Closed-form analytical solutions for timelike geodesics in Damour-Solodukhin wormhole spacetimes are obtained via elliptic integrals, with special cases for throat-root degeneracies and homoclinic orbits.
Motion of spinning particles in the Kerr-Newman black hole exterior. I. Periodic orbits,
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Four relativistic spinning particle models (vector oscillator, spinor oscillator, spherical top, massive twistor) describe identical physics in free and interacting theories within the spin-magnitude-preserving sector.
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Analytical solutions for timelike orbits around Damour-Solodukhin wormholes
Closed-form analytical solutions for timelike geodesics in Damour-Solodukhin wormhole spacetimes are obtained via elliptic integrals, with special cases for throat-root degeneracies and homoclinic orbits.
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Universality in Relativistic Spinning Particle Models
Four relativistic spinning particle models (vector oscillator, spinor oscillator, spherical top, massive twistor) describe identical physics in free and interacting theories within the spin-magnitude-preserving sector.