A Method and Apparatus for Cosmic Ray Origin Analysis Based on Non-Conventional Spacetime Structures Including Retrocausal Analysis of Ultra-High-Energy Cosmic Rays such as the "Amaterasu Particle"
Abstract
This paper proposes a non-conventional spacetime framework to explain the GZK paradox and missing-source problem in UHECR origin studies. It introduces (1) a retrocausal signal model correlating observed arrival directions with future singularity distributions, and (2) a higher-dimensional leakage model with an energy barrier. Applied to the 244 EeV “Amaterasu particle,” the approach yields statistically significant consistency beyond nearby-universe models.
Fields of Study & Subjects
Astrophysics and Cosmic Phenomena
Noncommutative and Quantum Gravity Theories
Gamma-ray bursts and supernovae
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 25 February 2026
- Language
- EN
- Document type
- Thesis