Covariant hamiltonian spin dynamics in curved space-time

被引:27
作者
d'Ambrosi, G. [1 ]
Kumar, S. Satish [2 ]
van Holten, J. W. [1 ,2 ]
机构
[1] Nikhef, Amsterdam, Netherlands
[2] Leiden Univ, Inst Lorentz, NL-2300 RA Leiden, Netherlands
关键词
TEST PARTICLES; CONSERVED QUANTITIES; KERR FIELD; BODIES;
D O I
10.1016/j.physletb.2015.03.007
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The dynamics of spinning particles in curved space-time is discussed, emphasizing the hamiltonian formulation. Different choices of hamiltonians allow for the description of different gravitating systems. We give full results for the simplest case with minimal hamiltonian, constructing constants of motion including spin. The analysis is illustrated by the example of motion in Schwarzschild space-time. We also discuss a non-minimal extension of the hamiltonian giving rise to a gravitational equivalent of the Stern-Gerlach force. We show that this extension respects a large class of known constants of motion for the minimal case. (C) 2015 The Authors. Published by Elsevier B.V.
引用
收藏
页码:478 / 483
页数:6
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