The Schwarzschild black hole: A general relativistic introduction

被引：0
|
作者：
Heinicke, C [1 ]
Hehl, FW [1 ]
机构：
[1] Univ Cologne, D-5000 Cologne 41, Germany
来源：
GALACTIC BLACK HOLE: LECTURES ON GENERAL RELATIVITY AND ASTROPHYSICS | 2003年
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The gravitational field of a homogeneous spherically symmetric body ('star') is derived in Newton's and in Einstein's gravitational theory, respectively. On the way to these results, Newton's theory is formulated in a quasi-field-theoretical form, its incompatibility with special relativity theory is pointed out, and it is outlined how one arrives at Einstein's field equation. The gravitational field of a simple Einsteinian model star consists of the exterior and the interior Schwarzschild solutions which are joined together at the surface of the star Their derivation and interpretation will be discussed; in particular the Schwarzschild radius (for the sun approximate to 3 km) and its relation to the event horizon of the corresponding black hole will be investigated.
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页码：3 / 34
页数：32
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