1989
DOI: 10.1016/0375-9601(89)90344-7
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Lyapunov stability of motion in Ernst space-time

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Cited by 3 publications
(4 citation statements)
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“…(47) the minimum radius for timelike circular orbit is same as null circular motion given in Eq. (29). The above values of energy E and the angular momentum are suitable for a circular orbit hence, the solution of φ is obtained by solving the following:…”
Section: Timelike Geodesics Of Sebh( = 1)mentioning
confidence: 99%
See 1 more Smart Citation
“…(47) the minimum radius for timelike circular orbit is same as null circular motion given in Eq. (29). The above values of energy E and the angular momentum are suitable for a circular orbit hence, the solution of φ is obtained by solving the following:…”
Section: Timelike Geodesics Of Sebh( = 1)mentioning
confidence: 99%
“…The case of orbits around a BH immersed in an external electric field has unfortunately received less attention than its magnetic counterpart. For example, geodesics work has focused on the magnetic case [27][28][29][30][31]. The motion of charged particles in BH immersed in magnetic field was studied in [32][33][34][35].…”
Section: Introductionmentioning
confidence: 99%
“…In the present case where the black hole is immersed in an electric field, it is not possible to cast Eq. (10) in the form of of an effective potential equation. Nevertheless, it is still possible to study the existence of bound and unbound orbits by rearranging to obtain…”
Section: Curves Of Zero Velocitymentioning
confidence: 99%
“…The geodesic motion for null and timelike particles is considered in [7,8,9]. Some later works on this topic include [10,11,12]. The motion of charged particles was also considered in the context of chaos and nonlinear dynamics in [13,14].…”
mentioning
confidence: 99%