Running Einstein Constant and a Possible Vacuum State of the Universe
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arXiv
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| Auteurs principaux: | , , , |
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| Format: | Preprint |
| Publié: |
2024
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| _version_ | 1866918131426918400 |
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| author | Montani, Giovanni Maniccia, Giulia Fazzari, Elisa Melchiorri, Alessandro |
| author_facet | Montani, Giovanni Maniccia, Giulia Fazzari, Elisa Melchiorri, Alessandro |
| contents | We propose a revised formulation of General Relativity for cosmological settings, in which the Einstein constant varies with the energy density of the Universe. We demonstrate that this modification has only phenomenological impact of providing an effective dark energy density expression. Assuming a state close to vacuum, here defined by the vanishing product of the Einstein coupling constant and the Universe's energy density, we perform a Taylor expansion of the theory and hence extend it to the whole domain. In this framework, the (renormalized) vacuum energy problem is studied, and an additional constant pressure term, which induces a Chaplygin-like contribution to the dark energy sector, arises in the late-time dynamics. The correction to the late-time Hubble parameter is investigated by comparing theoretical predictions with the late Universe observational data. Our findings indicate that the current value of the stated vacuum energy is consistent with zero within 1$σ$. Implications of the modified $Λ$CDM model with respect to the Hubble tension are also discussed. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2412_14747 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | Running Einstein Constant and a Possible Vacuum State of the Universe Montani, Giovanni Maniccia, Giulia Fazzari, Elisa Melchiorri, Alessandro General Relativity and Quantum Cosmology Cosmology and Nongalactic Astrophysics We propose a revised formulation of General Relativity for cosmological settings, in which the Einstein constant varies with the energy density of the Universe. We demonstrate that this modification has only phenomenological impact of providing an effective dark energy density expression. Assuming a state close to vacuum, here defined by the vanishing product of the Einstein coupling constant and the Universe's energy density, we perform a Taylor expansion of the theory and hence extend it to the whole domain. In this framework, the (renormalized) vacuum energy problem is studied, and an additional constant pressure term, which induces a Chaplygin-like contribution to the dark energy sector, arises in the late-time dynamics. The correction to the late-time Hubble parameter is investigated by comparing theoretical predictions with the late Universe observational data. Our findings indicate that the current value of the stated vacuum energy is consistent with zero within 1$σ$. Implications of the modified $Λ$CDM model with respect to the Hubble tension are also discussed. |
| title | Running Einstein Constant and a Possible Vacuum State of the Universe |
| topic | General Relativity and Quantum Cosmology Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2412.14747 |