English

A Simple Quintessence Model

Astrophysics 2008-09-11 v1

Abstract

A simple model of quintessential inflation with the modified exponential potential eαϕ[A+(ϕϕ0)2]e^{-\alpha \phi} [A+(\phi-\phi_0)^2] is analyzed in the braneworld context. Considering reheating via instant preheating, we conclude that the model exhibits transient acceleration at late times for 0.96Aα21.260.96 \lesssim A \alpha^2 \lesssim 1.26 and 271ϕ0α273271 \lesssim \phi_0 \alpha \lesssim 273, while permanent acceleration is obtained for 2.3×108Aα20.982.3\times10^{-8} \lesssim A \alpha^2 \lesssim 0.98 and 255ϕ0α273255 \lesssim \phi_0 \alpha \lesssim 273. The steep parameter α\alpha is constrained to be in the range 5.3α10.85.3 \lesssim \alpha \lesssim 10.8.

Cite

@article{arxiv.0809.1679,
  title  = {A Simple Quintessence Model},
  author = {M. C. Bento and R. Gonzalez Felipe and N. M. C. Santos},
  journal= {arXiv preprint arXiv:0809.1679},
  year   = {2008}
}

Comments

4 pages, 2 figures, presented at the "seventh alexander friedmann international seminar on gravitation and cosmology"

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