PaperPanorama

arXiv:1109.0941·v6·Cosmology and Nongalactic Astrophysics

Direction Dependence of the Deceleration Parameter

Ronggen Cai🇨🇳 · Zhongliang Tuo🇨🇳

PDFarXivINSPIREDOI

Abstract

In this paper we study the possibly existing anisotropy in the acceleration expansion by use of the full sample of Union2 data. Using the hemisphere comparison method to search for a preferred direction, we take the deceleration parameter q0 as the diagnostic to quantify the anisotropy level in the wCDM model. We find that the maximum accelerating expansion direction is ,with the maximum anisotropy level of , and that the anisotropy is more prominent when only low redshift data () are used. We also discuss this issue in the parameterized model, showing a similar result.

Comments: 6 pages, 2 tables,1 figure. arXiv admin note: text overlap with arXiv:1007.4347

Citation historyopen in Citation History ↗