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Primordial inflation with spontaneous symmetry breaking
In versions of the inflationary universe scenario where the universe has a chaotic beginning or starts from a bubble nucleation event it may be possible to relax some of the fine tuning of parameters that is usually required. Two models of this kind are presented here and compared with a supersymmet...
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Published in: | Physics letters. B 1985-01, Vol.154 (2), p.120-124 |
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Main Author: | |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | In versions of the inflationary universe scenario where the universe has a chaotic beginning or starts from a bubble nucleation event it may be possible to relax some of the fine tuning of parameters that is usually required. Two models of this kind are presented here and compared with a supersymmetric model. These new models require modifications to the usual treatment of density fluctuations. |
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ISSN: | 0370-2693 1873-2445 |
DOI: | 10.1016/0370-2693(85)90570-2 |