Gorde:
| Egile nagusia: | |
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| Formatua: | Recurso digital |
| Hizkuntza: | |
| Argitaratua: |
Zenodo
2025
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| Gaiak: | |
| Sarrera elektronikoa: | https://doi.org/10.5281/zenodo.17975232 |
| Etiketak: |
Etiketa erantsi
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Aurkibidea:
- <p>In the course of developing the framework of Quaternion Angular–Momentum<br>Gravity (QAMG), we have arrived at a geometric structure centered on global<br>angular–momentum neutrality (GAN) and an antisymmetric two–form field Bµν.<br>This structure is designed to complement the curvature–only description of gravity<br>in General Relativity by providing an independent and consistent geometric carrier<br>for rotation, vorticity, and angular–momentum transport. GAN is not introduced<br>as an ad hoc constraint; rather, it emerges as a global consistency principle re<br>quired by angular–momentum conservation, cosmological boundary conditions, and<br>the statistical isotropy of large–scale structure.<br>The central contribution of this work is to clarify the logical relation between<br>local angular–momentum flux conservation, global closure, and the structure of the<br>solution space. We show that the rotational flux current Jµ<br>rot induced by the two<br>form sector satisfies a covariant local continuity equation, implying a radially invari<br>ant integrated flux. However, local conservation alone is insufficient to fix the global<br>angular–momentum zero mode. The GAN condition acts as a global closure rela<br>tion that removes this continuous zero–mode freedom and decomposes the classical<br>solution space into mutually disconnected flux sectors. Under physically admissible<br>conditions of regularity, boundary behavior, and global neutrality, no continuous<br>classical deformation exists between solutions with different asymptotic flux. This<br>result is established explicitly in the form of a no–go theorem.<br>Onthis basis, we identify the geometric origin of so–called “macroscopic angular<br>momentum quantization”. The resulting discreteness does not rely on microscopic<br>quantum postulates. Instead, it follows from the interplay of (i) the topological<br>and flux–sector structure of the two–form gauge field, (ii) global closure enforced<br>by GAN, and (iii) regularity and boundary conditions. If neighboring flux sectors<br>are separated by a finite on–shell action difference, an emergent macroscopic con<br>stant ℏQ can be defined, which characterizes the minimal action increment between<br>distinct classical geometric sectors.<br>The physical consequences of this structure are consistent across scales. In<br>the weak–field regime, propagation of the two–form field produces Yukawa–type<br>corrections with a characteristic range of order ∼ 10kpc, providing a geometric ex<br>planation of spiral–galaxy rotation curves without invoking dark matter halos. In<br>the strong–field regime, the interplay of rotational flux and global neutrality natu<br>rally favors angular–momentum–dominated compact structures. In a cosmological setting,GAN is compatible with FLRW symmetry: it introduces no additional back<br>ground degrees of freedom whilee nforcing vanishing total rotational flux on spatial<br>hypersurfaces.<br>In summary, global angular–momentum neutrality andt wo–form geometry form<br>a coherent, structurally constrained, and testable core of the QAMG framework. By<br>extending gravitational geometry beyond curvature to include rotation and global<br>closure, this framework provides a new geometric starting point for connecting cosmic acceleration, galactic structure, and the potential unification of macroscopic<br>and microscopic descriptions of angular momentum.</p>