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