標(biāo)題: Titlebook: Black Hole Physics; From Collapse to Eva Daniel Grumiller,Mohammad Mehdi Sheikh-Jabbari Textbook 2022 The Editor(s) (if applicable) and The [打印本頁] 作者: ANNOY 時間: 2025-3-21 19:29
書目名稱Black Hole Physics影響因子(影響力)
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書目名稱Black Hole Physics網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Black Hole Physics被引頻次
書目名稱Black Hole Physics被引頻次學(xué)科排名
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書目名稱Black Hole Physics讀者反饋
書目名稱Black Hole Physics讀者反饋學(xué)科排名
作者: 表否定 時間: 2025-3-22 00:00
Black Hole Solutions and Basic Properties, Sect. .. In Sect. ., we analyze particle probes and geodesics in a Schwarzschild background. The maximal extension, near horizon, and causal structure, captured by Carter–Penrose diagrams, is presented in Sect. .. Thereafter, we generalize from Schwarzschild black holes to Reissner–Nordstr?m (Sect.作者: 青石板 時間: 2025-3-22 02:51
Formal Definitions and Classic Theorems,es and various definitions of horizons. We discuss their physical significance. In Sect. ., we summarize classic theorems and conjectures, namely singularity theorems, focusing theorem, area theorem, uniqueness theorems, topology theorems, and the cosmic censorship conjecture. In Sect. ., we focus o作者: HAIRY 時間: 2025-3-22 07:57
Probing Black Holes, Their Formation and Stability,e probed by light or other fields scattered off them leading to gravitational lensing, black hole shadows, and associated images, as discussed in Sect. .. Superradiance, the Penrose process, and black hole mining are investigated in Sect. .. GW from black hole mergers can be (and have been) detected作者: Frequency-Range 時間: 2025-3-22 08:55
,Black Hole Charges and?Thermodynamics, We then introduce the solution phase space method as a precise and handy formulation to define conserved charges for black holes in Sect.?.. While this method can be used for asymptotically stationary black holes, it is most conveniently used for stationary black holes with a Killing horizon. For t作者: 動物 時間: 2025-3-22 13:51
Semiclassical Aspects of Black Holes,particles are treated quantum mechanically. We first discuss the variational principle for gravity theories in Sect.?.. Then, in Sect.?., we briefly review QFT on curved backgrounds, which leads to the Unruh effect (Sect.?.) and, when applied to black hole backgrounds, to the Hawking effect (Sect.?.作者: 描述 時間: 2025-3-22 19:24 作者: MELON 時間: 2025-3-23 01:17
Aspects of Holography,ding chapters, the sections herein are self-contained. Therefore, readers familiar with more basic material can read them independently from the earlier parts of the book. Section . introduces basics of holography. Section . is devoted to the holographic formulation of quantum information-theoretic 作者: Reverie 時間: 2025-3-23 04:09 作者: judicial 時間: 2025-3-23 08:07 作者: ALE 時間: 2025-3-23 11:49 作者: 陶醉 時間: 2025-3-23 15:00
Graduate Texts in Physicshttp://image.papertrans.cn/b/image/188945.jpg作者: 壟斷 時間: 2025-3-23 20:45
Marc Lucotte,Shelagh Montgomery,Maxime Béginof general relativity (GR) in Sect. .. We then provide a historic summary of black holes, both from theoretical and observational perspectives in Sect. .. 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, 作者: 極小 時間: 2025-3-24 01:14
Mercury in the Biogeochemical Cycle Sect. .. In Sect. ., we analyze particle probes and geodesics in a Schwarzschild background. The maximal extension, near horizon, and causal structure, captured by Carter–Penrose diagrams, is presented in Sect. .. Thereafter, we generalize from Schwarzschild black holes to Reissner–Nordstr?m (Sect.作者: 檔案 時間: 2025-3-24 03:30
