REVIEW 1 cited by
Most general Type-D Black Hole and the Accelerating Reissner-Nordstrom-NUT-(A)dS solution
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
read the original abstract
The Plebanski-Demianski metric is commonly thought to describe the most general Type D black hole in general relativity (possibly coupled with Maxwell electromagnetism), but in the form we know at the moment, it fails to include the elusive accelerating spacetimes with gravitomagnetic mass without angular momentum. We propose a very general type D metric, stemming from a binary black hole system, which represents a novel branch of the type D spacetimes: accelerating Kerr-Newman-NUT black hole with cosmological constant. It has straightforward limits to all the known type D black holes in the Einstein-Maxwell theory and in particular to the accelerating Reissner-Nordstrom-NUT solution, yet unknown in the literature.
Forward citations
Cited by 1 Pith paper
-
Accelerating charged and rotating black holes in scalar multipolar universes
The authors construct a claimed family of exact Einstein-Maxwell-scalar solutions describing accelerating charged rotating NUT black holes in scalar multipolar universes.
Discussion (0). Continue with ORCID to comment.