Dark Energy Stars and the Cosmic Microwave Background

Details Dark Energy Stars and the Cosmic Microwave Background Dark Energy Stars and the Cosmic Microwave Background

2010-04-03

arxiv.org/abs/1004.0406v2

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

9 pages

Scientific paper

An initial state for the observable universe consisting of a finite region with a large vacuum energy will break-up due to near horizon quantum critical fluctuations. This will lead to a Friedmann-like early universe consisting of an expanding cloud of dark energy stars and radiation. In this note we point out that this scenario provides a simple explanation for the present day density of dark matter as well as the level of CMB temperature flucuations. It is also predicted that all dark matter will be clumped on mass scales ~ 10E3 solar masses.

Affiliated with

Also associated with

No associations

Rating

Dark Energy Stars and the 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 Dark Energy Stars and the Cosmic Microwave Background, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dark Energy Stars and the Cosmic Microwave Background will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-198487