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20162026
most citedTesting the Kerr black hole hypothesis using X-ray reflection spectroscopy

152 citations · 1.3k across the 50 of their papers we have counts for

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Showing 2020Show all

11 papers · 1 filter

astro-ph.HE2020★ 54 cited

Testing General Relativity with NuSTAR data of Galactic Black Holes

Ashutosh Tripathi, Yuexin Zhang, Askar B. Abdikamalov +5

Einstein's theory of General Relativity predicts that the spacetime metric around astrophysical black holes is described by the Kerr solution. In this work, we employ state-of-the-…

astro-ph.HE2020★ 152 cited

Towards precision measurements of accreting black holes using X-ray reflection spectroscopy

Cosimo Bambi, Laura W. Brenneman, Thomas Dauser +14

Relativistic reflection features are commonly observed in the X-ray spectra of accreting black holes. In the presence of high quality data and with the correct astrophysical model,…

astro-ph.HE2020★ 43 cited

Testing the Kerr Black Hole Hypothesis with GX 339-4 by a combined analysis of its thermal spectrum and reflection features

Ashutosh Tripathi, Askar B. Abdikamalov, Dimitry Ayzenberg +3

We analyze simultaneous observations with NuSTAR and Swift of the black hole binary GX 339-4 in which we clearly detect both a strong thermal component and prominent relativistic r…

astro-ph.HE2020★ 38 cited

A Possible -ray Quasi-periodic Oscillation of 314 days in the Blazar OJ 287

Pankaj Kushwaha, Arkadipta Sarkar, Alok C. Gupta +3

We report the detection of a probable -ray quasi-periodic oscillation (QPO) of around 314 days in the monthly binned 0.1 -- 300 GeV -ray {\it Fermi}-LAT light curve of the we…

astro-ph.HE2020★ 10 cited

Testing the Keplerian disk hypothesis using X-ray reflection spectroscopy

Ashutosh Tripathi, Biao Zhou, Askar B. Abdikamalov +3

The Novikov-Thorne model is the standard framework for the description of geometrically thin and optically thick accretion disks around black holes and is widely used to study the…

astro-ph.HE2020★ 17 cited

Impact of the reflection model on the estimate of the properties of accreting black holes

Ashutosh Tripathi, Honghui Liu, Cosimo Bambi

Relativistic reflection features in the X-ray spectra of black hole binaries and AGNs originate from illumination of the inner part of the accretion disk by a hot corona. In the pr…

astro-ph.HE2020★ 24 cited

Shining X-rays on asymptotically safe quantum gravity

Biao Zhou, Askar B. Abdikamalov, Dimitry Ayzenberg +3

Asymptotically safe quantum gravity is a promising candidate scenario to provide a UV extension for the effective quantum field theory of Einstein's gravity. The theory has its fou…

gr-qc2020★ 24 cited

X-ray reflection spectroscopy with Kaluza-Klein black holes

Jiachen Zhu, Askar B. Abdikamalov, Dimitry Ayzenberg +6

Kaluza-Klein theory is a popular alternative theory of gravity, with both non-rotating and rotating black hole solutions known. This allows for the possibility that the theory coul…

astro-ph.HE2020★ 10 cited

Thermal spectra of thin accretion disks of finite thickness around Kerr black holes

Menglei Zhou, Askar B. Abdikamalov, Dimitry Ayzenberg +3

The analysis of the thermal spectrum of geometrically thin and optically thick accretion disks of black holes, the so-called continuum-fitting method, is one of the leading techniq…

astro-ph.HE2020★ 61 cited

Testing the Kerr black hole hypothesis using X-ray reflection spectroscopy and a thin disk model with finite thickness

Askar B. Abdikamalov, Dimitry Ayzenberg, Cosimo Bambi +5

X-ray reflection spectroscopy is a powerful tool for probing the strong gravity region of black holes and can be used for testing general relativity in the strong field regime. Sim…

gr-qc2020★ 32 cited

Testing general relativity with the stellar-mass black hole in LMC X-1 using the continuum-fitting method

Ashutosh Tripathi, Menglei Zhou, Askar B. Abdikamalov +6

The iron line and the continuum-fitting methods are currently the two leading techniques for measuring black hole spins with electromagnetic radiation. They can be naturally extend…