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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
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