Observational constraints on the jerk parameter with the data of the Hubble parameter

被引:79
作者
Al Mamon, Abdulla [1 ]
Bamba, Kazuharu [2 ]
机构
[1] Jadavpur Univ, Dept Math, Kolkata 700032, India
[2] Fukushima Univ, Fac Symbiot Syst Sci, Div Human Support Syst, Fukushima 9601296, Japan
来源
EUROPEAN PHYSICAL JOURNAL C | 2018年 / 78卷 / 10期
关键词
BARYON ACOUSTIC-OSCILLATION; MODIFIED GRAVITY; PAST DECELERATION; SNE IA; DARK; SUPERNOVAE; LAMBDA; STATEFINDER; INFLATION; COSMOLOGY;
D O I
10.1140/epjc/s10052-018-6355-2
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We study the accelerated expansion phase of the universe by using the kinematic approach. In particular, the deceleration parameter q is parametrized in a model-independent way. Considering a generalized parametrization for q, we first obtain the jerk parameter j (a dimensionless third time derivative of the scale factor) and then confront it with cosmic observations. We use the latest observational dataset of the Hubble parameter H(z) consisting of 41 data points in the redshift range of 0.07 <= z <= 2.36, larger than the redshift range that covered by the Type Ia supernova. We also acquire the current values of the deceleration parameter q(0), jerk parameter j(0) and transition redshift z(t) (at which the expansion of the universe switches from being decelerated to accelerated) with la errors (68.3% confidence level). As a result, it is demonstrate that the universe is indeed undergoing an accelerated expansion phase following the decelerated one. This is consistent with the present observations. Moreover, we find the departure for the present model from the standard ACDM model according to the evolution of j. Furthermore, the evolution of the normalized Hubble parameter is shown for the present model and it is compared with the dataset of H(z).
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页数:8
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