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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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发表于 2025-3-21 17:12:01 | 显示全部楼层 |阅读模式
期刊全称Black Holes: A Laboratory for Testing Strong Gravity
影响因子2023Cosimo Bambi
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发行地址Provides 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
图书封面Titlebook: Black Holes: A Laboratory for Testing Strong Gravity;  Cosimo Bambi Textbook 2017 Springer Nature Singapore Pte Ltd. 2017 textbook black ho
影响因子. .This textbook introduces the current astrophysical observations of black holes, and discusses the leading techniques to study the strong gravity region 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 geometry around these objects should be well described by the Kerr solution. The electromagnetic radiation emitted by the gas in the inner part of the accretion disk can probe the metric of the strong gravity region and test the Kerr black hole hypothesis. With exercises and examples in each chapter, as well as calculations and analytical details in the appendix, the book is especially useful to the beginners or graduate students who are familiar with general relativity while they do not have any background in astronomy or astrophysics.<.
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发表于 2025-3-21 22:16:50 | 显示全部楼层
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.
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发表于 2025-3-22 11:52:33 | 显示全部楼层
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.
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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
发表于 2025-3-22 23:29:12 | 显示全部楼层
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
发表于 2025-3-23 02:54:07 | 显示全部楼层
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.
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