The Hubble Tension Through the Lens of GCST Global Complexity–Stability Theory as a Framework for Resolving the Discrepancy in the Cosmic Expansion Rate
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| Format: | Recurso digital |
| Langue: | anglais |
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2026
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| _version_ | 1866901064454766592 |
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| author | Lukin, Roman |
| author_facet | Lukin, Roman |
| contents | <p>Abstract <br> <br>The Hubble Tension — a ~5–6σ discrepancy between local measurements of the Hubble constant H₀ ≈ 73–74 km/s/Mpc (Cepheids + Type Ia supernovae) and early-universe inferences H₀ ≈ 67–68 km/s/Mpc (Planck CMB + ΛCDM) — remains unresolved. <br> <br>Global Complexity–Stability Theory (GCST) interprets the tension as a late-time structural debt effect in cosmic expansion. The stability index <br> <br>declines in the late universe as complexity C grows faster than global dissipation γ. Accumulated debt D forces accelerated expansion locally, producing higher effective H₀ compared to early-time (CMB) values. <br> <br>This paper formalizes the link between structural debt D and the energy-momentum tensor T_{\mu\nu} in Einstein’s equations, showing that D acts as an effective additional source term contributing to the observed late-time acceleration. </p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_18976333 |
| institution | Zenodo |
| language | eng |
| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | The Hubble Tension Through the Lens of GCST Global Complexity–Stability Theory as a Framework for Resolving the Discrepancy in the Cosmic Expansion Rate Lukin, Roman GCST Hubble Tension, structural debt cosmic expansion, Rate-Induced Transition dark energy, complexity theory Hubble constant, <p>Abstract <br> <br>The Hubble Tension — a ~5–6σ discrepancy between local measurements of the Hubble constant H₀ ≈ 73–74 km/s/Mpc (Cepheids + Type Ia supernovae) and early-universe inferences H₀ ≈ 67–68 km/s/Mpc (Planck CMB + ΛCDM) — remains unresolved. <br> <br>Global Complexity–Stability Theory (GCST) interprets the tension as a late-time structural debt effect in cosmic expansion. The stability index <br> <br>declines in the late universe as complexity C grows faster than global dissipation γ. Accumulated debt D forces accelerated expansion locally, producing higher effective H₀ compared to early-time (CMB) values. <br> <br>This paper formalizes the link between structural debt D and the energy-momentum tensor T_{\mu\nu} in Einstein’s equations, showing that D acts as an effective additional source term contributing to the observed late-time acceleration. </p> |
| title | The Hubble Tension Through the Lens of GCST Global Complexity–Stability Theory as a Framework for Resolving the Discrepancy in the Cosmic Expansion Rate |
| topic | GCST Hubble Tension, structural debt cosmic expansion, Rate-Induced Transition dark energy, complexity theory Hubble constant, |
| url | https://doi.org/10.5281/zenodo.18976333 |