Dark Energy as Magnetic Curvature: Resolving Cosmological Anomalies and the Vacuum Catastrophe
The discovery of cosmic acceleration introduced dark energy as the dominant component of the Universe, described in ΛCDM as a uniform vacuum energy with negative pressure. This picture has been remarkably successful in fitting Type Ia supernovae, baryon acoustic oscillations (BAO), and the cosmic microwave background (CMB), but it remains conceptually unsatisfying: the cosmological constant problem, the coincidence problem, and late-time tensions in structure growth and Hubble flows reveal cracks in the standard view.
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2025-10-01
- DOI
- https://doi.org/10.5281/zenodo.17240985
- Primary Topic
- Conservation, Biodiversity, and Resource Management
- Type
- article
- Field-Weighted Citation Impact
- 0.00