抄録
Wormhole formation is studied numerically by using a spherically symmetric cosmological code. Preparing a suitable initial inhomogeneity of a scalar field, we find that wormhole formation occurs. The criterion of wormhole formation is investigated and we find that it is in good agreement with the result of the thin-wall approximation.
本文言語 | 英語 |
---|---|
ページ(範囲) | 5367-5377 |
ページ数 | 11 |
ジャーナル | Physical Review D |
巻 | 46 |
号 | 12 |
DOI | |
出版ステータス | 出版済み - 1992 |
外部発表 | はい |
!!!All Science Journal Classification (ASJC) codes
- 物理学および天文学(その他)