Angular momentum at the black hole threshold

被引:14
作者
Gundlach, C [1 ]
机构
[1] Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14473 Potsdam, Germany
来源
PHYSICAL REVIEW D | 1998年 / 57卷 / 12期
关键词
D O I
10.1103/PhysRevD.57.R7080
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Near the black hole threshold in phase space, the black hole mass as a function of the initial data shows the "critical scaling" M similar or equal to C(p-p*)(gamma), where p labels a family of initial data, p* is the value of p at the threshold, and the critical exponent gamma is universal for a given matter model. The black hole charge Q obeys a similar law. To complete the picture, we include the angular momentum as a perturbation. For the black hole angular momentum (L) over right arrow, we find the oscillating behavior (L) over right arrow similar or equal to Re[((A) over left arrow + i (B) over right arrow)(p-p*)(mu+i omega)]. The assumptions of the calculation hold for p=rho/3 perfect fluid matter, and we calculate mu similar or equal to 0.799 and omega similar or equal to 0.231.
引用
收藏
页码:R7080 / R7083
页数:4
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