Understanding critical collapse of a scalar field

被引:105
作者
Gundlach, C [1 ]
机构
[1] INTA, LAEFF, MADRID 28080, SPAIN
关键词
D O I
10.1103/PhysRevD.55.695
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
I construct a spherically symmetric solution for a massless real scalar field minimally coupled to general relativity which is discretely self-similar (DSS) and regular. This solution coincides with the intermediate attractor found by Choptuik in critical gravitational collapse. The echoing period is Delta = 3.4453 +/- 0.0005. The solution is continued to the future self-similarity horizon, which is also the future light cone of a naked singularity. The scalar field and metric are C-1 but not C-2 at this Cauchy horizon. The curvature is finite nevertheless, and the horizon carries regular null data. These are very nearly flat. The solution has exactly one growing perturbation mode, thus confirming the standard explanation for universality. The growth of this mode corresponds to a critical exponent of gamma = 0.374 +/- 0.001, in agreement with the best experimental value. I predict that in critical collapse dominated by a DSS critical solution, the scaling of the black hole mass shows a periodic wiggle, which like gamma is universal. My results carry over to the free complex scalar field. Connections with previous investigations of self-similar scalar field solutions are discussed, as well as an interpretation of Delta and gamma as anomalous dimensions.
引用
收藏
页码:695 / 713
页数:19
相关论文
共 38 条
[21]   The spherically symmetric collapse of a massless scalar field [J].
Hamade, RS ;
Stewart, JM .
CLASSICAL AND QUANTUM GRAVITY, 1996, 13 (03) :497-512
[22]   Continuous self-similarity and S-duality [J].
Hamade, RS ;
Horne, JH ;
Stewart, JM .
CLASSICAL AND QUANTUM GRAVITY, 1996, 13 (08) :2241-2253
[23]  
HARA T, GRQC9607010
[24]   UNIVERSAL SCALING AND ECHOING IN THE GRAVITATIONAL COLLAPSE OF A COMPLEX SCALAR FIELD [J].
HIRSCHMANN, EW ;
EARDLEY, DM .
PHYSICAL REVIEW D, 1995, 51 (08) :4198-4207
[25]   CRITICAL EXPONENTS AND STABILITY AT THE BLACK-HOLE THRESHOLD FOR A COMPLEX SCALAR FIELD [J].
HIRSCHMANN, EW ;
EARDLEY, DM .
PHYSICAL REVIEW D, 1995, 52 (10) :5850-5856
[26]  
HIRSCHMANN EW, GRQC9511052
[27]  
Hod S., 1995, THESIS HEBREW U JERU
[28]  
HOD S, GRQC9606087
[30]   Black hole criticality in the Brans-Dicke model [J].
Liebling, SL ;
Choptuik, MW .
PHYSICAL REVIEW LETTERS, 1996, 77 (08) :1424-1427