Ashtekar-Wheeler-DeWitt Equation and Inflationary Scenario

Details Ashtekar-Wheeler-DeWitt Equation and Inflationary Scenario Ashtekar-Wheeler-DeWitt Equation and Inflationary Scenario

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.2307s&link_type=abstract

The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio

Physics

Scientific paper

Ashtekar-Wheeler-DeWitt Equation for quantized coupled gravitational and scalar fields is considered, together with its expansion in terms of a dimensionless parameter which is the ratio of the "typical" total potential energy density to the Planck energy density. Conditions favourable to the inflationary scenario are derived, and the correspondence between inflationary states and perturbations of the exact Chern-Simons State for quantum gravity in 4-dimensions are discussed. If certain conditions are satisfied, the Ashtekar-Wheeler-DeWitt equation reduces to a Schrodinger Equation which describes quantized scalar field which evolves with respect to a Schwinger-Tomonaga time which increases with the volume of the universe in an inflationary universe with approximate de Sitter metric.

Affiliated with

Also associated with

No associations

Rating

Ashtekar-Wheeler-DeWitt Equation and Inflationary Scenario 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 Ashtekar-Wheeler-DeWitt Equation and Inflationary Scenario, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Ashtekar-Wheeler-DeWitt Equation and Inflationary Scenario will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1841606