A Black-Hole–Driven, Time-Dependent Origin of Dark Energy: Resolving the 2026 DESI and JWST Anomalies via Holographic Scaling.

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Authors: Brian Joseph Miller
Cited by: 0

Abstract

We propose a dynamical mechanism for dark energy where the observed cosmological constant (Lambda) arises from the cumulative volume of Planck-density phases within black hole cores. Utilizing a holographic scaling law (Vc ∝ M²), we derive an effective dark energy density that tracks the integrated mass function of supermassive black holes (SMBHs). This framework provides a physical resolution to the 10^120 magnitude discrepancy in vacuum energy. We demonstrate that our model predicts the "thawing" dark energy signatures identified in the January 2026 DESI and Euclid results, providing a formal resolution to the 3.5-sigma clustering gap and the early-universe black hole anomalies reported in the JWST "Little Red Dot" census.

Fields of Study & Subjects

Cosmology and Gravitation Theories Black Holes and Theoretical Physics Dark Matter and Cosmic Phenomena

Publication details

Journal / source
Zenodo (CERN European Organization for Nuclear Research)
Publication date
28 January 2026
Document type
Preprint