Constraints on reconstructed dark energy model from SN Ia and BAO/CMB observations

The European Physical Journal C

Sudipta Das¹  Kazuharu Bamba²  Abdulla Al Mamon³ 

[1] Department of Physics, Visva-Bharati, 731235, Santiniketan, India;Division of Human Support System, Faculty of Symbiotic Systems Science, Fukushima University, 960-1296, Fukushima, Japan;Manipal Centre for Natural Sciences, Manipal University, 576104, Manipal, India;Department of Physics, Visva-Bharati, 731235, Santiniketan, India;

关键词: Dark Energy;    Scalar Field;    Cosmic Microwave Background;    Deceleration Parameter;    Dark Energy Model;   

DOI  :  10.1140/epjc/s10052-016-4590-y

来源: Springer

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