DYNAMICAL FRICTION ON COSMIC-STRING MOTION AND MAGNETIC-FIELD GENERATION

被引:23
|
作者
AVELINO, PP
SHELLARD, EPS
机构
[1] Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Cambridge CB3 9EW, Silver Street
来源
PHYSICAL REVIEW D | 1995年 / 51卷 / 10期
关键词
D O I
10.1103/PhysRevD.51.5946
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We demonstrate that the effects of dynamical friction on the motion of a wiggly cosmic string are much larger than previously estimated for a straight string. Although network simulations are not significantly affected by our results, this does provide a mechanism for transferring linear and angular momentum from the string network to the surrounding matter particles. A consequence of the vorticity produced by this process could be the generation of weak primordial magnetic fields which are necessary to explain observed galactic magnetic fields. © 1995 The American Physical Society.
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页码:5946 / 5949
页数:4
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