Circular orbits around gravitating configurations of phantom scalar fields
Vestnik Tverskogo gosudarstvennogo universiteta. Seriâ Prikladnaâ matematika, no. 4 (2016), pp. 61-78

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In this work we consider general properties of circular orbits in the neighborhood of spherically symmetric static configurations of gravitating phantom scalar fields. In this case the metric area function $C(r)$ (in the quasiglobal coordinates) completely determines the type of a configuration (black hole, naked singularity, wormhole). In any of these cases stable circular orbits can exist only in the region $r\geqslant 3m,\, r\geqslant r_0$, where $r_0$ is a unique minimum point of the function $C(r)$, and $m$ is the mass of the configuration. Wormholes that are symmetric relative to the throat, and topological geons can have circular orbits only on their throats or on the corresponding topological surfaces; at that, possible values of specific angular momentums on the corresponding stable orbits are bounded from above. We also present a classification of the gravitating configurations according to type of their innermost stable circular orbits.
Keywords: innermost stable circular orbit, phantom scalar field, black hole, wormhole, topological geon.
@article{VTPMK_2016_4_a4,
     author = {V. V. Nikonov and I. M. Potashov and A. N. Tsirulev and Yu. V. Tchemarina},
     title = {Circular orbits around gravitating configurations of phantom scalar fields},
     journal = {Vestnik Tverskogo gosudarstvennogo universiteta. Seri\^a Prikladna\^a matematika},
     pages = {61--78},
     publisher = {mathdoc},
     number = {4},
     year = {2016},
     language = {ru},
     url = {http://geodesic.mathdoc.fr/item/VTPMK_2016_4_a4/}
}
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V. V. Nikonov; I. M. Potashov; A. N. Tsirulev; Yu. V. Tchemarina. Circular orbits around gravitating configurations of phantom scalar fields. Vestnik Tverskogo gosudarstvennogo universiteta. Seriâ Prikladnaâ matematika, no. 4 (2016), pp. 61-78. http://geodesic.mathdoc.fr/item/VTPMK_2016_4_a4/