This research explores how spectral dimension running resolves dark energy issues in early universe cosmology, indicating new physics.
This paper refines the 4D Bulk Inflation model by resolving the tension between predicted dark energy density and early-universe constraints (BBN/CMB). We propose that dark energy suppression in the early universe is a geometric consequence of spectral dimension running (ds), a robust result from multiple quantum gravity frameworks including CDT and Loop Quantum Gravity. In the Planckian era, where ds≈2, 4D bulk pressure is geometrically suppressed as it lacks a consolidated 3D volume to act upon. Dark energy "activates" not via a scalar potential, but as spacetime achieves its full 3D character. Key Contributions Geometric Suppression: Explains why dark energy was negligible at early times without fine-tuning. Hubble Tension Resolution: Maintains an equation of state w≈−0.827, consistent with DESI 2024. Testable Predictions: 1. CMB Low-l Anomaly: Predicts power suppression at large angular scales (l<10). 2. Variation of G: Predicts G˙/G≈1.1×10−12 yr−1, testable by next-gen Lunar Laser Ranging. 3. Dark Matter: Identifies dark matter as ultra-light Kaluza-Klein modes of the inflating 4D bulk AI Disclosure: Concept and physical reasoning by the author; mathematical formalism and LaTeX assisted by AI
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Anamaria Moritz (2026) studied this question.
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