Abstract
In this work we study closed inflationary universe models by using a tachyonic field theory. We determine and characterize the existence of an inflationary universe with Ω > 1. We found that these models are less restrictive compared to the standard ones with a scalar field. We use recent astronomical observations to constraint the parameters appearing in the model.
Original language | English |
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Article number | 012010 |
Journal | Journal of Physics: Conference Series |
Volume | 134 |
DOIs | |
State | Published - 2008 |