Guardat en:
| Autor principal: | |
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| Format: | Recurso digital |
| Idioma: | anglès |
| Publicat: |
Zenodo
2026
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| Matèries: | |
| Accés en línia: | https://doi.org/10.5281/zenodo.18976333 |
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- <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>