Fluctuations of the luminosity distance
Astrophysics
2011-11-22 v5 General Relativity and Quantum Cosmology
Abstract
We derive an expression for the luminosity distance in a perturbed Friedmann universe. We define the correlation function and the power spectrum of the luminosity distance fluctuations and express them in terms of the initial spectrum of the Bardeen potential. We present semi-analytical results for the case of a pure CDM universe. We argue that the luminosity distance power spectrum represents a new observational tool which can be used to determine cosmological parameters. In addition, our results shed some light into the debate whether second order small scale fluctuations can mimic an accelerating universe.
Keywords
Cite
@article{arxiv.astro-ph/0511183,
title = {Fluctuations of the luminosity distance},
author = {Camille Bonvin and Ruth Durrer and M. Alice Gasparini},
journal= {arXiv preprint arXiv:astro-ph/0511183},
year = {2011}
}
Comments
23 pages, 15 figures, errors in published version corrected (eqs. (53), (55), (58) and (59))