Pith. sign in

REVIEW

Testing General Relativity with Black Hole X-Ray Data and ABHModels

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 2307.12755 v2 pith:RRAPZHEL submitted 2023-07-24 astro-ph.IM astro-ph.HEgr-qc

classification astro-ph.IMastro-ph.HEgr-qc
keywords blackdatageneralholesrelativityx-rayholeabhmodels
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
abstract

The past 10 years have seen tremendous progress in our capability of testing General Relativity in the strong field regime with black hole observations. 10 years ago, the theory of General Relativity was almost completely unexplored in the strong field regime. Today, we have gravitational wave data of the coalescence of stellar-mass black holes, radio images of the supermassive black holes SgrA$^*$ and M87$^*$, and high-quality X-ray data of stellar-mass black holes in X-ray binaries and supermassive black holes in active galactic nuclei. In this manuscript, we will review current efforts to test General Relativity with black hole X-ray data and we will provide a detailed description of the public codes available on ABHModels.

Discussion (0). Sign in to comment.

Pith tools