Get 20M+ Full-Text Papers For Less Than $1.50/day. Start a 7-Day Trial for You or Your Team.

Learn More →

Beyond the plane-parallel and Newtonian approach: wide-angle redshift distortions and convergence in general relativity

Beyond the plane-parallel and Newtonian approach: wide-angle redshift distortions and convergence... We extend previous analyses of wide-angle correlations in the galaxy power spectrum in redshift space to include all general relativistic effects. These general relativistic corrections to the standard approach become important on large scales and at high redshifts, and they lead to new terms in the wide-angle correlations. We show that in principle the new terms can produce corrections of nearly 10% on Gpc scales over the usual Newtonian approximation. General relativistic corrections will be important for future large-volume surveys such as SKA and Euclid, although the problem of cosmic variance will present a challenge in observing this. http://www.deepdyve.com/assets/images/DeepDyve-Logo-lg.png Journal of Cosmology and Astroparticle Physics IOP Publishing

Beyond the plane-parallel and Newtonian approach: wide-angle redshift distortions and convergence in general relativity

Loading next page...
 
/lp/iop-publishing/beyond-the-plane-parallel-and-newtonian-approach-wide-angle-redshift-Lm2p9BP7RK

References

References for this paper are not available at this time. We will be adding them shortly, thank you for your patience.

Copyright
Copyright © IOP Publishing Ltd
eISSN
1475-7516
DOI
10.1088/1475-7516/2012/10/025
Publisher site
See Article on Publisher Site

Abstract

We extend previous analyses of wide-angle correlations in the galaxy power spectrum in redshift space to include all general relativistic effects. These general relativistic corrections to the standard approach become important on large scales and at high redshifts, and they lead to new terms in the wide-angle correlations. We show that in principle the new terms can produce corrections of nearly 10% on Gpc scales over the usual Newtonian approximation. General relativistic corrections will be important for future large-volume surveys such as SKA and Euclid, although the problem of cosmic variance will present a challenge in observing this.

Journal

Journal of Cosmology and Astroparticle PhysicsIOP Publishing

Published: Oct 1, 2012

There are no references for this article.