Distance-Redshift in Inhomogeneous FLRW

Details Distance-Redshift in Inhomogeneous FLRW Distance-Redshift in Inhomogeneous FLRW

2000-02-16

arxiv.org/abs/astro-ph/0002334v2

Astronomy and Astrophysics

Astrophysics

22 pages, 3 figures

Scientific paper

We give distance--redshift relations in terms of elliptic integrals for three different mass distributions of the Friedmann-Lema\^\i tre-Robertson-Walker (FLRW) cosmology. These models are dynamically pressure free FLRW on large scales but, due to mass inhomogeneities, differ in their optical properties. They are the filled-beam model (standard FLRW), the empty-beam model (no mass density exists in the observing beams) and the 2/3 filled-beam model. For special $\OM$-- $\OL$ values the elliptic integrals reduce to more familiar functions. These new expressions for distance-redshift significantly reduce computer evaluation times.

Affiliated with

Also associated with

No associations

Rating

Distance-Redshift in Inhomogeneous FLRW 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 in Inhomogeneous FLRW, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Distance-Redshift in Inhomogeneous FLRW will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-312269