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Dynamics of a spinning particle in a linear in spin Hamiltonian approximation

Georgios Lukes-GerakopoulosInstitute of Theoretical Physics, Faculty of Mathematics and Physics, Charles University in Prague, 18000 Prague, Czech RepublicMatthaios KatsanikasResearch Center for Astronomy, Academy of Athens, Soranou Efessiou 4, GR-115 27 Athens, GreeceP. A. PatsisResearch Center for Astronomy, Academy of Athens, Soranou Efessiou 4, GR-115 27 Athens, GreeceJonathan SeyrichMathematisches Institut, Universität Tübingen, Auf der Morgenstelle, 72076 Tübingen, Germany
2016en
ABI

Abstract

We investigate for order and chaos the dynamical system of a spinning test particle of mass $m$ moving in the spacetime background of a Kerr black hole of mass $M$. This system is approximated in our investigation by the linear in spin Hamiltonian function [E. Barausse and A. Buonanno, Phys. Rev. D 81, 084024 (2010)]. We study the corresponding phase space by using 2D projections on a surface of section and the method of color and rotation on a 4D Poincar\'e section. Various topological structures coming from the nonintegrability of the linear in spin Hamiltonian are found and discussed. Moreover, an interesting result is that from the value of the dimensionless spin $S/(mM)={10}^{\ensuremath{-}4}$ of the particle and below, the impact of the nonintegrability of the system on the motion of the particle seems to be negligible.

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