Observations in a Super--Horizon-Scale Inhomogeneous Cosmological Model

Details Observations in a Super--Horizon-Scale Inhomogeneous Cosmological Model Observations in a Super--Horizon-Scale Inhomogeneous Cosmological Model

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995apj...451....1t&link_type=abstract

Astrophysical Journal v.451, p.1

Astronomy and Astrophysics

Astronomy

24

Cosmology: Large-Scale Structure Of Universe, Cosmology: Theory

Scientific paper

Observational relations are derived in an inhomogeneous cosmological model consisting of three regions: the inner low-density homogeneous region, the self-similar inhomogeneous region, and the outer, nearly flat homogeneous region. The boundary between the inner region and the self-similar region is assumed to be in a spherical shell corresponding to the epoch of redshift z = 1.5-2.0, when the numbers of quasars and Lyα clouds changed rapidly. The observational significance of the comparatively large matter density in the self-similar region is discussed in connection with various cosmological observations such as the angular diameter, the number density per unit redshift, and the number count of galaxies.

Affiliated with

Also associated with

No associations

Rating

Observations in a Super--Horizon-Scale Inhomogeneous Cosmological Model 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 Observations in a Super--Horizon-Scale Inhomogeneous Cosmological Model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observations in a Super--Horizon-Scale Inhomogeneous Cosmological Model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-824751