DYNAMICS OF APPARENT AND EVENT HORIZONS

被引:58
作者
ANNINOS, P
BERNSTEIN, D
BRANDT, S
LIBSON, J
MASSO, J
SEIDEL, E
SMARR, L
SUEN, WM
WALKER, P
机构
[1] UNIV ILLES BALEARS,DEPT FIS,E-07071 PALMA DE MALLORCA,SPAIN
[2] UNIV ILLINOIS,DEPT PHYS,URBANA,IL 61801
[3] WASHINGTON UNIV,MCDONNELL CTR SPACE SCI,DEPT PHYS,ST LOUIS,MO 63130
关键词
D O I
10.1103/PhysRevLett.74.630
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We have developed a powerful and efficient new method in numerical relativity for locating the event horizon to high accuracy, making possible the study of horizon dynamics in highly nonlinear black-hole spacetimes. We analyzed and compared evolutions of the apparent and event horizons of both Schwarzschild and Kerr black holes struck by strong bursts of gravitational radiation, and of colliding black holes. In all black-hole spacetimes studied, the horizons oscillate with the quasinormal frequency at late times. © 1995 The American Physical Society.
引用
收藏
页码:630 / 633
页数:4
相关论文
共 14 条
  • [1] COLLISION OF 2 BLACK-HOLES
    ANNINOS, P
    HOBILL, D
    SEIDEL, E
    SMARR, L
    SUEN, WM
    [J]. PHYSICAL REVIEW LETTERS, 1993, 71 (18) : 2851 - 2854
  • [2] ANNINOS P, IN PRESS
  • [3] ANNINOS P, 1994, NUMERICAL ASTROPHYSI
  • [4] NUMERICALLY GENERATED AXISYMMETRICAL BLACK-HOLE SPACETIMES - NUMERICAL-METHODS AND CODE TESTS
    BERNSTEIN, D
    HOBILL, D
    SEIDEL, E
    SMARR, L
    TOWNS, J
    [J]. PHYSICAL REVIEW D, 1994, 50 (08): : 5000 - 5024
  • [5] BRANDT S, IN PRESS
  • [6] BRANDT S, 1993, P PENN STATE NUMERIC
  • [7] CARTER B, 1979, GENERAL RELATIVITY E
  • [8] APPARENT HORIZONS FOR BOOSTED OR SPINNING BLACK-HOLES
    COOK, GB
    YORK, JW
    [J]. PHYSICAL REVIEW D, 1990, 41 (04): : 1077 - 1085
  • [9] Ellis G. F. R., 1973, LARGE SCALE STRUCTUR
  • [10] HOOP CONJECTURE FOR BLACK-HOLE HORIZON FORMATION
    FLANAGAN, E
    [J]. PHYSICAL REVIEW D, 1991, 44 (08): : 2409 - 2420