Testing the Kerr Black Hole Hypothesis with GX 339-4 by a combined analysis of its thermal spectrum and reflection features
arXiv:2010.13474 · doi:10.3847/1538-4357/abccbd
Abstract
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 reflection features. We employ NKBB and RELXILL_NK, which are the state of the art of, respectively, the thermal and reflection models to test the Kerr black hole hypothesis. We obtain unprecedented precise measurements of the Johannsen deformation parameter : (lamppost coronal geometry) and (broken power-law emissivity profile) at a 90% confidence level, where the Kerr metric corresponds to . We investigate the systematic uncertainties by fitting the data with different models.
10 pages, 5 figures. v2: refereed version
References in corpus (21)
- Constraining Black Hole Spin Via X-ray Spectroscopy
- Gravitational Test Beyond the First Post-Newtonian Order with the Shadow of the M87 Black Hole
- Thin accretion disks in stationary axisymmetric wormhole spacetimes
- A code to compute the emission of thin accretion disks in non-Kerr space-times and test the nature of black hole candidates
- A Grid of Relativistic, non-LTE Accretion Disk Models for Spectral Fitting of Black Hole Binaries
- Testing the space-time geometry around black hole candidates with the analysis of the broad K iron line
- Testing Hořava-Lifshitz gravity using thin accretion disk properties
- High Density Reflection Spectroscopy: II. the Density of the Inner Black Hole Accretion Disc in AGN
- Profiles of emission lines generated by rings orbiting braneworld Kerr black holes
- Possible observational windows for quantum effects from black holes
- High Density Reflection Spectroscopy I. A case study of GX~339-4
- Public Release of RELXILL_NK: A Relativistic Reflection Model for Testing Einstein's Gravity
- Self-Consistent Black Hole Accretion Spectral Models and the Forgotten Role of Coronal Comptonization of Reflection Emission
- Testing the Kerr black hole hypothesis using X-ray reflection spectroscopy and a thin disk model with finite thickness
- Returning radiation in strong gravity around black holes: Reverberation from the accretion disc
- Impact of the returning radiation on the analysis of the reflection spectra of black holes
- Testing general relativity with the stellar-mass black hole in LMC X-1 using the continuum-fitting method
- XSPEC model for testing the Kerr black hole hypothesis using the continuum-fitting method
- Testing the Kerr hypothesis using X-ray reflection spectroscopy with NuSTAR data of Cygnus X-1 in the soft state
- Modeling uncertainties in X-ray reflection spectroscopy measurements II: Impact of the radiation from the plunging region
- Gravitational effects on the high energy emission of accreting black holes
Cited by in corpus (37)
- Towards precision measurements of accreting black holes using X-ray reflection spectroscopy
- Astrophysical Wormholes
- Testing General Relativity with NuSTAR data of Galactic Black Holes
- Testing the Kerr black hole hypothesis with GRS 1716-249 by combining the continuum-fitting and the iron-line methods
- Implementation of a radial disk ionization profile in the RELXILL_NK model
- Constraints on Einstein-Maxwell dilaton-axion gravity from X-ray reflection spectroscopy
- Testing regular black holes with X-ray and GW data
- Reflection spectra of accretion disks illuminated by disk-like coronae
- Testing the Kerr black hole hypothesis with the continuum-fitting and the iron line methods: the case of GRS 1915+105
- Testing General Relativity with black hole X-ray data: a progress report
- Impact of the disk thickness on X-ray reflection spectroscopy measurements
- The spins of the Galactic black holes in MAXI J1535-571 and 4U 1630-472 from Insight-HXMT
- Constraining the Konoplya-Rezzolla-Zhidenko deformation parameters II: limits from stellar-mass black hole X-ray data
- A reflection model with a radial disk density profile
- Probing bumblebee gravity with black hole X-ray data
- Dynamics of null particles and shadow for general rotating black hole
- Constraining the KRZ deformation parameters I: limits from supermassive black hole X-ray data
- Exploring departures from Schwarzschild black hole in gravity
- Testing the Weak Equivalence Principle near black holes
- Distinct thermodynamic and dynamic effects produced by scale factors in conformally related Einstein-power-Yang-Mills black holes
- Testing Gravity with Black Hole X-Ray Data
- Non-Kerr Constraints using Binary Black Hole inspirals considering phase modifications up to 4 PN order
- Impact of the returning radiation in current tests of the Kerr black hole hypothesis using X-ray reflection spectroscopy
- Testing the -Kerr metric with black hole X-ray data
- The population of NuSTAR Black Hole X-ray Binaries
- X-Ray Tests of General Relativity with Black Holes
- The generalized holographic -function for regular AdS black holes
- Testing Regular Black Holes with X-ray data of GX 339-4
- Stellar-Mass Black Holes
- Quasi-normal modes of slowly-rotating Johannsen black holes
- Testing General Relativity with black hole X-ray data
- Possible Coronal Geometry in the Hard and Soft State of Black Hole X-ray Binaries from MONK Simulations
- Tests of General Relativity using black hole X-ray data
- About the ability of agnostic X-ray tests of the Kerr Hypothesis to discover new physics
- Constraining the Konoplya-Rezzolla-Zhidenko deformation parameters III: limits from stellar-mass black holes using gravitational-wave observations
- Improved Constraints on Non-Kerr Deviations from Binary Black Hole Inspirals Using GWTC-4 Data
- Testing General Relativity with Black Holes