11,787 research outputs found

    Deformation Quantization of the Isotropic Rotator

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    We perform a deformation quantization of the classical isotropic rigid rotator. The resulting quantum system is not invariant under the usual SU(2)×SU(2)SU(2)\times SU(2) chiral symmetry, but instead SUq1(2)×SUq(2)SU_{q^{-1}}(2) \times SU_q(2).Comment: 12pp, LATE

    Two-parameter deformation of the Poincar\'e algebra

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    We examine a two-parameter (,\hbar , λ\lambda ) deformation of the Poincar\`e algebra which is covariant under the action of SLq(2,C).SL_q(2,C). When λ0\lambda \rightarrow 0 it yields the Poincar\`e algebra, while in the 0\hbar\rightarrow 0 limit we recover the classical quadratic algebra discussed previously in \cite{ssy95}, \cite{sy95}. The analogues of the Pauli-Lubanski vector ww and Casimirs p2p^2 and w2w^2 are found and a set of mutually commuting operators is constructed.Comment: 10 pages, Latex2

    Proposed experiments to probe the non-abelian \nu=5/2 quantum Hall state

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    We propose several experiments to test the non-abelian nature of quasi-particles in the fractional quantum Hall state of \nu=5/2. One set of experiments studies interference contribution to back-scattering of current, and is a simplified version of an experiment suggested recently. Another set looks at thermodynamic properties of a closed system. Both experiments are only weakly sensitive to disorder-induced distribution of localized quasi-particles.Comment: Additional references and an improved figure, 5 page

    Properties of Quantum Hall Skyrmions from Anomalies

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    It is well known that the Fractional Quantum Hall Effect (FQHE) may be effectively represented by a Chern-Simons theory. In order to incorporate QH Skyrmions, we couple this theory to the topological spin current, and include the Hopf term. The cancellation of anomalies for chiral edge states, and the proviso that Skyrmions may be created and destroyed at the edge, fixes the coefficients of these new terms. Consequently, the charge and the spin of the Skyrmion are uniquely determined. For those two quantities we find the values eνNSkye\nu N_{Sky} and νNSky/2\nu N_{Sky}/2, respectively, where ee is electron charge, ν\nu is the filling fraction and NSkyN_{Sky} is the Skyrmion winding number. We also add terms to the action so that the classical spin fluctuations in the bulk satisfy the standard equations of a ferromagnet, with spin waves that propagate with the classical drift velocity of the electron.Comment: 8 pages, LaTeX file; Some remarks are included to clarify the physical results obtained, and the role of the Landau-Lifshitz equation is emphasized. Some references adde

    Lie-Poisson Deformation of the Poincar\'e Algebra

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    We find a one parameter family of quadratic Poisson structures on R4×SL(2,C){\bf R}^4\times SL(2,C) which satisfies the property {\it a)} that it is preserved under the Lie-Poisson action of the Lorentz group, as well as {\it b)} that it reduces to the standard Poincar\'e algebra for a particular limiting value of the parameter. (The Lie-Poisson transformations reduce to canonical ones in that limit, which we therefore refer to as the `canonical limit'.) Like with the Poincar\'e algebra, our deformed Poincar\'e algebra has two Casimir functions which we associate with `mass' and `spin'. We parametrize the symplectic leaves of R4×SL(2,C){\bf R}^4\times SL(2,C) with space-time coordinates, momenta and spin, thereby obtaining realizations of the deformed algebra for the cases of a spinless and a spinning particle. The formalism can be applied for finding a one parameter family of canonically inequivalent descriptions of the photon.Comment: Latex file, 26 page

    Lorentz Transformations as Lie-Poisson Symmetries

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    We write down the Poisson structure for a relativistic particle where the Lorentz group does not act canonically, but instead as a Poisson-Lie group. In so doing we obtain the classical limit of a particle moving on a noncommutative space possessing SLq(2,C)SL_q(2,C) invariance. We show that if the standard mass shell constraint is chosen for the Hamiltonian function, then the particle interacts with the space-time. We solve for the trajectory and find that it originates and terminates at singularities.Comment: 18 page
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