REVIEW 2 cited by
Regular scalar clouds around a Kerr-Newman black hole: subextremal and extremal scenarios
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
abstract
In this work we analyze the existence of electrically charged scalar clouds which are bound states of a complex-valued massive scalar field in the background of subextremal and extremal Kerr-Newman black holes (BH). In particular, we reanalyze neutral (uncharged) clouds in extremal Kerr BH's. For the extremal scenarios we have implemented a novel technique which allows us to obtain regular clouds at the BH horizon ${\cal H}^+$ which turn out to be connected ``continuously'' with the cloud solutions in the subextremal case even if some derivatives of the scalar field are unbounded at the horizon. In particular, for subextremal BH's we have established regularity conditions at ${\cal H}^+$, by demanding that the field and its radial derivatives are bounded there, but in the extremal scenarios we relax this last condition while demanding that some scalar invariants are well behaved at ${\cal H}^+$. Furthermore we have implemented an integral technique to understand and justify in a simple and heuristic way the existence of such cloud configurations in those BH backgrounds.
Forward citations
Cited by 2 Pith papers
-
Electroweak clouds supported by magnetically charged black holes: Analytic treatment along the existence-line
In the large-charge limit, the allowed masses of electroweak W-boson clouds on magnetically charged black holes follow a compact WKB formula that matches numerical results at n=100 to better than one percent.
-
A sufficient condition for the development of superradiant instabilities in charged black-hole spacetimes
For very massive fields, a charged black hole with horizon potential Φ_H greater than Q/M can support the stationary scalar cloud that triggers superradiant instability.
Discussion (0). Continue with ORCID to comment.