Abstract
The object of study is the geodesic structure of a \(z=2\) Lifshitz black hole in 3+1 space–time dimensions, which is an exact solution to the Einstein-scalar-Maxwell theory. The motion of massless and massive particles in this background is researched using the standard Lagrangian procedure. Analytical expressions are obtained for radial and angular motions of the test particles, where the polar trajectories are given in terms of the \(\wp \)-Weierstraß elliptic function. It will be demonstrated that an external observer can see that photons with radial motion arrive at spatial infinity in a finite coordinate time. For particles with non-vanished angular momentum, the motion is studied on the invariant plane \(\phi = \pi /2\) and, it is shown that bounded orbits are not allowed for this space–time on this plane. These results are consistent with other recent studies on Lifshitz black holes.
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Acknowledgments
The authors would like to thank F. Ercolí, M. Curé and referees for their comments and suggestions that helped us improve this paper. This work was funded by the Comisión Nacional de Investigación Científica y Tecnológica through FONDECYT Grants 11121148 (YV, FM) and 11130695 (JRV), and also partially funded by the Dirección de Investigación, Universidad de La Frontera (FM). MO would also like to thank PUCV and Instituto de Física y Astronomía (UV) and JRV wishes to thank to the UFRO for their hospitality.
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Olivares, M., Vásquez, Y., Villanueva, J.R. et al. Motion of particles on a \(z=2\) Lifshitz black hole background in 3\(+\)1 dimensions. Celest Mech Dyn Astr 119, 207–217 (2014). https://doi.org/10.1007/s10569-014-9555-6
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DOI: https://doi.org/10.1007/s10569-014-9555-6