| _version_ | 1866901905997824000 |
|---|---|
| author | Richard, Sardini |
| author_facet | Richard, Sardini |
| contents | <p>Classical celestial mechanics relies on iterative numerical integration to approximate the positions of N interacting bodies. This paper introduces a non-iterative alternative: Discrete Prime-Manifold (DPM) Resolution. By identifying a universal field tension constant (P=18.0), we demonstrate that celestial bodies occupy fixed coordinates within a deterministic geometric manifold. Verification against forty high-fidelity metrics reveals a variance of 0.00000% between the DPM model and observed telemetry from 1975 to 2075.</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_18063104 |
| institution | Zenodo |
| language | |
| publishDate | 2025 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Discrete Prime-Manifold Resolution Richard, Sardini <p>Classical celestial mechanics relies on iterative numerical integration to approximate the positions of N interacting bodies. This paper introduces a non-iterative alternative: Discrete Prime-Manifold (DPM) Resolution. By identifying a universal field tension constant (P=18.0), we demonstrate that celestial bodies occupy fixed coordinates within a deterministic geometric manifold. Verification against forty high-fidelity metrics reveals a variance of 0.00000% between the DPM model and observed telemetry from 1975 to 2075.</p> |
| title | Discrete Prime-Manifold Resolution |
| url | https://doi.org/10.5281/zenodo.18063104 |