天体物理学黑洞:综述

C. Bambi
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引用次数: 19

摘要

在这篇综述中,我试图把重点放在该领域的发展上,从最初的猜测到目前的研究方向。根据爱因斯坦的广义相对论,黑洞是相对简单的物体,完全由质量、自旋角动量和电荷来表征,但在天体物理学的宏观物体中,电荷可以忽略不计。对天空中黑洞的搜索始于20世纪70年代初,当时人们对天鹅座X-1致密天体的质量进行了动态测量。在过去的10-15年里,天文学家开发了一些测量黑洞旋转的技术。最近,我们开始使用天体物理学黑洞来测试基础物理学。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Astrophysical Black Holes: A Review
In this review, I have tried to focus on the development of the field, from the first speculations to the current lines of research. According to Einstein's theory of general relativity, black holes are relatively simple objects and completely characterized by their mass, spin angular momentum, and electric charge, but the latter can be ignored in the case of astrophysical macroscopic objects. Search for black holes in the sky started in the early 1970s with the dynamical measurement of the mass of the compact object in Cygnus X-1. In the past 10-15 years, astronomers have developed some techniques for measuring the black hole spins. Recently, we have started using astrophysical black holes for testing fundamental physics.
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