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Simple inflationary quintessential model. II. Power law potentials

Author
Haro, J.; Amoros, J.; Pan, S.
Type of activity
Journal article
Journal
Physical review D
Date of publication
2016-09-21
Volume
94
Number
6
DOI
https://doi.org/10.1103/PhysRevD.94.064060 Open in new window
Repository
http://hdl.handle.net/2117/95850 Open in new window
https://arxiv.org/abs/1607.06726 Open in new window
URL
http://journals.aps.org/prd/abstract/10.1103/PhysRevD.94.064060 Open in new window
Abstract
The present work is a sequel of our previous work [Phys. Rev. D 93, 084018 (2016)] which depicted a simple version of an inflationary quintessential model whose inflationary stage was described by a Higgs-type potential and the quintessential phase was responsible due to an exponential potential. Additionally, the model predicted a nonsingular universe in past which was geodesically past incomplete. Further, it was also found that the model is in agreement with the Planck 2013 data when running ...
Citation
Haro, J., Amoros, J., Pan, S. Simple inflationary quintessential model. II. Power law potentials. "Physical review D - Particles, fields, gravitation and cosmology", 21 Setembre 2016, vol. 94, núm. 6.
Group of research
EDP - Partial Differential Equations and Applications
GEOMVAP - Geometry of Manifolds and Applications

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