DYNAMICAL SYMMETRY AND MAGNETIC CHARGE

被引:16
作者
SCHONFELD, JF [1 ]
机构
[1] UNIV MINNESOTA, SCH PHYS & ASTRON, MINNEAPOLIS, MN 55455 USA
关键词
D O I
10.1063/1.524360
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
By adding to the force between an electric and a magnetic point charge a central force arising from a specially chosen potential, one can construct a system known to have the same SO (3,1) and/or SO (4) dynamical symmetry algebra as the Kepler system. We derive protective changes of variables under which the classical orbits of any such system are put in one-to-one correspondence with SO (3,1)- and/or SO (4)-invariant sets of curves on similarly invariant surfaces. This extends results hitherto established only for the Kepler system. This is surprising in that there is a sense in which the phase space of such a magnetic system is a truncation of the Kepler phase space and so one might have expected such global properties not to generalize. Our transformations apparently do not permit transcription of the corresponding Schrödinger equation into a manifestly SO (3,1)-and/or SO (4)-symmetric form, in contrast to the pure Kepler case. Such magnetic systems play roles in the theory of quantum fields in Taub-NUT space-times, and in the theory of quantum-mechanical fluctuations about extended magnetic monopoles in supersymmetric gauge theories. In passing, we use the properties of the magnetic systems to formulate a very short and direct proof that the classical orbits of the Kepler system are conic sections. © 1980 American Institute of Physics.
引用
收藏
页码:2528 / 2533
页数:6
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