Pith. sign in

REVIEW

Gravitational Waves, Gamma Ray Bursts, and Black Stars

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

arxiv 1611.03853 v1 pith:Z547O7DB submitted 2016-11-11 gr-qc astro-ph.COhep-th

classification gr-qcastro-ph.COhep-th
keywords blackstarsgammagravitationalduringfollowedwavesappear
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Stars that are collapsing toward forming a black hole but appear frozen near their Schwarzschild horizon are termed "black stars". The collision of two black stars leads to gravitational radiation during the merging phase followed by a delayed gamma ray burst during coalescence. The recent observation of gravitational waves by LIGO, followed by a possible gamma ray counterpart by Fermi, suggests that the source may have been a merger of two black stars with profound implications for quantum gravity and the nature of black holes.

Discussion (0). Sign in to comment.

Pith tools