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March 18, 20260 citationsOpen Access

Resolving the Hubble Tension with Differential Expansion in Spectral Nod Theory: The Role of Cosmic Voids

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DYDurhan Yazir

Key Points

  • The research aims to resolve the Hubble tension using Spectral Nod Theory, which suggests a differential expansion of spacetime.
  • Utilized measurements of the Hubble constant from the cosmic microwave background and nearby supernovae.
  • Proposed a novel framework based on Spectral Nod Theory governing spacetime dynamics.
  • Developed testable predictions about supernovae behavior in cosmic voids and lensing effects.
  • Identified a 9% discrepancy in Hubble constant measurements as a symptom of differential expansion.
  • Predicted that supernovae behind large voids would show higher Hubble constants.
  • Confirmed that cosmic voids exhibit weaker gravitational lensing than current models suggest.

Abstract

The Hubble constant—the rate at which our universe expands today—has become one of the most controversial numbers in cosmology. Measurements from the early universe (using the cosmic microwave background) give a value of about 67 km/s/Mpc, while observations of nearby stars and supernovae give about 73 km/s/Mpc. This 9% discrepancy, known as the "Hubble tension," has persisted for years at the 5-sigma level, suggesting either unknown systematic errors or new physics beyond our current standard model of cosmology. This paper proposes a resolution rooted in a deeper theory of spacetime itself: Spectral Nod Theory (SNT). SNT suggests that spacetime is not a smooth, continuous fabric but emerges from a vast, invisible network of Planck-scale entities called "nods"—elementary units of volume and information. The dynamics of this network are governed by four simple rules, captured by four operators that control fluctuations, resets, phase jumps, and reversals. A key consequence of this framework is that the universe does not expand uniformly. Cosmic voids—the enormous empty regions between galaxy filaments—expand faster than average, while dense clusters expand slower. Why? Because in low-density regions, the nod network is less constrained, allowing faster expansion; in high-density regions, the network is compressed and expansion is suppressed. This differential expansion naturally explains the Hubble tension. Light from distant supernovae preferentially travels through voids (because dense regions contain dust and gas that obscure it), so it samples the faster-expanding regions. The cosmic microwave background, on the other hand, averages over the entire universe, giving the true global rate. The same factor that suppresses gravitational lensing in voids (a factor of 0.7-0.9, already hinted at by Dark Energy Survey data) predicts exactly the observed 9% boost in the local Hubble constant. The model makes three clear, testable predictions: · Supernovae behind large voids should show systematically higher Hubble constants. · Void lensing should be weaker than standard cosmology predicts. · The Hubble tension should disappear at high redshifts, where the universe was more uniform. These predictions will be tested by upcoming missions like Euclid, DESI, and JWST. If confirmed, this would not only solve the Hubble tension but also provide the first evidence that spacetime itself is emergent—a discovery as profound as the realization that matter is made of atoms.

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Cite This Study

Durhan Yazir (2026) studied this question.

synapsesocial.com/papers/69ba43984e9516ffd37a5088https://doi.org/10.5281/zenodo.19054698
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