Gravitational wave extraction and outer boundary conditions by perturbative matching

被引：83

作者：

Abrahams, AM ^{[1
]}

Rezzolla, L

Rupright, ME

Anderson, A

Anninos, P

Baumgarte, TW

Bishop, NT

Brandt, SR

Browne, JC

Camarda, K

Choptuik, MW

Cook, GB

Correll, RR

Evans, CR

Finn, LS

Fox, GC

Gomez, R

Haupt, T

Huq, MF

Kidder, LE

Klasky, SA

Laguna, P

Landry, W

Lehner, L

Lenaghan, J

Marsa, RL

Masso, J

Matzner, RA

Mitra, S

Papadopoulos, P

Parashar, M

Saied, F

Saylor, PE

Scheel, MA

Seidel, E

Shapiro, SL

Shoemaker, D

Smarr, L

Szilagyi, B

Teukolsky, SA

van Putten, MHPM

Walker, P

Winicour, J

York, JW

机构：

[1] Univ Illinois, Urbana, IL 61801 USA

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

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

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

[5] Univ Texas, Austin, TX 78712 USA

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

[7] Cornell Univ, Ithaca, NY 14853 USA

[8] Northwestern Univ, Evanston, IL 60208 USA

[9] Syracuse Univ, Syracuse, NY 13244 USA

[10] Univ Pittsburgh, Pittsburgh, PA 15260 USA

来源：

PHYSICAL REVIEW LETTERS | 1998年 / 80卷 / 09期

关键词：

D O I：

10.1103/PhysRevLett.80.1812

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

We present a method for extracting gravitational radiation from a three-dimensional numerical relativity simulation and, using the extracted data, to provide outer boundary conditions. The method treats dynamical gravitational variables as nonspherical perturbations of Schwarzschild geometry. We discuss a code which implements this method and present results of tests which have been performed with a three-dimensional numerical relativity code.

引用

页码：1812 / 1815

页数：4

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