Boosted three-dimensional black-hole evolutions with singularity excision

被引：84

作者：

Cook, GB ^{[1
]}

Huq, MF

Klasky, SA

Scheel, MA

Abrahams, AM

Anderson, A

Anninos, P

Baumgarte, TW

Bishop, NT

Brandt, SR

Browne, JC

Camarda, K

Choptuik, MW

Correll, RR

Evans, CR

Finn, LS

Fox, GC

Gomez, R

Haupt, T

Kidder, LE

Laguna, P

Landry, W

Lehner, L

Lenaghan, J

Marsa, RL

Masso, J

Matzner, RA

Mitra, S

Papadopoulos, P

Parashar, M

Rezzolla, L

Rupright, ME

Saied, F

Saylor, PE

Seidel, E

Shapiro, SL

Shoemaker, D

Smarr, L

Suen, WM

Szilagyi, B

Teukolsky, SA

van Putten, MHPM

Walker, P

Winicour, J

York, JW

机构：

[1] Cornell Univ, Ithaca, NY 14853 USA

[2] Univ Texas, Austin, TX 78712 USA

[3] Syracuse Univ, Syracuse, NY 13244 USA

[4] Univ Illinois, Urbana, IL 61801 USA

[5] JP Morgan, New York, NY 10260 USA

[6] Univ N Carolina, Chapel Hill, NC 27599 USA

[7] Univ S Africa, ZA-0001 Pretoria, South Africa

[8] Penn State Univ, University Pk, PA 16802 USA

[9] AF Space Command, Peterson AFB, CO 80914 USA

[10] Northwestern Univ, Evanston, IL 60208 USA

[11] Univ Pittsburgh, Pittsburgh, PA 15260 USA

[12] Washington Univ, St Louis, MO 63130 USA

来源：

PHYSICAL REVIEW LETTERS | 1998年 / 80卷 / 12期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1103/PhysRevLett.80.2512

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Binary black-hole interactions provide potentially the strongest source of gravitational radiation for detectors currently under development. We present some results from the Binary Black Hole Grand Challenge Alliance three-dimensional Cauchy evolution module. These constitute essential steps towards modeling such interactions and predicting gravitational radiation waveforms. We report on single black-hole evolutions and the first successful demonstration of a black hole moving freely through a three-dimensional computational grid via a Cauchy evolution: a hole moving near 6M at 0.1c during a total evolution of duration near 60M.

引用

页码：2512 / 2516

页数：5

共 19 条

[11]

HUQ MF, 1996, THESIS U TEXAS AUSTI

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