different properties for those theories. Some thermodynamic properties of the black hole solution are also discussed. At the end, considering the Kerr/CFT correspondence is valid for our black hole solution, the central charge from the CFT of this extremal solution is derived.
Forward citations
Cited by 2 Pith papers
-
Impact of Rastall gravity on hydrostatic mass of galaxy clusters
Rastall gravity modifies hydrostatic mass estimates of galaxy clusters to produce near-unity slopes when compared to baryonic mass (no dark matter) or lensing mass (with dark matter).
-
Dynamics of Charged and Rotating NUT Black Holes in Rastall Gravity
A rotating, charged black hole with NUT charge in Rastall gravity is constructed and shown to have NUT-dependent horizons, temperatures, and stable orbit radii.
Discussion (0). Continue with ORCID to comment.