找回密码
 To register

QQ登录

只需一步,快速开始

扫一扫,访问微社区

Titlebook: Black Hole Physics; Basic Concepts and N Valeri P. Frolov,Igor D. Novikov Book 1998 Springer Science+Business Media Dordrecht 1998 Gravity.

[复制链接]
楼主: 正当理由
发表于 2025-3-25 07:02:22 | 显示全部楼层
发表于 2025-3-25 11:02:29 | 显示全部楼层
发表于 2025-3-25 13:19:21 | 显示全部楼层
Kurven, Kegel und Zylinder zweiter Ordnungherically symmetric. The . (spacetime with spherical three-dimensional space) is described in every textbook on general relativity [see, e.g., Landau and Lifshitz (1975), Misner, Thorne, and Wheeler (1973)]. Therefore, here we will only reproduce the necessary results. Mathematical details connected
发表于 2025-3-25 17:53:00 | 显示全部楼层
发表于 2025-3-25 20:11:40 | 显示全部楼层
Die Durchdringungslinien von Vielflachens. Both Schwarzschild and Kerr spacetimes are stationary and possess certain symmetries. A study of geodesies (corresponding to the motion of test particles and light rays) and wave fields in these metrics enabled us to describe a number of interesting and important features of physical effects in t
发表于 2025-3-26 01:31:46 | 显示全部楼层
Die Durchdringungslinien von Vielflachenlyzing the efficiency of energy extraction from black holes. Recall that although a black hole is by definition a region of no escape for material bodies and light rays, situations are possible in which energy can be extracted via certain physical processes. We will see later that this energy is ext
发表于 2025-3-26 05:56:05 | 显示全部楼层
Lehrbuch der darstellenden Geometrieo observation by distant observers. At first glance, black hole electrodynamics is quite trivial. Indeed, the electromagnetic field of a stationary black hole (of a given mass .) is determined unambiguously by its electric charge . and rotation parameter .. If the charged black hole does not rotate,
发表于 2025-3-26 10:11:54 | 显示全部楼层
发表于 2025-3-26 16:21:31 | 显示全部楼层
Lehrbuch der darstellenden Geometrieare, indeed, insignificant for black holes of about a solar mass (and greater). However, for a small-mass (primordial) black hole these effects cannot be ignored; in fact, they qualitatively change the black hole’s evolution. They are also likely to become important for those regions inside a black
发表于 2025-3-26 20:12:58 | 显示全部楼层
Die Ellipse: Konjugierte Durchmessersehnen drawing the inevitable conclusion that the particle flux to infinity which carries away positive energy is accompanied by a flux of negative energy across the horizon into the black hole. This would be impossible in classical theory, with ordinary physical assumptions satisfied (energy dominance co
 关于派博传思  派博传思旗下网站  友情链接
派博传思介绍 公司地理位置 论文服务流程 影响因子官网 SITEMAP 大讲堂 北京大学 Oxford Uni. Harvard Uni.
发展历史沿革 期刊点评 投稿经验总结 SCIENCEGARD IMPACTFACTOR 派博系数 清华大学 Yale Uni. Stanford Uni.
|Archiver|手机版|小黑屋| 派博传思国际 ( 京公网安备110108008328) GMT+8, 2025-5-28 01:02
Copyright © 2001-2015 派博传思   京公网安备110108008328 版权所有 All rights reserved
快速回复 返回顶部 返回列表