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Testing regular black holes with X-ray data of GX 339–4

Shafqat RiazCenter for Astronomy and Astrophysics, Center for Field Theory and Particle Physics, and Department of Physics, Fudan University, 2005 Songhu Road, Shanghai 200438, ChinaMichail KyriazisTheoretical Astrophysics, Eberhard-Karls Universität Tübingen, Auf der Morgenstelle 10, D-72076 Tübingen, GermanyAskar B. AbdikamalovCenter for Astronomy and Astrophysics, Center for Field Theory and Particle Physics, and Department of Physics, Fudan University, 2005 Songhu Road, Shanghai 200438, ChinaCosimo BambiCenter for Astronomy and Astrophysics, Center for Field Theory and Particle Physics, and Department of Physics, Fudan University, 2005 Songhu Road, Shanghai 200438, ChinaSwarnim ShashankCenter for Astronomy and Astrophysics, Center for Field Theory and Particle Physics, and Department of Physics, Fudan University, 2005 Songhu Road, Shanghai 200438, China
ABI

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Abstract Regular black holes are singularity-free black hole spacetimes proposed to solve the problem of the presence of spacetime singularities that plagues the black holes of general relativity and most theories of gravity. In this work, we consider the regular black holes recently proposed by Mazza, Franzin & Liberati and we extend previous studies to get a more stringent observational constraint on the regularization parameter l . We study simultaneous observations of NuSTAR and Swift of the Galactic black hole in GX 339–4 during its outburst in 2015. The quality of the NuSTAR data is exceptionally good and the spectrum of the source presents both a strong thermal component and prominent relativistically blurred reflection features. This permits us to measure the regularization parameter l from the simultaneous analysis of the thermal spectrum and the reflection features. From our analysis, we find the constraint l/M < 0.44 (90% CL), which is stronger than previous constraints inferred with X-ray and gravitational wave data.

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