Astrophysical black holes are thought to be Kerr solution of general relativity but there is not yet observational evidence to prove them. One can study the emission of electromagnetic waves around them to test their geometry of space time. In this review article, we consider the deviation from Kerr solution to test the strong gravity regime of General Relativity. We introduce and employ black hole shadow, X-ray reflection spectroscopy, iron line reverberation mapping, quasi-periodic oscillations, and continuum-fitting method to solve the degeneracy problem.
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Ghasemi Nodehi,M. (2023). Review of testing black hole candidates with electromagnetic radiation. Iranian Journal of Physics Research, 23(2), 379-389. doi: 10.47176/ijpr.23.2.11635
MLA
Ghasemi Nodehi,M. . "Review of testing black hole candidates with electromagnetic radiation", Iranian Journal of Physics Research, 23, 2, 2023, 379-389. doi: 10.47176/ijpr.23.2.11635
HARVARD
Ghasemi Nodehi M. (2023). 'Review of testing black hole candidates with electromagnetic radiation', Iranian Journal of Physics Research, 23(2), pp. 379-389. doi: 10.47176/ijpr.23.2.11635
CHICAGO
M. Ghasemi Nodehi, "Review of testing black hole candidates with electromagnetic radiation," Iranian Journal of Physics Research, 23 2 (2023): 379-389, doi: 10.47176/ijpr.23.2.11635
VANCOUVER
Ghasemi Nodehi M. Review of testing black hole candidates with electromagnetic radiation. Dear user; Recently we have changed our software to Sinaweb. If you had already registered with the old site, you may use the same USERNAME but you need to change your password. To do so at the first use, please choose, 2023; 23(2): 379-389. doi: 10.47176/ijpr.23.2.11635