A Rigorous Treatment of Energy Extraction from a Rotating Black Hole

被引:13
|
作者
Finster, F. [1 ]
Kamran, N. [2 ]
Smoller, J. [3 ]
Yau, S. -T. [4 ]
机构
[1] Univ Regensburg, NWF Mathemat I, D-93040 Regensburg, Germany
[2] McGill Univ, Dept Math & Stat, Montreal, PQ H3A 2K6, Canada
[3] Univ Michigan, Dept Math, Ann Arbor, MI 48109 USA
[4] Harvard Univ, Dept Math, Cambridge, MA 02138 USA
基金
美国国家科学基金会; 加拿大自然科学与工程研究理事会;
关键词
KERR GEOMETRY; WAVE-EQUATION; DECAY;
D O I
10.1007/s00220-009-0730-7
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The Cauchy problem is considered for the scalar wave equation in the Kerr geometry. We prove that by choosing a suitable wave packet as initial data, one can extract energy from the black hole, thereby putting supperradiance, the wave analogue of the Penrose process, into a rigorous mathematical framework. We quantify the maximal energy gain. We also compute the infinitesimal change of mass and angular momentum of the black hole, in agreement with Christodoulou's result for the Penrose process. The main mathematical tool is our previously derived integral representation of the wave propagator.
引用
收藏
页码:829 / 847
页数:19
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