Submitted:
12 September 2025
Posted:
12 September 2025
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Abstract
Keywords:
1. Introduction
2. Theoretical Framework
2.1. Multiverse and Anisotropic Boundary Conditions
2.2. Fermion Generations from Anisotropic Excitations
2.3. Neutrino Oscillations As Geometric Interference
2.4. Jwst Anomalies and Multiverse Glimpses
3. Implications and Predictions
3.1. Static Predictions
3.2. Temporal Evolution of Stiffness Axes and a Second Bounce Scenario
3.3. Gamma-Ray Decay and Anisotropic Energy Dissipation
4. Conclusions
- It provides a physical foundation for the three-generation structure of leptons, offering a mechanistic cause for their mass hierarchy and decay patterns, rather than treating them as arbitrary parameters of the Standard Model.
- It investigates the critical role of boundary conditions in a Big Bounce scenario, exploring its potential non-uniqueness across time and space within a larger hyper-universe.
- It proposes a second, complementary rebound trigger based on multiverse-induced phase transitions, alongside the exotic matter collapse mechanism previously suggested.
- This novel and complementary bounce scenario could eliminate the need for a primordial hyper-inflation epoch. This occurs only if the matter-instability phase transition is triggered while the universe is still sufficiently contracted. In this case, the subsequent re-creation of matter (baryogenesis) would occur within a hot, dense, and finite volume, naturally yielding a homogeneous and flat universe without requiring a separate inflationary phase. Conversely, if this transition occurred in a highly dilated universe, the result would be a cold, radiated and matter-empty space that would rapidly dissipate its energy into adjacent domains, leading to a cosmological dead-end. This conditional outcome underscores the critical link between the multiverse dynamics, the contraction phase, and viable cosmology.
Author’s Note
References
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