{"title":"Black holes","authors":"A. Steane","doi":"10.1093/oso/9780192895646.003.0020","DOIUrl":null,"url":null,"abstract":"We discuss event horizons and black holes. First Birkhoff’s theorem is derived, and we consider the general nature of spherically symmetric spaces. Then the concepts of null surface, Killing horizon and event horizon are defined and related to one another. Cosmic censorship is briefly discussed. The Schwarzshild horizon is discussed in detail. The divergence or otherwise of redshift, acceleration, speed and proper time is obtained for infalling observers and for Schwarzschild observers. Eddington-Finkelstein coordinates are introduced and used to discuss gravitational collapse. The growth of the horizon is noted, and the causality structure is briefly considered via an introduction to the conformal (Penrose-Carter) diagram. The maximal extension is then presented, with the Kruskal-Szekeres coordinates and associated diagram. Wormholes are briefly discussed. The chapter finishes with a survey of astronomical evidence for black holes.","PeriodicalId":365636,"journal":{"name":"Relativity Made Relatively Easy Volume 2","volume":"24 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2021-11-02","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Relativity Made Relatively Easy Volume 2","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1093/oso/9780192895646.003.0020","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
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Abstract

We discuss event horizons and black holes. First Birkhoff’s theorem is derived, and we consider the general nature of spherically symmetric spaces. Then the concepts of null surface, Killing horizon and event horizon are defined and related to one another. Cosmic censorship is briefly discussed. The Schwarzshild horizon is discussed in detail. The divergence or otherwise of redshift, acceleration, speed and proper time is obtained for infalling observers and for Schwarzschild observers. Eddington-Finkelstein coordinates are introduced and used to discuss gravitational collapse. The growth of the horizon is noted, and the causality structure is briefly considered via an introduction to the conformal (Penrose-Carter) diagram. The maximal extension is then presented, with the Kruskal-Szekeres coordinates and associated diagram. Wormholes are briefly discussed. The chapter finishes with a survey of astronomical evidence for black holes.
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黑洞
我们讨论了视界和黑洞。首先推导了Birkhoff定理,并考虑了球对称空间的一般性质。然后定义了零曲面、杀伤视界和事件视界的概念,并将它们联系起来。简要讨论了宇宙审查制度。详细讨论了史瓦西视界。得到了落体观测者和史瓦西观测者的红移、加速度、速度和固有时的散度。引入Eddington-Finkelstein坐标,并将其用于讨论引力坍缩。注意到视界的增长,并通过介绍保形图(Penrose-Carter)简要地考虑因果关系结构。然后用Kruskal-Szekeres坐标和相关图给出了最大扩展。简要讨论虫洞。本章以对黑洞的天文学证据的调查结束。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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Rotating bodies; the Kerr metric Black hole thermodynamics Further spherically symmetric solutions Cosmological dynamics Linearized General Relativity
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