https://doi.org/10.1007/978-94-010-0403-9es and various definitions of horizons. We discuss their physical significance. In Sect. ., we summarize classic theorems and conjectures, namely singularity theorems, focusing theorem, area theorem, uniqueness theorems, topology theorems, and the cosmic censorship conjecture. In Sect. ., we focus o作者: HAUNT 時間: 2025-3-24 07:13
https://doi.org/10.1007/978-94-010-0403-9e probed by light or other fields scattered off them leading to gravitational lensing, black hole shadows, and associated images, as discussed in Sect. .. Superradiance, the Penrose process, and black hole mining are investigated in Sect. .. GW from black hole mergers can be (and have been) detected作者: BROW 時間: 2025-3-24 11:39 作者: 諂媚于人 時間: 2025-3-24 16:42
https://doi.org/10.1007/978-1-349-25464-4particles are treated quantum mechanically. We first discuss the variational principle for gravity theories in Sect.?.. Then, in Sect.?., we briefly review QFT on curved backgrounds, which leads to the Unruh effect (Sect.?.) and, when applied to black hole backgrounds, to the Hawking effect (Sect.?.作者: Morose 時間: 2025-3-24 19:52 作者: Jogging 時間: 2025-3-25 02:59
Developing the Mereology of Chemistryding chapters, the sections herein are self-contained. Therefore, readers familiar with more basic material can read them independently from the earlier parts of the book. Section . introduces basics of holography. Section . is devoted to the holographic formulation of quantum information-theoretic 作者: Infantry 時間: 2025-3-25 06:31
Building Enduring Objects Out of Spacetimeme general aspects of black holes in QG. In Sect.?. we discuss black hole complementarity and firewalls. In Sect.?. we focus on black holes in string theory. In Sect.?. we review microstate countings for certain supersymmetric black holes, in particular, we discuss the celebrated Cardy formula, whic作者: Hyperalgesia 時間: 2025-3-25 09:44
Claudio Calosi,Pierluigi GrazianiIn this final chapter, we start with a summary of our book in Sect.?., continue with selected open conceptual issues that are the subject of ongoing research in Sect.?. and then finish in Sect.?. with future observational prospects.作者: Evocative 時間: 2025-3-25 15:01 作者: Anemia 時間: 2025-3-25 19:52 作者: Fermentation 時間: 2025-3-25 22:42
https://doi.org/10.1007/978-94-010-0403-9es and various definitions of horizons. We discuss their physical significance. In Sect. ., we summarize classic theorems and conjectures, namely singularity theorems, focusing theorem, area theorem, uniqueness theorems, topology theorems, and the cosmic censorship conjecture. In Sect. ., we focus on the area theorem, also known as the second law.作者: judiciousness 時間: 2025-3-26 00:14 作者: demote 時間: 2025-3-26 05:38 作者: 龍蝦 時間: 2025-3-26 08:40 作者: dithiolethione 時間: 2025-3-26 16:19 作者: Gentry 時間: 2025-3-26 19:43 作者: Exuberance 時間: 2025-3-27 00:59
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作者: Spinal-Tap 時間: 2025-3-27 04:26 作者: jovial 時間: 2025-3-27 07:52
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作者: 小教堂 時間: 2025-3-27 09:35
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. ..作者: myalgia 時間: 2025-3-27 14:51
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. .).作者: habitat 時間: 2025-3-27 18:56 作者: NEEDY 時間: 2025-3-27 22:01 作者: monochromatic 時間: 2025-3-28 05:11 作者: 地名詞典 時間: 2025-3-28 09:11
,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.?..作者: jovial 時間: 2025-3-28 10:48
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.作者: Munificent 時間: 2025-3-28 15:54 作者: 彎腰 時間: 2025-3-28 19:38 作者: ANNUL 時間: 2025-3-28 23:07
Semiclassical Aspects of Black Holes,). 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.作者: conduct 時間: 2025-3-29 03:37
