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Reconstruction of symmetric teleparallel gravity with energy conditions
International Journal of Geometric Methods in Modern Physics ( IF 2.1 ) Pub Date : 2024-05-15 , DOI: 10.1142/s0219887824502049
Irfan Mahmood 1 , Hira Sohail 2 , Allah Ditta 1 , S. H. Shekh 3 , Anil Kumar Yadav 4
Affiliation  

This research investigates the impact of modified gravity on cosmic scales, focusing on f(Q) cosmology. By applying energy conditions, the study reconstructs various f(Q) models, considering an accelerating Universe, quintessence, and a cosmological constant Λ. Using up-to-date observational data, including the Supernova Pantheon sample and cosmic chronometer data, Hubble constants H0 are estimated as 70.370.92+0.84 km/s/Mpc (from H(z) data) and 70.020.25+0.44 km/s/Mpc (from pantheon compilation of SN Ia data). The matter energy density parameter (Ω0m) is calculated as 0.260.0100.015 (OHD) and 0.270.0140.025 (SN Ia). Furthermore, as a function of red-shift z, explicit expressions of f(Q) and the EOS parameter ω are produced, and their graphical analysis describes the late time acceleration of the Universe without the usage of dark energy.



中文翻译:


用能量条件重建对称远平行引力



这项研究研究了修正引力对宇宙尺度的影响,重点是 f(Q) 宇宙学。通过应用能量条件,该研究重建了各种 f(Q) 模型,考虑了加速宇宙、本质和宇宙常数 Λ 。使用最新的观测数据,包括超新星万神殿样本和宇宙天文钟数据,哈勃常数 H0 估计为 70.370.92+0.84 km/s/Mpc(来自 H(z) km/s/Mpc(来自 SN Ia 数据的万神殿编译)。物质能量密度参数( Ω0m )计算为 0.260.0100.015 (OHD)和 0.270.0140.025 (SN Ia)。此外,作为红移 z 的函数,生成了 f(Q) 和 EOS 参数 ω 的显式表达式,并且它们的图形分析描述了后期加速不使用暗能量的宇宙。

更新日期:2024-05-15
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