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| Format: | Recurso digital |
| Language: | English |
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2026
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| Online Access: | https://doi.org/10.5281/zenodo.19005284 |
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| _version_ | 1866901964148703232 |
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| author | Suffers, Craig |
| author_facet | Suffers, Craig |
| contents | <p> </p> <p>This has been replaced by https://doi.org/10.5281/zenodo.20335233</p> <p>This paper extends the information–geometry cosmology developed in earlier work by providing a natural, falsifiable explanation for dark energy and the ∼9% early–late Hubble discrepancy. In this framework, a collapsing black hole that reaches the Planck–limit surface (Ξ = 1) nucleates a child FRW universe. A fraction of the parent black hole’s information appears as warm dark matter (WDM), while a residual fraction manifests as an inherited vacuum–energy term.</p> <p>We show that this inherited vacuum energy relaxes slowly over cosmic time, producing a small epoch‑dependent deviation from a constant Λ and naturally generating the observed Hubble tension without modifying general relativity. Two mechanisms are proposed:</p> <ol> <li><strong>One‑off relaxation:</strong> a fixed vacuum‑energy offset inherited at nucleation that decays with timescale τ ≈ 8–12 Gyr.</li> <li><strong>Accretion‑driven leakage:</strong> ongoing information inflow into the parent black hole drives a steady, tap‑like leakage of vacuum energy into the child universe through the Planck‑boundary rupture.</li> </ol> <p>Using the warm‑dark‑matter mass scale (m_WDM ≈ 2–4 keV) and the local halo density of Andromeda, we obtain a local number density of <strong>~1.1×10¹¹ WDM particles per cubic metre</strong>, providing a direct observational anchor for the inherited information density. Combining this with the inherited‑information budget (I_child ≈ 10⁸⁷ bits) and the parent black hole capacity (I_BH ≈ 10⁹³ bits for M_BH ≈ 10⁸ M_⊙), we show that only a minute fraction of the parent manifold’s information is required to generate both warm dark matter and the observed dark‑energy behaviour.</p> <p>The model is fully falsifiable, requires no exotic fields, and offers a unified information‑geometric origin for warm dark matter, dark energy, and the Hubble tension.</p> <p> </p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_19005284 |
| institution | Zenodo |
| language | eng |
| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Dark Energy as Vacuum-Energy Continuity Across a Planck-Boundary Black Hole Suffers, Craig Information geometry Planck-limit surface Black Hole Cosmology Universe nucleation Warm dark matter Vacuum-Energy continuity Dark Energy Hubble Tension Parent-Child Universe Models Information Inheritance Berkenstein-Hawking Entropy Accretion-Driven leakage Cosmological relaxation timescale FRW cosmology small-scale structure formation Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena <p> </p> <p>This has been replaced by https://doi.org/10.5281/zenodo.20335233</p> <p>This paper extends the information–geometry cosmology developed in earlier work by providing a natural, falsifiable explanation for dark energy and the ∼9% early–late Hubble discrepancy. In this framework, a collapsing black hole that reaches the Planck–limit surface (Ξ = 1) nucleates a child FRW universe. A fraction of the parent black hole’s information appears as warm dark matter (WDM), while a residual fraction manifests as an inherited vacuum–energy term.</p> <p>We show that this inherited vacuum energy relaxes slowly over cosmic time, producing a small epoch‑dependent deviation from a constant Λ and naturally generating the observed Hubble tension without modifying general relativity. Two mechanisms are proposed:</p> <ol> <li><strong>One‑off relaxation:</strong> a fixed vacuum‑energy offset inherited at nucleation that decays with timescale τ ≈ 8–12 Gyr.</li> <li><strong>Accretion‑driven leakage:</strong> ongoing information inflow into the parent black hole drives a steady, tap‑like leakage of vacuum energy into the child universe through the Planck‑boundary rupture.</li> </ol> <p>Using the warm‑dark‑matter mass scale (m_WDM ≈ 2–4 keV) and the local halo density of Andromeda, we obtain a local number density of <strong>~1.1×10¹¹ WDM particles per cubic metre</strong>, providing a direct observational anchor for the inherited information density. Combining this with the inherited‑information budget (I_child ≈ 10⁸⁷ bits) and the parent black hole capacity (I_BH ≈ 10⁹³ bits for M_BH ≈ 10⁸ M_⊙), we show that only a minute fraction of the parent manifold’s information is required to generate both warm dark matter and the observed dark‑energy behaviour.</p> <p>The model is fully falsifiable, requires no exotic fields, and offers a unified information‑geometric origin for warm dark matter, dark energy, and the Hubble tension.</p> <p> </p> |
| title | Dark Energy as Vacuum-Energy Continuity Across a Planck-Boundary Black Hole |
| topic | Information geometry Planck-limit surface Black Hole Cosmology Universe nucleation Warm dark matter Vacuum-Energy continuity Dark Energy Hubble Tension Parent-Child Universe Models Information Inheritance Berkenstein-Hawking Entropy Accretion-Driven leakage Cosmological relaxation timescale FRW cosmology small-scale structure formation Cosmology and Nongalactic Astrophysics General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena |
| url | https://doi.org/10.5281/zenodo.19005284 |