What question did this study set out to answer?

This research aims to develop the Void-Amplified Dimensional Flow (VADF) model to explain variations in spacetime dimensionality influenced by curvature.

March 4, 2026Open Access

Void-Amplified Dimensional Flow (VADF): Curvature-Suppressed Anomalous Dimension and Emergent Phenomena(v4.1)

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Authors

VHVladyslav Hruznov G(Grok (xAI)

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Overview

This model proposes a mechanism altering spacetime dimensionality in cosmic voids, suggesting implications for gravity and cosmology.

Key Points

This research aims to develop the Void-Amplified Dimensional Flow (VADF) model to explain variations in spacetime dimensionality influenced by curvature.
Introduce a curvature-suppressed anomalous dimension η(R) derived from competition between the Seeley–deWitt coefficient and bi-metric splitting.
Analyze spectral dimension ds(R) across different curvature regimes.
Explore implications for physical phenomena like Casimir enhancement, fractional tunneling, and cosmic signatures.
Demonstrates ds ≈ 4 in dense regions and ds ≈ 4.06–4.20 in cosmic voids.
Finds potential enhancements in Hubble parameters indicating a 5–7% boost and effects on void lensing of ∆κ/κ ≈ 0.18–0.25.
Addresses Hubble tension and mild S8 tension with no introduction of new fields.

Cite This Study

Hruznov et al. (2026) studied this question.

synapsesocial.com/papers/69a7cd1dd48f933b5eed920e https://doi.org/10.5281/zenodo.18833457

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March 4, 2026Open Access

Void-Amplified Dimensional Flow (VADF): Curvature-Suppressed Anomalous Dimension and Emergent Phenomena(v4.1)

View Full Paper

Ask AI

Bookmark

Authors

VHVladyslav Hruznov G(Grok (xAI)

Discussion

Member takes

Overview

This model proposes a mechanism altering spacetime dimensionality in cosmic voids, suggesting implications for gravity and cosmology.

Key Points

This research aims to develop the Void-Amplified Dimensional Flow (VADF) model to explain variations in spacetime dimensionality influenced by curvature.
Introduce a curvature-suppressed anomalous dimension η(R) derived from competition between the Seeley–deWitt coefficient and bi-metric splitting.
Analyze spectral dimension ds(R) across different curvature regimes.
Explore implications for physical phenomena like Casimir enhancement, fractional tunneling, and cosmic signatures.
Demonstrates ds ≈ 4 in dense regions and ds ≈ 4.06–4.20 in cosmic voids.
Finds potential enhancements in Hubble parameters indicating a 5–7% boost and effects on void lensing of ∆κ/κ ≈ 0.18–0.25.
Addresses Hubble tension and mild S8 tension with no introduction of new fields.

Cite This Study

Hruznov et al. (2026) studied this question.

synapsesocial.com/papers/69a7cd1dd48f933b5eed920e https://doi.org/10.5281/zenodo.18833457

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