Isotherms clustering in cosmic microwave background

Details Isotherms clustering in cosmic microwave background Isotherms clustering in cosmic microwave background

2006-07-17

arxiv.org/abs/astro-ph/0607370v2

Phys.Lett. A360 (2006) 210-216

Astronomy and Astrophysics

Astrophysics

Scientific paper

10.1016/j.physleta.2006.08.026

Since the strong clustering of luminous matter in the observable universe is a consequence of an initial non-uniformity of the baryon-photon fluid in the last scattering surface, an investigation of clustering of the isotherms in the cosmic microwave background has been performed. The isotherms clustering has been related to the baryon-photon fluid dynamics and the Taylor-microscale Reynolds number of this motion is estimated to be $10^2$. 3-year WMAP cosmic microwave background map has been used in this investigation.

Affiliated with

Also associated with

No associations

Rating

Isotherms clustering in cosmic microwave background 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 Isotherms clustering in cosmic microwave background, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Isotherms clustering in cosmic microwave background will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-507060