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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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21#
發(fā)表于 2025-3-25 05:40:21 | 只看該作者
Erforderliche ZeichenmaterialienThe 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.
22#
發(fā)表于 2025-3-25 07:55:03 | 只看該作者
23#
發(fā)表于 2025-3-25 13:25:52 | 只看該作者
24#
發(fā)表于 2025-3-25 18:46:35 | 只看該作者
Motion Around Black HolesThe chapter reviews the geodesic motion of massless and massive particles in stationary, axisymmetric, and asymptotically flat spacetimes and in the particular case of the Kerr metric.
25#
發(fā)表于 2025-3-25 21:24:36 | 只看該作者
Astrophysical Black HolesThe chapter reviews the astrophysical observations of stellar-mass black holes, intermediate mass black holes, supermassive black holes, the observations supporting the idea that these objects are indeed black holes, and the spectral state classification.
26#
發(fā)表于 2025-3-26 02:52:33 | 只看該作者
27#
發(fā)表于 2025-3-26 05:55:11 | 只看該作者
Continuum-Fitting MethodThe chapter reviews the continuum-fitting method, namely the technique to fit the thermal spectrum of a geometrically thin and optically thick accretion disk of a black hole to probe the metric close to the compact object.
28#
發(fā)表于 2025-3-26 12:00:12 | 只看該作者
X-Ray Reflection SpectroscopyX-ray reflection spectroscopy is the study of the reflection spectrum of a thin accretion disk. The reflection spectrum has some emission lines and the most prominent one is usually the iron K. line. The reflection spectrum is generated in the inner part of the accretion disk and it can be employed to probe the metric close to the black hole.
29#
發(fā)表于 2025-3-26 16:41:55 | 只看該作者
30#
發(fā)表于 2025-3-26 17:44:49 | 只看該作者
Gravitational WavesThe chapter briefly reviews gravitational waves from black hole coalescences, gravitational waves from extreme-mass ratio inspirals, and quasi-normal modes from black holes.
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