On the trajectories of null and timelike geodesics in different wormhole geometries
arXiv:1710.06791 · doi:10.1140/epjc/s10052-018-5854-5
Abstract
The paper deals with an extensive study of null and timelike geodesics in the background of wormhole geometries. Starting with a spherically symmetric spacetime, null geodesics are analyzed for the Morris-Thorne wormhole(WH) and photon spheres are examined in WH geometries. Both bounded and unbounded orbits are discussed for timelike geodesics. A similar analysis has been done for trajectories in a dynamic spherically symmetric WH and for a rotating WH. Finally, the invariant angle method of Rindler and Ishak has been used to calculate the angle between radial and tangential vectors at any point on the photon's trajectory.
19 pages, 10 figures
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- Dynamics in wormhole spacetimes: a Jacobi metric approach
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- Static spherically symmetric wormhole with quadratic shape function and particle trajectories around it
- Particle motion around traversable wormholes: Possibility of closed timelike geodesics
- Bound orbits near black holes with scalar hair