CPL effective dark energy from the backreaction effect
Fuente:
arXiv
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| Autori principali: | , |
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| Natura: | Preprint |
| Pubblicazione: |
2024
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| _version_ | 1866913401148538880 |
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| author | Yao, Yan-Hong Meng, Xin-He |
| author_facet | Yao, Yan-Hong Meng, Xin-He |
| contents | In this paper, we interpret the dark energy as an effect caused by small scale inhomogeneities of the universe with the use of the spatial averaged approach of Buchert. The model considered here adopts the Chevallier-Polarski-Linder(CPL) parameterizations of the equation of state of the effective perfect fluid from the backreaction effect. Thanks to the effective geometry introduced by Larena et. al.\cite{larena2009testing} in their previous work, we confront such backreaction model with latest type Ia supernova and Hubble parameter observations, coming out with results that reveal the difference between the Friedmann-Lema\^ıtre-Robertson-Walker model and backreaction model. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2406_15442 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | CPL effective dark energy from the backreaction effect Yao, Yan-Hong Meng, Xin-He Cosmology and Nongalactic Astrophysics In this paper, we interpret the dark energy as an effect caused by small scale inhomogeneities of the universe with the use of the spatial averaged approach of Buchert. The model considered here adopts the Chevallier-Polarski-Linder(CPL) parameterizations of the equation of state of the effective perfect fluid from the backreaction effect. Thanks to the effective geometry introduced by Larena et. al.\cite{larena2009testing} in their previous work, we confront such backreaction model with latest type Ia supernova and Hubble parameter observations, coming out with results that reveal the difference between the Friedmann-Lema\^ıtre-Robertson-Walker model and backreaction model. |
| title | CPL effective dark energy from the backreaction effect |
| topic | Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2406.15442 |