Physics – High Energy Physics – High Energy Physics - Phenomenology
Scientific paper
1995-12-01
Phys.Rev. D54 (1996) 6083-6087
Physics
High Energy Physics
High Energy Physics - Phenomenology
12 pages, plain TeX; Comments and references added, version to appear in Phys. Rev. D
Scientific paper
10.1103/PhysRevD.54.6083
It is tempting to inflate along one of the many flat directions that arise in supersymmetric theories. The required flatness of the potential to obtain sufficient inflation and to not overproduce density fluctuations occurs naturally. However, the density perturbations (in the case of a single moduli field) that arise from inflaton quantum fluctuations are too small for structure formation. Here we propose that topological defects (such as cosmic strings), which arise during a phase transition near the end of moduli inflation can provide an alternative source of structure. The strings produced will be `fat', yet have the usual evolution by the time of nucleosynthesis. Possible models are discussed.
Freese Katherine
Gherghetta Tony
Umeda Hideyuki
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