是比赛 发表于 2025-3-27 00:02:10
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.PHONE 发表于 2025-3-27 02:10:07
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.heart-murmur 发表于 2025-3-27 06:51:34
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核心 发表于 2025-3-27 11:45:17
http://reply.papertrans.cn/19/1890/188949/188949_34.pngNATAL 发表于 2025-3-27 16:18:40
https://doi.org/10.1007/978-981-10-4524-0textbook black holes; Continuum-Fitting Method; Iron Line Method; Quasi-Periodic Oscillations; Kerr Para围裙 发表于 2025-3-27 18:45:17
978-981-13-5158-7Springer Nature Singapore Pte Ltd. 2017GULF 发表于 2025-3-28 00:54:03
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http://reply.papertrans.cn/19/1890/188949/188949_38.png庄严 发表于 2025-3-28 09:37:57
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产生 发表于 2025-3-28 10:37:34
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.