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Titlebook: Black Hole Physics; From Collapse to Eva Daniel Grumiller,Mohammad Mehdi Sheikh-Jabbari Textbook 2022 The Editor(s) (if applicable) and The

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31#
發(fā)表于 2025-3-27 00:59:34 | 只看該作者
Textbook 2022and want to get up-to-date on recent and current research topics; advanced researchers intending to teach (or learn) basic and advanced aspects of black hole physics and the associated mathematical tools. Besides general relativity, the reader needs to be familiar with standard undergraduate physics
32#
發(fā)表于 2025-3-27 04:26:39 | 只看該作者
33#
發(fā)表于 2025-3-27 07:52:17 | 只看該作者
1868-4513 he gravitational waves detection.Includes a plethora of exer.This textbook gradually introduces the reader to several topics related to black hole physics with a didactic approach. It starts with the most basic black hole solution, the Schwarzschild metric, and discusses the basic classical properti
34#
發(fā)表于 2025-3-27 09:35:13 | 只看該作者
Marc Lucotte,Shelagh Montgomery,Maxime Bégin. .. We discuss the core collapse of typical stars to black holes at the end of the star’s lifetime in Sect. .. Besides their observational richness, black holes give rise to several profound theoretical questions, particularly in the context of QG. We summarize different schools of thought developed to address them in Sect. ..
35#
發(fā)表于 2025-3-27 14:51:56 | 只看該作者
Mercury in the Biogeochemical Cyclee, captured by Carter–Penrose diagrams, is presented in Sect. .. Thereafter, we generalize from Schwarzschild black holes to Reissner–Nordstr?m (Sect. .), Kerr (Sect. .), Kottler and Kerr (A)dS (Sect. .), Plebanski–Demianski (Sect. .), and Vaydia (Sect. .).
36#
發(fā)表于 2025-3-27 18:56:23 | 只看該作者
37#
發(fā)表于 2025-3-27 22:01:25 | 只看該作者
38#
發(fā)表于 2025-3-28 05:11:17 | 只看該作者
39#
發(fā)表于 2025-3-28 09:11:44 | 只看該作者
,Black Hole Charges and?Thermodynamics,is method can be used for asymptotically stationary black holes, it is most conveniently used for stationary black holes with a Killing horizon. For the latter family, we provide a concise derivation of the entropy as Noether charge in Sect.?. and of the four laws of black hole thermodynamics in Sect.?..
40#
發(fā)表于 2025-3-28 10:48:54 | 只看該作者
https://doi.org/10.1007/978-1-349-25464-4). We then review Bekenstein’s arguments for black hole entropy and entropy bounds in Sect.?.. In Sect.?., we discuss tunneling, in Sect.?. black hole evaporation, and in Sect.?. the membrane paradigm. We close this chapter with preliminary remarks in Sect.?. on the information puzzle and apparent loss of unitarity in the semiclassical analysis.
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