Abstract
Brane inflationary universe model in the context of a Chaplygin gas equation of state is studied. General conditions for this model to be realizable are discussed. In the high-energy limit and by using a chaotic potential we describe in great details the characteristic of this model. The parameters of the model are restricted by using recent astronomical observations.
Original language | English |
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Pages (from-to) | 149-153 |
Number of pages | 5 |
Journal | Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics |
Volume | 664 |
Issue number | 3 |
DOIs | |
State | Published - 19 Jun 2008 |
Externally published | Yes |