Preferred Cosmological Direction and Anisotropies within the RQAM Framework
Fuente:
Zenodo
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Recurso digital |
| Sprache: | Englisch |
| Veröffentlicht: |
Zenodo
2025
|
| Schlagworte: | |
| Online-Zugang: | |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| _version_ | 1866901833462579200 |
|---|---|
| author | Viso Cervera, Miguel |
| author_facet | Viso Cervera, Miguel |
| contents | <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> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_15499585 |
| institution | Zenodo |
| language | eng |
| publishDate | 2025 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Preferred Cosmological Direction and Anisotropies within the RQAM Framework Viso Cervera, Miguel Preferred cosmological axis cosmic microwave background (CMB) large-scale anisotropies circular polarization gravitational waves EB/TB cross-correlations quasar alignment cosmological chirality inherited rotation quantum bounce torsion cosmology RQAM model falsifiability <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> |
| title | Preferred Cosmological Direction and Anisotropies within the RQAM Framework |
| topic | Preferred cosmological axis cosmic microwave background (CMB) large-scale anisotropies circular polarization gravitational waves EB/TB cross-correlations quasar alignment cosmological chirality inherited rotation quantum bounce torsion cosmology RQAM model falsifiability |
| url | https://doi.org/10.5281/zenodo.15499585 |