English

Direction Dependence of the Deceleration Parameter

Cosmology and Nongalactic Astrophysics 2012-09-26 v6 High Energy Physics - Phenomenology

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 (l,b)=(314+2013,28+1133)(l,b)=(314_{+20^{\circ}}^{\circ-13^{\circ}},28_{+11^{\circ}}^{\circ-33^{\circ}}),with the maximum anisotropy level of δq0,max/qˉ0=0.79+0.270.28\delta q_{0,max}/\bar{q}_0=0.79_{+0.27}^{-0.28}, and that the anisotropy is more prominent when only low redshift data (z0.2z\leq0.2) are used. We also discuss this issue in the CPLCPL parameterized model, showing a similar result.

Cite

@article{arxiv.1109.0941,
  title  = {Direction Dependence of the Deceleration Parameter},
  author = {Ronggen Cai and Zhongliang Tuo},
  journal= {arXiv preprint arXiv:1109.0941},
  year   = {2012}
}

Comments

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

R2 v1 2026-06-21T18:59:56.631Z