Can topological defects be formed during preheating?

被引:42
作者
Kasuya, S [1 ]
Kawasaki, M [1 ]
机构
[1] Univ Tokyo, Inst Cosm Ray Res, Tanashi, Tokyo 188, Japan
关键词
D O I
10.1103/PhysRevD.56.7597
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the dynamics of a scalar field Phi with the potential g(\Phi\(2)-eta(2))(2)/2 (g=self-coupling constant, eta=symmetry breaking scale) after inflation and make clear whether topological defects can ever be formed during preheating. In particular, we pay attention to GUT defects (eta similar or equal to 10(15) GeV-10(17) GeV), and consider three types of fluctuations. The first one is produced through the parametric resonance, the second is due to the negative curvature of the potential, and the last is created during inflation. We search the parameters g and eta for which the nonthermal fluctuations of the scalar field do not lead to the defect formation. We find that the GUT defects an not produced after inflation. This fact shows that the positiveness of the effective mass square of the scalar field and the production of large fluctuations whose amplitude is as large as that of homogeneous mode are not enough conditions for full symmetry restoration. [S0556-2821(97)02524-1].
引用
收藏
页码:7597 / 7607
页数:11
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