Constraining cosmic superstrings with dilaton emission

被引:21
作者
Babichev, E
Kachelriess, M
机构
[1] Max Planck Inst Phys & Astrophys, Werner Heisenberg Inst Phys, D-80805 Munich, Germany
[2] Russian Acad Sci, Inst Nucl Res, Moscow 117312, Russia
基金
俄罗斯基础研究基金会;
关键词
D O I
10.1016/j.physletb.2005.03.053
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Brane inflation predicts the production of cosmic superstrings with tension 10(-12) <= G mu <= 10(-7). Superstring theory predicts also the existence of a dilaton. We show that the emission of dilatons imposes severe constraints on the allowed evolution of a cosmic superstring network. In particular, the detection of gravitational wave burst from cosmic superstrings by LIGO is only possible if the typical length of string loops is much smaller than usually assumed. (c) 2005 Elsevier B.V. All rights reserved.
引用
收藏
页码:1 / 6
页数:6
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