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• W2073957345 abstract "The construction of a generic parametrization to describe the spacetime geometry around astrophysical black hole candidates is an important step to test the Kerr black hole hypothesis. In the last few years, the Johannsen-Psaltis metric has been the most common framework to study possible deviations from the Kerr solution with present and near-future observations. Recently, Cardoso, Pani, and Rico have proposed a more general parametrization. The aim of the present paper is to study this new metric in a specific context, namely, the thermal spectrum of geometrically thin and optically thick accretion disks. The most relevant finding is that the spacetime geometry around objects that look like very-fast-rotating Kerr black holes may still have large deviations from the Kerr solution. This is not the case with the Johannsen-Psaltis metric, which means the latter is missing an important class of non-Kerr spacetimes." @default.
• W2073957345 created "2016-06-24" @default.
• W2073957345 creator A5052113197 @default.
• W2073957345 date "2014-08-18" @default.
• W2073957345 modified "2023-09-26" @default.
• W2073957345 title "Note on the Cardoso-Pani-Rico parametrization to test the Kerr black hole hypothesis" @default.
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• W2073957345 doi "https://doi.org/10.1103/physrevd.90.047503" @default.
• W2073957345 hasPublicationYear "2014" @default.
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