Dark energy from a scale-free distribution

We investigate some intriguing consequences of characterizing dark energy by the so-called scale-free statistics in a flat Friedman-Robertson-Walker cosmology. We adopt a toy model, derived from a power law distribution, being P(k)∼k− γ, with 2<γ< 3, showing as a result that the dynamics mimic...

Full description

Saved in:
Bibliographic Details
Published inEurophysics letters Vol. 94; no. 4; pp. 49002 - 49007
Main Authors Iannone, G, Luongo, O
Format Journal Article
LanguageEnglish
Published IOP Publishing 01.05.2011
EPS, SIF, EDP Sciences and IOP Publishing
Subjects
Online AccessGet full text

Cover

Loading…