CBR Anisotropy in an Open Inflation, CDM Cosmogony

Details CBR Anisotropy in an Open Inflation, CDM Cosmogony CBR Anisotropy in an Open Inflation, CDM Cosmogony

1994-06-27

arxiv.org/abs/astro-ph/9406069v1

Astrophys.J. 434 (1994) L1-L4

Astronomy and Astrophysics

Astrophysics

(12 pages, plain TeX; 3 figures available upon request from the authors), IASSNS-HEP-94/39, PUPT-1470, POP-568, CfPA-TH-94-27,

Scientific paper

10.1086/187558

We compute the cosmic background radiation anisotropy, produced by
energy-density fluctuations generated during an early epoch of inflation, in an
open cosmological model based on the cold dark matter scenario. At $\Omega_0
\sim$ 0.3 -- 0.4, the COBE normalized open model appears to be consistent with
most observations.

Affiliated with

Also associated with

No associations

Rating

CBR Anisotropy in an Open Inflation, CDM Cosmogony 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 CBR Anisotropy in an Open Inflation, CDM Cosmogony, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and CBR Anisotropy in an Open Inflation, CDM Cosmogony will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-231338