Distance-redshift relation in an isotropic inhomogeneous universe: Spherically symmertic dust-shell universe

Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

latex, 18 pages, 10 figures. Accepted for publication in Physical Review D

Scientific paper

10.1103/PhysRevD.58.103504

The relation between angular diameter distance and redshift in a spherically symmetric dust-shell universe is studied. This model has large inhomogeneities of matter distribution on small scales. We have discovered that the relation agrees with that of an appropriate Friedmann-Lemaitre(FL) model if we set a ``homogeneous'' expansion law and a ``homogeneous'' averaged density field. This will support the averaging hypothesis that a universe looks like a FL model in spite of small-scale fluctuations of density field, if its averaged density field is homogeneous on large scales.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Distance-redshift relation in an isotropic inhomogeneous universe: Spherically symmertic dust-shell universe 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 Distance-redshift relation in an isotropic inhomogeneous universe: Spherically symmertic dust-shell universe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Distance-redshift relation in an isotropic inhomogeneous universe: Spherically symmertic dust-shell universe will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-347672

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.