Void and Density Walls Inhomogeneous Cosmic Web And Dark Energy
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arXiv
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| Format: | Preprint |
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2025
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| _version_ | 1866915214980546560 |
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| author | Moffat, John W. |
| author_facet | Moffat, John W. |
| contents | Recent observations from the Dark Energy Spectroscopic Instrument (DESI 2025) indicate a weakening of cosmic acceleration at low redshifts $z < 1$, with effective dark energy equation of state parameters $w_0 > -1$ and $w_a < 0$. We demonstrate that this evolution in dark energy can be explained by cosmic inhomogeneities and the Cosmic Web without modifying fundamental physics. Our model shows how the differential expansion between underdense voids and overdense walls creates an effective backreaction term that simulates evolving dark energy when interpreted within homogeneous cosmological frameworks. The inhomogeneous cosmic structure formation becomes significant $z\sim 1-2$, the increasing gravitational influence of wall regions counteracting the cosmic acceleration, producing both a weakening acceleration signal and a direction-dependent Hubble parameter consistent with local measurements. This mechanism reconciles the higher locally measured Hubble constant $H_0\approx 73~ km/s/Mpc$ with the lower value inferred from CMB observations $H_0\approx 67-69~ km/s/Mpc$ without introducing new energy components or modifying general relativity. Our model makes testable predictions regarding directional and scale-dependent variations in cosmological parameters that can be verified with next-generation surveys. This work suggests that properly accounting for cosmic structure may be essential for resolving apparent tensions in cosmological parameters. |
| format | Preprint |
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arxiv_https___arxiv_org_abs_2503_20912 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Void and Density Walls Inhomogeneous Cosmic Web And Dark Energy Moffat, John W. Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology Recent observations from the Dark Energy Spectroscopic Instrument (DESI 2025) indicate a weakening of cosmic acceleration at low redshifts $z < 1$, with effective dark energy equation of state parameters $w_0 > -1$ and $w_a < 0$. We demonstrate that this evolution in dark energy can be explained by cosmic inhomogeneities and the Cosmic Web without modifying fundamental physics. Our model shows how the differential expansion between underdense voids and overdense walls creates an effective backreaction term that simulates evolving dark energy when interpreted within homogeneous cosmological frameworks. The inhomogeneous cosmic structure formation becomes significant $z\sim 1-2$, the increasing gravitational influence of wall regions counteracting the cosmic acceleration, producing both a weakening acceleration signal and a direction-dependent Hubble parameter consistent with local measurements. This mechanism reconciles the higher locally measured Hubble constant $H_0\approx 73~ km/s/Mpc$ with the lower value inferred from CMB observations $H_0\approx 67-69~ km/s/Mpc$ without introducing new energy components or modifying general relativity. Our model makes testable predictions regarding directional and scale-dependent variations in cosmological parameters that can be verified with next-generation surveys. This work suggests that properly accounting for cosmic structure may be essential for resolving apparent tensions in cosmological parameters. |
| title | Void and Density Walls Inhomogeneous Cosmic Web And Dark Energy |
| topic | Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology |
| url | https://arxiv.org/abs/2503.20912 |