paper

Testing conformal gravity with the supermassive black hole in 1H0707-495

arXiv:1803.07849 · doi:10.1103/PhysRevD.98.024007

Abstract

Recently, two of us have found a family of singularity-free rotating black hole solutions in Einstein's conformal gravity. These spacetimes are characterized by three parameters: the black hole mass , the black hole spin angular momentum , and a parameter that is not specified by the theory but can be expected to be proportional to the black hole mass . The Kerr black hole solution of Einstein's gravity is recovered for . In a previous paper, we showed that X-ray data of astrophysical black holes require . In the present paper, we report the results of a more sophisticated analysis. We apply the X-ray reflection model {\sc relxill\_nk} to \textsl{NuSTAR} and \textsl{Swift} data of the supermassive black hole in 1H0707-495. We find the constraint (90% confidence level).

6 pages, 2 figures. v2: refereed version

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