6,706 research outputs found

    Supersymmetry of the magnetic vortex

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    The N=2 supersymmetry of the Pauli Hamiltonian in any static magnetic field in the plane combines, for the magnetic vortex, with Jackiw's bosonic o(2)×o(2,1)o(2)\times o(2,1) symmetry, into an o(2)×osp(1/2)o(2)\times osp(1/2) dynamical supersymmetry.Comment: 4 pages. Originally Tours Preprint no 60/93 (1993). Unpublishe

    Chiral fermions as classical massless spinning particles

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    Semiclassical chiral fermion models with Berry term are studied in a symplectic framework. In the free case, the system can be obtained from Souriau's model for a relativistic massless spinning particle by "enslaving" the spin. The Berry term is identified with the classical spin two-form of the latter model. The Souriau model carries a natural Poincar\'e symmetry that we highlight, but spin enslavement breaks the boost symmetry. However the relation between the models allows us to derive a Poincare symmetry of unconventional form for chiral fermions. Then we couple our system to an external electromagnetic field. For gyromagnetic ratio g=0g=0 we get curious superluminal Hall-type motions; for g=2g=2 and in a pure constant magnetic field in particular, we find instead spiraling motions.Comment: Substantially revised and extended version. 31 pages, 5 figures. Details clarified and references added. To be published in PR

    Anyons with anomalous gyromagnetic ratio & the Hall effect

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    Letting the mass depend on the spin-field coupling as M2=m2−(eg/2c2)FαβSαβM^2=m^2-(eg/2c^2)F_{\alpha\beta}S^{\alpha\beta}, we propose a new set of relativistic planar equations of motion for spinning anyons. Our model can accommodate any gyromagnetic ratio gg and provides us with a novel version of the Bargmann-Michel-Telegdi equations in 2+1 dimensions. The system becomes singular when the field takes a critical value, and, for g≠2g\neq2, the only allowed motions are those which satisfy the Hall law. For each g≠2,0g\neq2,0 a secondary Hall effect arises also for another critical value of the field. The non-relativistic limit of our equations yields new models which generalize our previous ``exotic'' model, associated with the two-fold central extension of the planar Galilei group.Comment: The affiliation of the first author's Institution is presented in detail. LaTeX, 12 pages no figures. To appear in Phys. Lett.
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