领口
发表于 2025-3-21 17:12:01
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–FER
发表于 2025-3-21 22:16:50
https://doi.org/10.1007/978-3-476-02758-0in a stationary and axisymmetric spacetime and in the Kerr metric in particular. Last, the chapter discusses possible deviations from the Kerr background due to the presence of an accretion disk or of a non-vanishing electric charge of the central black hole.
IVORY
发表于 2025-3-22 00:58:38
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Fretful
发表于 2025-3-22 05:57:40
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Cumulus
发表于 2025-3-22 11:52:33
Non-Kerr Spacetimesmetric. In the bottom-up approach, we consider instead a phenomenological parameterization of the metric, which ideally should be able to describe the spacetime of any possible black hole in any possible gravity theory.
模范
发表于 2025-3-22 16:22:14
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Acclaim
发表于 2025-3-22 20:24:34
Textbook 2017gion around these objects with electromagnetic radiation. More importantly, it provides the basic tools for writing an astrophysical code and testing the Kerr paradigm. Astrophysical black holes are an ideal laboratory for testing strong gravity. According to general relativity, the spacetime geomet
fulmination
发表于 2025-3-22 23:29:12
https://doi.org/10.1007/978-3-476-02758-0holes, 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
是突袭
发表于 2025-3-23 02:54:07
Ausgleichung nach Tschebyscheff,lity 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.
小故事
发表于 2025-3-23 07:48:57
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