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Regular PapersNo Access

COSMOLOGICAL DISTANCE MEASURE CONSTRAINTS ON THE DECELERATION PARAMETER

Institute of Theoretical Physics, School of Physics & Optoelectronic Technology, Dalian University of Technology, Dalian 116024, P. R. China

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Institute of Theoretical Physics, School of Physics & Optoelectronic Technology, Dalian University of Technology, Dalian 116024, P. R. China

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Department of Astronomy, Nanjing University, Nanjing 210093, P. R. China

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https://doi.org/10.1142/S0218271809015163Cited by:2 (Source: Crossref)

Abstract

Constraints on a parametrized deceleration parameter, q(a) = q₀ + q₁(1 - a), are investigated using cosmological observations of type Ia supernovae (SN Ia), baryon acoustic oscillations (BAOs) and cosmic microwave background (CMB) and observational Hubble data (OHD) which correspond to the cosmological distance measure. When a high redshift dataset of CMB is added in the SN + BAO + OHD case, a stronger constraint is obtained than for the lower redshift case, SN + BAO + OHD. The evolutions of the deceleration and Hubble parameters with respect to redshift z are reconstructed from cosmic observations. With cosmic observations as constraints, it is found that a smaller current deceleration parameter and a larger transition redshift are obtained in the SN + BAO + OHD case than in the SN + BAO + OHD + CMB case. In the SN + BAO + OHD + CMB case, slightly larger Hubble parameter values will be obtained than in the SN + BAO + OHD case.

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PACS: 98.80.-k, 98.80.Es

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Vol. 18, No. 09

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Received 28 December 2008

Revised 23 March 2009

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