Probing the Time Variation of a Fine Structure Constant Using Galaxy Clusters and the Quintessence Model
We explore a possible time variation of the fine structure constant (α ≡ e²/â„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 Y_(SZ)D²_A and its X-ray counterpar...
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ftcaltechauth:oai:authors.library.caltech.edu:6e7jj-6tc73 2024-10-13T14:10:51+00:00 Probing the Time Variation of a Fine Structure Constant Using Galaxy Clusters and the Quintessence Model Liu, Zhi-E Liu, Wen-Fei Zhang, Tong-Jie Zhai, Zhong-Xu Bora, Kamal 2021-11-20 https://doi.org/10.3847/1538-4357/ac2150 unknown American Astronomical Society https://arxiv.org/abs/2109.00134 eprintid:112204 info:eu-repo/semantics/openAccess Other Astrophysical Journal, 922(1), Art. No. 19, (2021-11-20) Quintessence Cosmological models Galaxy clusters Space and Planetary Science Astronomy and Astrophysics info:eu-repo/semantics/article 2021 ftcaltechauth https://doi.org/10.3847/1538-4357/ac2150 2024-09-25T18:46:44Z We explore a possible time variation of the fine structure constant (α ≡ e²/â„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 Y_(SZ)D²_A and its X-ray counterpart Y_X 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. Received 2021 June 18; revised 2021 August 22; accepted 2021 August 24; published 2021 November 16. We thank the anonymous referee for the helpful and constructive feedback. This work was supported by the National Key R & D Program of China (2017YFA0402600), the Natural Science Foundation of Shandong Province, China (Grant NO.ZR2019MA059), and the National Natural Science Foundation of China (grant No. 11929301). Z.Z. is supported in part by NASA grant 15-WFIRST15-0008, Cosmology with the High Latitude Survey Roman Science Investigation Team (SIT). K.B. acknowledges Department of Science and Technology, Government of India for providing the financial support under the DST-INSPIRE Fellowship program. Published - Liu_2021_ApJ_922_19.pdf Accepted Version - 2109.00134.pdf Article in Journal/Newspaper South pole Caltech Authors (California Institute of Technology) South Pole The Astrophysical Journal 922 1 19 |
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Caltech Authors (California Institute of Technology) |
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ftcaltechauth |
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unknown |
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Quintessence Cosmological models Galaxy clusters Space and Planetary Science Astronomy and Astrophysics |
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Quintessence Cosmological models Galaxy clusters Space and Planetary Science Astronomy and Astrophysics Liu, Zhi-E Liu, Wen-Fei Zhang, Tong-Jie Zhai, Zhong-Xu Bora, Kamal Probing the Time Variation of a Fine Structure Constant Using Galaxy Clusters and the Quintessence Model |
topic_facet |
Quintessence Cosmological models Galaxy clusters Space and Planetary Science Astronomy and Astrophysics |
description |
We explore a possible time variation of the fine structure constant (α ≡ e²/â„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 Y_(SZ)D²_A and its X-ray counterpart Y_X 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. Received 2021 June 18; revised 2021 August 22; accepted 2021 August 24; published 2021 November 16. We thank the anonymous referee for the helpful and constructive feedback. This work was supported by the National Key R & D Program of China (2017YFA0402600), the Natural Science Foundation of Shandong Province, China (Grant NO.ZR2019MA059), and the National Natural Science Foundation of China (grant No. 11929301). Z.Z. is supported in part by NASA grant 15-WFIRST15-0008, Cosmology with the High Latitude Survey Roman Science Investigation Team (SIT). K.B. acknowledges Department of Science and Technology, Government of India for providing the financial support under the DST-INSPIRE Fellowship program. Published - Liu_2021_ApJ_922_19.pdf Accepted Version - 2109.00134.pdf |
format |
Article in Journal/Newspaper |
author |
Liu, Zhi-E Liu, Wen-Fei Zhang, Tong-Jie Zhai, Zhong-Xu Bora, Kamal |
author_facet |
Liu, Zhi-E Liu, Wen-Fei Zhang, Tong-Jie Zhai, Zhong-Xu Bora, Kamal |
author_sort |
Liu, Zhi-E |
title |
Probing the Time Variation of a Fine Structure Constant Using Galaxy Clusters and the Quintessence Model |
title_short |
Probing the Time Variation of a Fine Structure Constant Using Galaxy Clusters and the Quintessence Model |
title_full |
Probing the Time Variation of a Fine Structure Constant Using Galaxy Clusters and the Quintessence Model |
title_fullStr |
Probing the Time Variation of a Fine Structure Constant Using Galaxy Clusters and the Quintessence Model |
title_full_unstemmed |
Probing the Time Variation of a Fine Structure Constant Using Galaxy Clusters and the Quintessence Model |
title_sort |
probing the time variation of a fine structure constant using galaxy clusters and the quintessence model |
publisher |
American Astronomical Society |
publishDate |
2021 |
url |
https://doi.org/10.3847/1538-4357/ac2150 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
Astrophysical Journal, 922(1), Art. No. 19, (2021-11-20) |
op_relation |
https://arxiv.org/abs/2109.00134 eprintid:112204 |
op_rights |
info:eu-repo/semantics/openAccess Other |
op_doi |
https://doi.org/10.3847/1538-4357/ac2150 |
container_title |
The Astrophysical Journal |
container_volume |
922 |
container_issue |
1 |
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19 |
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1812818378985832448 |