Motion of massive particles around a charged Weyl black hole and the geodetic precession of orbiting gyroscopes
arXiv:2009.03399 · doi:10.1140/epjc/s10052-020-7945-3
Abstract
The advanced state of cosmological observations constantly tests the alternative theories of gravity that originate from Einstein's theory. However, this is not restricted to modifications to general relativity. In this sense, we work in the context of Weyl's theory, more specifically, on a particular black hole solution for a charged massive source, which is confronted with the classical test of the geodetic precession, to obtain information about the parameters associated with this theory. To fully assess this spacetime, the complete geodesic structure for massive test particles is presented.
22 pages, 15 figures
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- Conformal Weyl gravity via two stages of quasinormal ringing and late-time behavior
- Gravitational Rutherford scattering of electrically charged particles from a charged Weyl black hole
- Ergosphere, photon region structure, and the shadow of a rotating charged Weyl black hole
- Geodetic precession and shadow of quantum extended black holes
- Orbits of particles with magnetic dipole moment around magnetized Schwarzschild black holes: Applications to S2 star orbit
- A Critical Assessment of Black Hole Solutions With a Linear Term in Their Redshift Function
- Chaotic dynamics of string around the conformal black hole
- Analytical study of particle geodesics around a scale-dependent de Sitter black hole
- Null geodesics around a black hole with weakly coupled global monopole charge
- The role of elliptic integrals in calculating the gravitational lensing of a charged Weyl black hole surrounded by plasma