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Direction Dependence of the Deceleration Parameter

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arxiv 1109.0941 v6 pith:HANSWA4I submitted 2011-09-05 astro-ph.CO hep-ph

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

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Cited by 2 Pith papers

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    astro-ph.CO 2025-10 conditional novelty 6.0 of 10

    Off-center observers in a spherical LTB overdensity get accurate cosmographic distances up to δc≈2.5 near the structure, while linear perturbation theory is better beyond ~3Rs; a gauge dictionary links the two.

  2. Redshift Dependence of $H_0$ Dipole in Pantheon+ Supernovae

    astro-ph.CO 2026-08 conditional novelty 4.0 of 10

    A dipole in the locally measured Hubble constant appears at 2-3 sigma in the lowest-redshift Pantheon+ supernova bins, points near the Shapley supercluster and CMB dipole, and disappears for higher redshift thresholds.

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