Proof of the angular momentum-mass inequality for axisymmetric black holes

被引:0
作者
Dain, Sergio [1 ,2 ]
机构
[1] Univ Nacl Cordoba, Fac Math Astron & Fis, RA-5000 Cordoba, Argentina
[2] Albert Einstein Inst, Max Planck Inst Gravitat Phys, D-14476 Potsdam, Germany
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中图分类号
O1 [数学];
学科分类号
0701 ; 070101 ;
摘要
We prove that an extreme Kerr initial data set is a unique absolute minimum of the total mass in a (physically relevant) class of vacuum, maximal, asymptotically flat, axisymmetric data for Einstein equations with fixed angular momentum. These data represent non-stationary, axially symmetric black holes. As a consequence, we obtain that any data in this class satisfy the inequality root J <= m, where m and J are the total mass and angular momentum of spacetime.
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页码:33 / 67
页数:35
相关论文
共 46 条
[1]  
[Anonymous], 1983, GRADUATE TEXTS MATH
[2]  
Arnowitt R., 1962, DYNAMICS GEN RELATIV
[3]   THE MASS OF AN ASYMPTOTICALLY FLAT MANIFOLD [J].
BARTNIK, R .
COMMUNICATIONS ON PURE AND APPLIED MATHEMATICS, 1986, 39 (05) :661-693
[4]   TIME-ASYMMETRIC INITIAL DATA FOR BLACK-HOLES AND BLACK-HOLE COLLISIONS [J].
BOWEN, JM ;
YORK, JW .
PHYSICAL REVIEW D, 1980, 21 (08) :2047-2056
[6]   NECESSARY AND SUFFICIENT CONDITION FOR YORK DATA TO SPECIFY AN ASYMPTOTICALLY FLAT SPACETIME [J].
CANTOR, M .
JOURNAL OF MATHEMATICAL PHYSICS, 1979, 20 (08) :1741-1744
[7]  
CANTOR M, 1981, COMPOS MATH, V43, P317
[9]   AXISYMMETRIC BLACK HOLE HAS ONLY 2 DEGREES OF FREEDOM [J].
CARTER, B .
PHYSICAL REVIEW LETTERS, 1971, 26 (06) :331-+
[10]  
CARTER B, 1999, 8 M GROSSM M A B JER, P136