Towards an understanding of the stability properties of the 3+1 evolution equations in general relativity -: art. no. 124011

被引:83
作者
Alcubierre, M
Allen, G
Brügmann, B
Seidel, E
Suen, WM
机构
[1] Albert Einstein Inst, Max Planck Inst Gravitat Phys, D-14476 Golm, Germany
[2] Univ Illinois, Beckman Inst, Natl Ctr Supercomp Applicat, Urbana, IL 61801 USA
[3] Washington Univ, Dept Phys, St Louis, MO 63130 USA
[4] Chinese Univ Hong Kong, Dept Phys, Hong Kong, Hong Kong, Peoples R China
来源
PHYSICAL REVIEW D | 2000年 / 62卷 / 12期
关键词
D O I
10.1103/PhysRevD.62.124011
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the stability properties of the standard ADM formulation of the 3+1 evolution equations of general relativity through linear perturbations of flat spacetime. We focus attention on modes with zero speed of propagation and conjecture that they are responsible for instabilities encountered in numerical evolutions of the ADM formulation. These zero speed modes are of two kinds: pure gauge modes and constraint violating modes. We show how the decoupling of the gauge by a conformal rescaling can eliminate the problem with the gauge modes. The zero speed constraint violating modes can be dealt with by using the momentum constraints to give them a finite speed of propagation. This analysis sheds some light on the question of why some recent reformulations of the 3+1 evolution equations have better stability properties than the standard ADM formulation.
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页码:1 / 15
页数:15
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