Saved in:
| Main Author: | |
|---|---|
| Format: | Recurso digital |
| Language: | |
| Published: |
Zenodo
2026
|
| Online Access: | https://doi.org/10.5281/zenodo.19447492 |
| Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
| _version_ | 1866901222814908416 |
|---|---|
| author | ghosh, Pranab |
| author_facet | ghosh, Pranab |
| contents | <p>We present a refined formulation of the Wave-3 framework in which spacetime is modeled as an emergent medium exhibiting fluctuation-driven corrections to a $\Lambda$CDM background. The model is restricted to phenomenologically supported components and formulated within an effective field theory (EFT) approach. A fluctuation tensor field with nonlinear self-interactions is introduced and coupled to the energy–momentum tensor, allowing external fields to influence the emergent structure of spacetime.</p> <p>Numerical simulations demonstrate that while uniform background fields produce weak, non-scaling corrections, spatially structured fields induce statistically significant and scale-dependent deviations from a red-noise spectrum. A sub-linear scaling relation of the form $|\Delta P| \propto \gamma^{0.41}$ is observed, indicating a nonlinear but stable response of the system. These results suggest that the structure of background fields, rather than their magnitude alone, plays a central role in generating large-scale correlations within an emergent spacetime medium.</p> <p>The framework remains consistent with General Relativity in the weak-fluctuation limit and is interpreted as an effective theory valid below a cutoff scale. No claim of a complete quantum gravity theory is made; instead, the model provides a testable phenomenological approach for exploring fluctuation-driven deviations from standard cosmological behavior.</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_19447492 |
| institution | Zenodo |
| language | |
| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | "Wave-3 Framework (Refined): Emergent Spacetime Fluctuations and Structured Field Coupling" ghosh, Pranab <p>We present a refined formulation of the Wave-3 framework in which spacetime is modeled as an emergent medium exhibiting fluctuation-driven corrections to a $\Lambda$CDM background. The model is restricted to phenomenologically supported components and formulated within an effective field theory (EFT) approach. A fluctuation tensor field with nonlinear self-interactions is introduced and coupled to the energy–momentum tensor, allowing external fields to influence the emergent structure of spacetime.</p> <p>Numerical simulations demonstrate that while uniform background fields produce weak, non-scaling corrections, spatially structured fields induce statistically significant and scale-dependent deviations from a red-noise spectrum. A sub-linear scaling relation of the form $|\Delta P| \propto \gamma^{0.41}$ is observed, indicating a nonlinear but stable response of the system. These results suggest that the structure of background fields, rather than their magnitude alone, plays a central role in generating large-scale correlations within an emergent spacetime medium.</p> <p>The framework remains consistent with General Relativity in the weak-fluctuation limit and is interpreted as an effective theory valid below a cutoff scale. No claim of a complete quantum gravity theory is made; instead, the model provides a testable phenomenological approach for exploring fluctuation-driven deviations from standard cosmological behavior.</p> |
| title | "Wave-3 Framework (Refined): Emergent Spacetime Fluctuations and Structured Field Coupling" |
| url | https://doi.org/10.5281/zenodo.19447492 |