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説明
We discuss the gravitationally interacting system of a thick domain wall and a black hole. We numerically solve the scalar field equation in the Schwarzschild spacetime and obtain a sequence of static axi-symmetric solutions representing thick domain walls. We find that, for the walls near the horizon, the Nambu--Goto approximation is no longer valid.
18 pages, 11 figures, one reference added
収録刊行物
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- Physical Review D
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Physical Review D 67 2003-01-28
American Physical Society (APS)
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詳細情報 詳細情報について
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- CRID
- 1871991017856884352
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- ISSN
- 10894918
- 05562821
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- データソース種別
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- OpenAIRE