Cosmology with non-linear scalar field

Details Cosmology with non-linear scalar field Cosmology with non-linear scalar field

May 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010ap%26ss.327..117z&link_type=abstract

Astrophysics and Space Science, Volume 327, Issue 1, pp.117-124

Astronomy and Astrophysics

Astrophysics

Dark Energy, Non-Linear Scalar Field, Quintessence, Square Potential

Scientific paper

Mukhanov and Vikman have studied inflation model with the non-linear (NL) scalar field. We discuss the dark energy model with the Lagrangian in the presence of the square potential. We analyse the sufficient condition for the existence of an attractor solution, and compare the equation of state parameter, the present age of universe and the transition redshift with the quintessence model. We also use the Gold dataset of 157 SN-Ia to finally constrain the parameter of the models. We find that the considered model is consistent with the observation and a little inferior to the quintessence model. The above Lagrangian is similar to the non-linear Born-Infeld (NLBI) scalar field model, while which is superior to the quintessence model.

Affiliated with

Also associated with

No associations

Rating

Cosmology with non-linear scalar field 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 Cosmology with non-linear scalar field, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmology with non-linear scalar field will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1892620