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• W2225509841 abstract "The iron $mathrm{K}ensuremath{alpha}$ line commonly observed in the x-ray spectrum of black hole candidates is produced by x-ray fluorescence of the inner accretion disk. This line can potentially be quite a powerful tool to probe the spacetime geometry around these objects and test the Kerr black hole hypothesis. In a previous paper, we studied the ability to constrain possible deviations from the Kerr solution from the standard time-integrated iron line spectrum within the Cardoso-Pani-Rico framework. In the present work, we expand on that study and consider iron line reverberation mapping in the Cardoso-Pani-Rico framework. That is, we consider the time evolution of the iron line profile in response to fluctuations in the x-ray primary source. Our simulations clearly show that the time information in reverberation mapping can better constrain the background metric than the time-integrated approach, and this is true, notably, for the deformation parameter ${ensuremath{epsilon}}_{3}^{r}$, which is only weakly informed by a time-integrated observation." @default.
• W2225509841 created "2016-06-24" @default.
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• W2225509841 date "2016-06-16" @default.
• W2225509841 modified "2023-10-16" @default.
• W2225509841 title "Testing the Kerr nature of black hole candidates using iron line reverberation mapping in the Cardoso-Pani-Rico framework" @default.
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• W2225509841 doi "https://doi.org/10.1103/physrevd.93.123008" @default.
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