Probing the Time Variation of a Fine Structure Constant Using Galaxy Clusters and the Quintessence Model
Liu, Zhi-E and Liu, Wen-Fei and Zhang, Tong-Jie and Zhai, Zhong-Xu and Bora, Kamal (2021) Probing the Time Variation of a Fine Structure Constant Using Galaxy Clusters and the Quintessence Model. The Astrophysical Journal, 922 (1). p. 19. ISSN 0004-637X
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Abstract
We explore a possible time variation of the fine structure constant (α ≡ e2/ℏ c) using the Sunyaev-Zel'dovich effect measurements of galaxy clusters along with their X-ray observations. Specifically, the ratio of the integrated Comptonization parameter YSZ DA2 and its X-ray counterpart YX is used as an observable to constrain the bounds on the variation of α. Considering the violation of the cosmic distance duality relation, this ratio depends on the fine structure constant of ∼ α3. We use the quintessence model to provide the origin of α time variation. In order to give a robust test on α variation, two galaxy cluster samples, the 61 clusters provided by the Planck collaboration and the 58 clusters detected by the South Pole Telescope (SPT), are collected for analysis. Their X-ray observations are given by the XMM-Newton survey. Our results give ζ =-0.203-0.099+0.101 for the Planck sample and ζ =-0.043-0.148+0.165 for the SPT sample, indicating that α is constant with redshift within 3σ and 1σ for the two samples, respectively. © 2021. The American Astronomical Society. All rights reserved.
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Item Type: | Article | ||
Uncontrolled Keywords: | Time Variation,Galaxy Clusters,Quintessence Model | ||
Subjects: | Physics | ||
Divisions: | Department of Physics | ||
Depositing User: | . LibTrainee 2021 | ||
Date Deposited: | 17 Sep 2022 09:24 | ||
Last Modified: | 17 Sep 2022 09:24 | ||
URI: | http://raiithold.iith.ac.in/id/eprint/10614 | ||
Publisher URL: | http://doi.org/10.3847/1538-4357/ac2150 | ||
OA policy: | https://v2.sherpa.ac.uk/id/publication/6401 | ||
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