Strong spin-gravity coupling in the linear approximation for circular orbits in Schwarzschild’s field
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Overview
Analytical calculations reveal conditions for ultrarelativistic spinning particles in circular orbits around massive bodies, suggesting implications for gravitational interactions.
Key Points
Circular orbits are analyzed for ultrarelativistic spinning particles in Schwarzschild’s field, indicating specific conditions for their admissibility.
Direct analytical calculations provide necessary and sufficient conditions for the existence of such orbits.
The method involves solutions of the Mathisson-Papapetrou equations within the linear spin approximation focused on non-equatorial scenarios.
Insights into spin-gravity force are presented, highlighting its role in maintaining ultrarelativistic circular orbits.