Size of the smallest scales in cosmic string networks
被引:47
作者:
Siemens, X
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h-index: 0
机构:
Tufts Univ, Dept Phys & Astron, Inst Cosmol, Medford, MA 02155 USATufts Univ, Dept Phys & Astron, Inst Cosmol, Medford, MA 02155 USA
Siemens, X
[1
]
Olum, KD
论文数: 0引用数: 0
h-index: 0
机构:
Tufts Univ, Dept Phys & Astron, Inst Cosmol, Medford, MA 02155 USATufts Univ, Dept Phys & Astron, Inst Cosmol, Medford, MA 02155 USA
Olum, KD
[1
]
论文数: 引用数:
h-index:
机构:
Vilenkin, A
[1
]
机构:
[1] Tufts Univ, Dept Phys & Astron, Inst Cosmol, Medford, MA 02155 USA
来源:
PHYSICAL REVIEW D
|
2002年
/
66卷
/
04期
关键词:
D O I:
10.1103/PhysRevD.66.043501
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We present a method for the calculation of the gravitational back-reaction cutoff on the smallest scales of cosmic string networks taking into account that not all modes on strings interact with all other modes. This results in a small scale structure cutoff that is sensitive to the initial spectrum of perturbations present on strings. From a simple model, we compute cutoffs in radiation- and matter-dominated universes which are much smaller than the results usually presented in the literature.