Accelerating Kerr-Newman black holes in (anti-)de Sitter space-time

J. B. Griffiths; J. Podolsky

Accelerating Kerr-Newman black holes in (anti-)de Sitter space-time

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

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

arxiv gr-qc/0601130 v1 pith:EHIZTV6R submitted 2006-01-30 gr-qc

J. Podolsky , J. B. Griffiths This is my paper

classification gr-qc

keywords sitteracceleratingblackpresentedanti-anti-deasymptoticallycharged

verification ladder T0 review T1 audit T2 compute T3 formal

0 comments

read the original abstract

A class of exact solutions of the Einstein-Maxwell equations is presented which describes an accelerating and rotating charged black hole in an asymptotically de Sitter or anti-de Sitter universe. The metric is presented in a new and convenient form in which the meaning of the parameters is clearly identified, and from which the physical properties of the solution can readily be interpreted.

Discussion (0). Sign in to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

Optical Characteristics of the Kerr-Bertotti-Robinson Black Hole
gr-qc 2025-08 conditional novelty 6.0 of 10

For the Kerr-Bertotti-Robinson black hole, the magnetic field mainly enlarges the shadow and Einstein ring while rotation mainly distorts the shadow shape, and current M87* and Sgr A* data give only weak bounds on the field.

Pith tools