Contraction of broken symmetries via Kac-Moody formalism
arXiv:math-ph/0608008 · doi:10.1063/1.2234726
Abstract
I investigate contractions via Kac-Moody formalism. In particular, I show how the symmetry algebra of the standard 2-D Kepler system, which was identified by Daboul and Slodowy as an infinite-dimensional Kac-Moody loop algebra, and was denoted by , gets reduced by the symmetry breaking term, defined by the Hamiltonian \[ H(β)= \frac 1 {2m} (p_1^2+p_2^2)- \frac αr - βr^{-1/2} \cos ((ϕ-γ)/2). \] For this I define two symmetry loop algebras , by choosing the `basic generators' differently. These can be mapped isomorphically onto subalgebras of , of codimension 2 or 3, revealing the reduction of symmetry. Both factor algebras , relative to the corresponding energy-dependent ideals , are isomorphic to and for and , respectively, just as for the pure Kepler case. However, they yield two different non-standard contractions as , namely to the Heisenberg-Weyl algebra or to an abelian Lie algebra, instead of the Euclidean algebra for the pure Kepler case. The above example suggests a general procedure for defining generalized contractions, and also illustrates the {\em `deformation contraction hysteresis'}, where contraction which involve two contraction parameters can yield different contracted algebras, if the limits are carried out in different order.
21 pages, 1 figure