Trapped Quintessential Inflation

@inproceedings{Snchez2006TrappedQI,
  title={Trapped Quintessential Inflation},
  author={J. C. Bueno S{\'a}nchez and Konstantinos Dimopoulos},
  year={2006}
}
Quintessential inflation is studied using a string modulus as the inflaton-quintessence field. The modulus begins its evolution at the steep part of its scalar potential, which is due to non-perturbative effects (e.g. gaugino condensation). It is assumed that the modulus crosses an enhanced symmetry point (ESP) in field space. Particle production at the ESP temporarily traps the modulus resulting in a brief period of inflation. More inflation follows, due to the flatness of the potential, since… 

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