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On the trajectories of null and timelike geodesics in different wormhole geometries

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arxiv 1710.06791 v2 pith:NVY5RWKO submitted 2017-10-17 gr-qc

classification gr-qc
keywords geodesicsgeometriesnulltimelikewormholeanglebeenphoton
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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.

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  1. Bound orbits near scalar field naked singularities

    gr-qc 2019-08 conditional novelty 6.0 of 10

    In scalar field naked singularities the lapse function has a global minimum, creating a stable static orbit for zero-angular-momentum particles that can mimic a black hole shadow, and nearby bound orbits precess backwards.

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