Guardat en:
| Autor principal: | |
|---|---|
| Format: | Recurso digital |
| Idioma: | anglès |
| Publicat: |
Zenodo
2025
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| Matèries: | |
| Accés en línia: | https://doi.org/10.5281/zenodo.15499585 |
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- <p>This paper investigates the hypothesis of a preferred cosmological axis in light of several large-scale anomalies observed in the universe, including the hemispherical asymmetry in the CMB, the alignment of low-order multipoles, quasar polarization, and hints of chirality in cosmic signals. Within the framework of the Rotating Quantum Asymmetric Multiversal (RQAM) model, which posits that our universe emerged from a nonsingular quantum bounce inside a rotating black hole, a coherent physical axis is predicted to arise from inherited angular momentum and amplified through two quantum mechanisms: the Quantum Inertia Gradient (QIG) and the Quantum Vacuum Phase Shift (QVP). The paper explores observational consequences across multiple fronts—including CMB polarization cross-correlations (EB/TB), circular polarization in gravitational waves, and extragalactic alignments—proposes a mathematical parametrization of the axis, and outlines falsifiability paths through missions such as LiteBIRD, CMB-S4, LISA, and SKA.</p> <p><strong>This work has been timestamped and integrity-protected using a SHA-256 cryptographic hash and sealed into the Bitcoin blockchain, providing immutable proof of authorship and publication date, independently of institutional affiliation or platform.</strong></p>