Geodesic motion in Euclidean Schwarzschild geometry
Emmanuele Battista, Giampiero Esposito
Abstract
This paper performs a systematic investigation of geodesic motion in Euclidean Schwarzschild geometry, which is studied in the equatorial plane. The explicit form of geodesic motion is obtained in terms of incomplete elliptic integrals of first, second and third kind. No elliptic-like orbits exist in Euclidean Schwarzschild geometry, unlike the corresponding Lorentzian pattern. Among unbounded orbits, only unbounded first-kind orbits are allowed, unlike general relativity where unbounded second-kind orbits are always allowed.
Topics & Concepts
Schwarzschild radiusGeodesicMotion (physics)Non-Euclidean geometryEuclidean geometryAbsolute geometrySchwarzschild geodesicsGeometrySchwarzschild metricGeodesic mapMathematicsPlane (geometry)PhysicsSolving the geodesic equationsClassical mechanicsGeneral relativityMathematical analysisKerr metricGravitationConvex setConvex optimizationRegular polygonBlack Holes and Theoretical PhysicsCosmology and Gravitation TheoriesRelativity and Gravitational Theory