Approximately self-similar critical collapse in 2+1 dimensions -: art. no. 044010

被引:10
|
作者
Cavaglià, M
Clément, G
Fabbri, A
机构
[1] Univ Mississippi, Dept Phys & Astron, University, MS 38677 USA
[2] CNRS, LAPTH, Phys Theor Lab, F-74941 Annecy Le Vieux, France
[3] Univ Bologna, Dipartmento Fis, I-40126 Bologna, Italy
[4] Ist Nazl Fis Nucl, Sez Bologna, I-40126 Bologna, Italy
[5] CNRS, Inst Astrophys Paris, GReCO, F-75014 Paris, France
来源
PHYSICAL REVIEW D | 2004年 / 70卷 / 04期
关键词
D O I
10.1103/PhysRevD.70.044010
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Critical collapse of a self-gravitating scalar field in a (2+1)-dimensional spacetime with negative cosmological constant seems to be dominated by a continuously self-similar solution of the field equations without cosmological constant. However, previous studies of linear perturbations in this background were inconclusive. We extend the continuously self-similar solutions to solutions of the field equations with negative cosmological constant, and analyze their linear perturbations. The extended solutions are characterized by a continuous parameter. A suitable choice of this parameter seems to improve the agreement with the numerical results. We also study the dynamics of the apparent horizon in the extended background.
引用
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页数:5
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