SIGMA 7 (2011), 113, 11 pages arXiv:1112.2333
Breaking Pseudo-Rotational Symmetry through H+2 Metric Deformation in the Eckart Potential Problem
Nehemias Leija-Martinez a, David Edwin Alvarez-Castillo b and Mariana Kirchbach a
a) Institute of Physics, Autonomous University of San Luis Potosi, Av. Manuel Nava 6, San Luis Potosi, S.L.P. 78290, Mexico
b) H. Niewodniczanski Institute of Nuclear Physics, Radzikowskiego 152, 31-342 Kraków, Poland
Received October 12, 2011, in final form December 08, 2011; Published online December 11, 2011; Misprints are corrected December 24, 2011
The peculiarity of the Eckart potential problem
on H+2 (the upper sheet of the two-sheeted two-dimensional
to preserve the (2l+1)-fold degeneracy of the states
typical for the geodesic motion there, is usually explained in casting
the respective Hamiltonian in terms of the Casimir invariant of
an so(2,1) algebra, referred to as potential algebra. In general,
there are many possible
similarity transformations of the symmetry algebras of the free motions on
curved surfaces towards potential algebras, which are not all
In the literature, a transformation of the symmetry algebra of the geodesic
motion on H+2 towards the potential algebra of Eckart's Hamiltonian
has been constructed for the prime purpose to prove that
the Eckart interaction belongs to the class of Natanzon potentials.
We here take a different path and search for a transformation which
connects the (2l+1) dimensional representation space of the
pseudo-rotational so(2,1) algebra, spanned by the rank-l
pseudo-spherical harmonics, to the representation space of equal dimension
of the potential algebra and find a transformation of the scaling type.
Our case is that in so doing one is producing a deformed isometry copy
to H+2 such that the free motion on the copy
is equivalent to a motion on H+2, perturbed by a
In this way, we link the so(2,1) potential algebra concept of the
Eckart Hamiltonian to a subtle type of pseudo-rotational symmetry breaking
through H+2 metric deformation.
From a technical point of view, the results reported here are obtained by
virtue of certain nonlinear finite expansions of Jacobi polynomials into
pseudo-spherical harmonics. In due places, the pseudo-rotational
case is paralleled by its so(3) compact analogue, the cotangent
perturbed motion on S2.
We expect awareness of different so(2,1)/so(3) isometry copies
to benefit simulation studies on curved manifolds of many-body systems.
pseudo-rotational symmetry; Eckart potential; symmetry breaking through metric deformation.
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