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| Main Authors: | , , , , , |
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| Format: | Preprint |
| Published: |
2024
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2405.05798 |
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| _version_ | 1866929616230285312 |
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| author | Wang, Junchao Huang, Zhiqi Yao, Yanhong Liu, Jianqi Huang, Lu Su, Yan |
| author_facet | Wang, Junchao Huang, Zhiqi Yao, Yanhong Liu, Jianqi Huang, Lu Su, Yan |
| contents | The unified dark fluid model unifies dark matter and dark energy into a single component, providing an alternative and more concise framework for interpreting cosmological observations. We introduce a PAge-like Unified Dark Fluid (PUDF) model based on the PAge approximation (Huang 2020), which is parameterized by the age of the universe and an $η$ parameter indicating the deviation from Einstein-De Sitter Universe. The PUDF model shares many similar features of the standard Lambda cold dark matter ($Λ$CDM) model and can effectively describe the large-scale structure formation and late-time cosmic acceleration. We constrain the PUDF model with the Planck 2018 cosmic microwave background anisotropies, baryon acoustic oscillation measurements including those from the most recent DESI 2024, the Pantheon+ sample of Type Ia supernovae, and the Cosmic Chronometers compilation. Although the PUDF performs well in fitting all the cosmological datasets, the joint analysis of the data still favors the $Λ$CDM model over the PUDF model, according to the Bayesian evidence of model comparison. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2405_05798 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | A PAge-like Unified Dark Fluid Model Wang, Junchao Huang, Zhiqi Yao, Yanhong Liu, Jianqi Huang, Lu Su, Yan Cosmology and Nongalactic Astrophysics The unified dark fluid model unifies dark matter and dark energy into a single component, providing an alternative and more concise framework for interpreting cosmological observations. We introduce a PAge-like Unified Dark Fluid (PUDF) model based on the PAge approximation (Huang 2020), which is parameterized by the age of the universe and an $η$ parameter indicating the deviation from Einstein-De Sitter Universe. The PUDF model shares many similar features of the standard Lambda cold dark matter ($Λ$CDM) model and can effectively describe the large-scale structure formation and late-time cosmic acceleration. We constrain the PUDF model with the Planck 2018 cosmic microwave background anisotropies, baryon acoustic oscillation measurements including those from the most recent DESI 2024, the Pantheon+ sample of Type Ia supernovae, and the Cosmic Chronometers compilation. Although the PUDF performs well in fitting all the cosmological datasets, the joint analysis of the data still favors the $Λ$CDM model over the PUDF model, according to the Bayesian evidence of model comparison. |
| title | A PAge-like Unified Dark Fluid Model |
| topic | Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2405.05798 |