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Three-dimensional distorted black holes
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DOI：10.1088/0264-9381/20/1/301.png)
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摘要
En 中文
We present three-dimensional, non-axisymmetric distorted black-hole initial data which generalize the axisymmetric, distorted, non-rotating [1] and rotating [2] single black-hole data developed by Bernstein, Brandt and Seidel. These initial data should be useful for studying the dynamics of fully 3D, distorted black holes, such as those created by the spiralling coalescence of two black holes. We describe the mathematical construction of several families of such datasets, and show how to construct numerical solutions. We survey quantities associated with the numerically constructed solutions, such as ADM masses, apparent horizons, measurements of the horizon distortion and the maximum possible radiation loss.
Keyword:
INITIAL DATA
GRAVITATIONAL-WAVES
CLOSE LIMIT
EVOLUTION
COLLISIONS
DYNAMICS
SINGULARITIES
BINARIES
SYSTEMS
ORDER
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期刊
IF:
3.7
论文数:
1.3W
被引数:
3.0W
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