Absolute medium Flowline Formation Law and Galaxy Spins: A Comparative Analysis with ΛCDM
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2026
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| _version_ | 1866901964359467008 |
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| author | BARUA, SREEMAN |
| author_facet | BARUA, SREEMAN |
| contents | <p><span lang="EN-US"><span>We derive a general formation law—AM Flow-Line Formation Law (AFFL)—stating that seeding, clustering, and bound-system formation (from star-forming cores to solar-system-like structures) occur preferentially along local Absolute-Medium (AM) flow-lines and are exponentially suppressed for cross- or counter-flow. The derivation integrates the Scale-Dependent Rigidity (NLEP) and Static–Dynamic Duality (SDDP) postulates, yields a local alignment–drag equation, a variational (action-like) </span><span>functional</span><span>, and a macroscopic rate law that encodes a </span><span>cross-flow</span><span> quench. We summarize falsifiable predictions across galactic filaments, spiral arms, and circumstellar disks, and outline a simulation–observation pipeline to measure AM stiffness and coherence from spatial clustering and age gradients aligned with AM streams.</span></span><span> </span></p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_18837279 |
| institution | Zenodo |
| language | |
| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Absolute medium Flowline Formation Law and Galaxy Spins: A Comparative Analysis with ΛCDM BARUA, SREEMAN <p><span lang="EN-US"><span>We derive a general formation law—AM Flow-Line Formation Law (AFFL)—stating that seeding, clustering, and bound-system formation (from star-forming cores to solar-system-like structures) occur preferentially along local Absolute-Medium (AM) flow-lines and are exponentially suppressed for cross- or counter-flow. The derivation integrates the Scale-Dependent Rigidity (NLEP) and Static–Dynamic Duality (SDDP) postulates, yields a local alignment–drag equation, a variational (action-like) </span><span>functional</span><span>, and a macroscopic rate law that encodes a </span><span>cross-flow</span><span> quench. We summarize falsifiable predictions across galactic filaments, spiral arms, and circumstellar disks, and outline a simulation–observation pipeline to measure AM stiffness and coherence from spatial clustering and age gradients aligned with AM streams.</span></span><span> </span></p> |
| title | Absolute medium Flowline Formation Law and Galaxy Spins: A Comparative Analysis with ΛCDM |
| url | https://doi.org/10.5281/zenodo.18837279 |