Published June 1, 2021
| Version v1
Journal article
Testing General Relativity with NuSTAR Data of Galactic Black Holes
Creators
- 1. Center for Field Theory and Particle Physics and Department of Physics, Fudan University, 200438 Shanghai (China)
- 2. Kapteyn Astronomical Institute, University of Groningen, 9747 AD Groningen (Netherlands)
- 3. Theoretical Astrophysics, Eberhard-Karls Universität Tübingen, D-72076 Tübingen (Germany)
- 4. Department of Astronomy, Tsinghua University, 100084 Beijing (China)
- 5. Institut für Astronomie und Astrophysik, Eberhard-Karls Universität Tübingen, D-72076 Tübingen (Germany)
Description
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-art relativistic reflection modeling to analyze a selected set of NuSTAR spectra of Galactic black holes to obtain the most robust and precise constraints on the Kerr black hole hypothesis possible today. Our constraints are much more stringent than those from other electromagnetic techniques and, with some sources, we find stronger constraints than those currently available from gravitational waves.
Availability note (English)
Available from http://dx.doi.org/10.3847/1538-4357/abf6cdAdditional details
Identifiers
Publishing Information
- Journal Title
- Astrophysical Journal
- Journal Volume
- 913
- Journal Issue
- 2
- Journal Page Range
- [14 p.]
- ISSN
- 0004-637X
- CODEN
- ASJOAB
INIS
- Country of Publication
- United Kingdom
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 53073474
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ASTROPHYSICS; BLACK HOLES; GENERAL RELATIVITY THEORY; GRAVITATIONAL WAVES
- Descriptors DEC
- FIELD THEORIES; PHYSICS; RELATIVITY THEORY