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A no-boundary method for numerical relativity
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DOI：10.1088/1361-6382/ab5e99.png)
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摘要
En 中文
We propose a method for numerical relativity in which the spatial grid is finite and no outer boundary condition is needed. As a 'proof of concept' we implement this method for the case of a self-gravitating, spherically symmetric scalar field.
Keyword:
numerical relativity
boundary conditions
black hole formation
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期刊
IF:
3.7
论文数:
1.3W
被引数:
3.0W
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