Topological Defects and Inflation

Details Topological Defects and Inflation Topological Defects and Inflation

1995-10-11

arxiv.org/abs/hep-ph/9510275v1

Phys.Lett.B372:20-24,1996

Physics

High Energy Physics

High Energy Physics - Phenomenology

11 pages, LaTEX

Scientific paper

10.1016/0370-2693(96)00136-0

In the context of supersymmetric models, we analyze the production of topological defects at the end of inflation driven by a conjugate pair of inflaton fields which are non-singlets under the continuous symmetry group of the theory. We find that magnetic monopoles of mass on the order of $10^{13}\ GeV$ can survive inflation and be present in our galaxy at an observable level. We also consider cosmic strings as well as domain walls.

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