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Titlebook: Black Holes: A Laboratory for Testing Strong Gravity; Cosimo Bambi Textbook 2017 Springer Nature Singapore Pte Ltd. 2017 textbook black ho

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31#
發(fā)表于 2025-3-27 00:02:10 | 只看該作者
Testing the Kerr Paradigm with X-Ray ObservationsThe chapter briefly reviews current attempts to test the Kerr metric around astrophysical black holes with the continuum-fitting method, X-ray reflection spectroscopy, and quasi-periodic oscilations.
32#
發(fā)表于 2025-3-27 02:10:07 | 只看該作者
Tests with Other ApproachesThe chapter briefly reviews current/future attempts to test the Kerr metric around astrophysical black holes with SgrA., precise measurements in the weak gravitational field of black holes, and with gravitational waves.
33#
發(fā)表于 2025-3-27 06:51:34 | 只看該作者
Cosimo BambiProvides the mathematical tools to compute some key-features in the X-ray spectrum of black holes.Contains calculations and analytical details in the appendix.Offers exercises and examples for student
34#
發(fā)表于 2025-3-27 11:45:17 | 只看該作者
35#
發(fā)表于 2025-3-27 16:18:40 | 只看該作者
https://doi.org/10.1007/978-981-10-4524-0textbook black holes; Continuum-Fitting Method; Iron Line Method; Quasi-Periodic Oscillations; Kerr Para
36#
發(fā)表于 2025-3-27 18:45:17 | 只看該作者
978-981-13-5158-7Springer Nature Singapore Pte Ltd. 2017
37#
發(fā)表于 2025-3-28 00:54:03 | 只看該作者
38#
發(fā)表于 2025-3-28 03:14:15 | 只看該作者
39#
發(fā)表于 2025-3-28 09:37:57 | 只看該作者
Thin Accretion Disksholes, pointing out its assumptions. It also describes the transfer function for thin accretion disks and how the transfer function can be calculated in a stationary and axisymmetric spacetime and in the Kerr metric in particular. Last, the chapter discusses possible deviations from the Kerr backgro
40#
發(fā)表于 2025-3-28 10:37:34 | 只看該作者
Imaging Black Holeslity of imaging astrophysical black holes is mainly motivated by the special situation of SgrA., because it is widely thought that sub-mm VLBI facilities will be soon able to image this black hole and detect its shadow.
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