Envelopes for orbits around axially symmetric sources with spheroidal shape

Abstract

We introduce a method to obtain the envelopes of eccentric orbits in axially symmetric potentials, $\Phi (R,z)$, endowed with $z$-symmetry of reflection. By making the transformation $z\to a+\sqrt{a^2+z^2}$, with $a>0$, we compute the resulting mass density, referred here as the \emph{effective density} ${\rho }_{\mathrm{ef}}(R,z;a)$, in order to calculate the envelopes $Z(R)$ of orbits in the meridional plane $(R,z)$. We find that they obey the approximated formula $Z(R)\propto [{\Sigma }_{\mathrm{ef}}(R;a\approx 0){]}^{-1/3}$, where ${\Sigma }_{\mathrm{ef}}(R;a)$ is the integrated surface density associated with ${\rho }_{\mathrm{ef}}(R,z;a)$. As examples we consider the dynamics in two potentials: the monopole plus quadrupole and the Kalnajs disc.

arXiv comment7 pages, 12 figures

References in corpus (8)

• Models of our Galaxy II
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• Motion around a Monopole + Ring system: I. Stability of Equatorial Circular Orbits vs Regularity of Three-dimensional Motion
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Cited by in corpus (2)

• Chaotic dynamics of pulsating spheres orbiting black holes
• Chaotic orbital dynamics of pulsating stars around black holes surrounded by dark matter halos