Significance of gyropotentials in metric theory of inertia
I.E. Bulyzhenkov

TL;DR
This paper explores the role of gyropotentials in the metric theory of inertia, suggesting they influence galactic rotation and orbital velocities, with implications for astrophysical phenomena and potential experimental verifications.
Contribution
It introduces the concept of gyropotentials within a metric framework, linking them to galactic dynamics and proposing new avenues for observational tests.
Findings
Gyropotentials affect orbital velocities in spiral galaxies.
Gyropotential creates centripetal gyroforces surpassing Newtonian attraction.
Potential verifications could be conducted in the Kuiper Belt and planetary rings.
Abstract
The constancy of orbital velocities of peripheral stars in a spiral galaxy points to a potential regime of co-rotation together with the interstellar densities of the galactic disk. The Einstein gyropotential rises to the evolutionary constant of a self-rotating metric profile, while the Newtonian potential falls radially. Gyropotential in vortex self-organizations creates centripetal gyroforces that prevail over Newtonian attraction of probe bodies at large distances from the axis of rotation. For practical verifications, the 1914 geodesic relations of Einstein predict the inverse distance velocities for retrograde stars. For the solar system, gyrometric corrections of Newtonian forces under transitions to the potential circulation in material vortexes can be sought in the Kuiper Belt, the peripheral rings of Saturn and high equatorial orbits around other planets.
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Taxonomy
TopicsAstro and Planetary Science · Geomagnetism and Paleomagnetism Studies · Stellar, planetary, and galactic studies
