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2007

Puncture Evolution of Schwarzschild Black Holes

Brown, J. David

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The moving puncture method is analyzed for a single, non-spinning black hole.

It is shown that the puncture region is not resolved by current numerical codes.
As a result, the geometry near the puncture appears to evolve to an infinitely long cylinder of finite areal radius.
The puncture itself actually remains at spacelike infinity throughout the evolution.

Puncture Evolution of Schwarzschild Black Holes · Around

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Original
2004
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