On the width of the last scattering surface

Details On the width of the last scattering surface On the width of the last scattering surface

2004-11-24

arxiv.org/abs/astro-ph/0411657v1

Int.J.Mod.Phys. D13 (2004) 1425-1429

Astronomy and Astrophysics

Astrophysics

10 pages, 1 figure, 2 tables, accepted to IJMPD

Scientific paper

10.1142/S0218271804005638

We discuss the physical effects of some accelerated world models on the width of the last scattering surface (LSS) of the cosmic microwave background radiation (CMBR). The models considered in our analysis are X-matter (XCDM) and a Chaplygin type gas. The redshift of the LSS does not depend on the kind of dark energy (if XCDM of Chaplygin). Further, for a Chaplygin gas, the width of the LSS is also only weakly dependent on the kind of scenario (if we have dark energy plus cold dark matter or the unified picture).

Affiliated with

Also associated with

No associations

Rating

On the width of the last scattering surface 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 On the width of the last scattering surface, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the width of the last scattering surface will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-576539