Observational constraints on dark energy model

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

10 pages, 9 figures, update refererences, use ws-ijmpd style, use new supernova data and add model independent analysis. The u

Scientific paper

10.1142/S0218271805006080

The recent observations support that our universe is flat and expanding with acceleration. A quintessence model with a general relation between the quintessence potential and the quintessence kinetic energy was proposed to explain the phenomenon. The dark energy potential includes both the hyperbolic and the double exponential potentials. We analyze this model in detail by using the recent supernova and the first year Wilkinson Microwave Anisotropy Probe (WMAP) observations. For a flat universe dominated by a dark energy with constant $\omega$ which is a special case of the general model, we find that $\Omega_{\rm m0}=0.30^{+0.06}_{-0.08}$ and $\omega_{\rm Q}\le -0.82$, and the turnaround redshift $z_{\rm T}$ when the universe switched from the deceleration phase to the acceleration phase is $z_{\rm T}=0.65$. For the general model, we find that $\Omega_{\rm m0}\sim 0.3$, $\omega_{\rm Q0}\sim -1.0$, $\beta\sim 0.5$ and $z_{\rm T}\sim 0.67$. A model independent polynomial parameterization is also considered, the best fit model gives $\Omega_{\rm m0}=0.40\pm 0.14$, $\omega_{\rm Q0}=-1.4$ and $z_{\rm T}=0.37$.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Observational constraints on dark energy model does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Observational constraints on dark energy model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observational constraints on dark energy model will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-372645

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.