Abstract
Brane inflationary universe model in the context of logamediate inflation is studied. As the energy density we consider two different fields, first a standard scalar field, and then a tachyon field. In the high-energy limit we describes the conditions for theses models. The parameters of our models are constrained from the observational data.
Original language | English |
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Article number | 1250101 |
Journal | Modern Physics Letters A |
Volume | 27 |
Issue number | 18 |
DOIs | |
State | Published - 14 Jun 2012 |
Keywords
- Inflation