Автор |
Kouji Nakamura |
Дата выпуска |
2002-02-21 |
dc.description |
The initial data of the gravitational field produced by a thick loop string are considered. We show that a thick loop is not a geodesic on the initial hypersurface, while a loop conical singularity is. This suggests that there is a critical thickness of a string, at which the linear perturbation theory with a flat space background fails to describe the gravity of a loop cosmic string. Using the above initial data, we also show that the linear perturbation around the flat space is plausible if the string thickness is larger than ∼5 × 10<sup>−3</sup>a, where a is the curvature radius of the loop. |
Формат |
application.pdf |
Издатель |
Institute of Physics Publishing |
Название |
Initial condition of a gravitating thick loop cosmic string and linear perturbations |
Тип |
paper |
DOI |
10.1088/0264-9381/19/4/310 |
Electronic ISSN |
1361-6382 |
Print ISSN |
0264-9381 |
Журнал |
Classical and Quantum Gravity |
Том |
19 |
Первая страница |
783 |
Последняя страница |
797 |
Аффилиация |
Kouji Nakamura; Theory Division, National Astronomical Observatory, Mitaka, Tokyo, 181-8588, Japan; Department of Physics, Keio University, Hiyoshi Yokohama, 223-8521, Japan |
Выпуск |
4 |