Quintessence Model With Double Exponential Potential

Details Quintessence Model With Double Exponential Potential Quintessence Model With Double Exponential Potential

2001-11-25

arxiv.org/abs/gr-qc/0111082v2

Phys.Lett. B532 (2002) 159-165

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

6 pages, Revtex Style, four eps figures,some new comments are added regarding the fitting analysis. Conclusion has been rewrit

Scientific paper

10.1016/S0370-2693(02)01547-2

We have reinvestigated the quintessence model with minimally coupled scalar field in the context of recent Supernova observation at $z=1.7$. By assuming the form of the scale factor which gives both the early time deceleration and late time acceleration, consistent with the observations, we show that one needs a double exponential potential. We have also shown that the equation of state and the behaviour of dark energy density are reasonably consistent with earlier constraints obtained by different authors. This work shows again the importance of double exponential potential for a quintessence field.

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