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      Kohn's Theorem, Larmor's Equivalence Principle and the Newton-Hooke Group

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          Abstract

          We consider non-relativistic electrons, each of the same charge to mass ratio, moving in an external magnetic field with an interaction potential depending only on the mutual separations, possibly confined by a harmonic trapping potential. We show that the system admits a "relativity group" which is a one-parameter family of deformations of the standard Galilei group to the Newton-Hooke group which is a Wigner-Inonu contraction of the de Sitter group. This allows a group-theoretic interpretation of Kohn's theorem and related results. Larmor's Theorem is used to show that the one-parameter family of deformations are all isomorphic. We study the "Eisenhart" or "lightlike" lift of the system, exhibiting it as a pp-wave. In the planar case, the Eisenhart lift is the Brdicka-Eardley-Nappi-Witten pp-wave solution of Einstein-Maxwell theory, which may also be regarded as a bi-invariant metric on the Cangemi-Jackiw group.

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          Rotating trapped Bose-Einstein condensates

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            A WZW model based on a non-semi-simple group

            , (2010)
            We present a conformal field theory which desribes a homogeneous four dimensional Lorentz-signature space-time. The model is an ungauged WZW model based on a central extension of the Poincar\'e algebra. The central charge of this theory is exactly four, just like four dimensional Minkowski space. The model can be interpreted as a four dimensional monochromatic plane wave. As there are three commuting isometries, other interesting geometries are expected to emerge via \(O(3,3)\) duality.
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              Celestial Mechanics, Conformal Structures, and Gravitational Waves

              The equations of motion for \(N\) non-relativistic particles attracting according to Newton's law are shown to correspond to the equations for null geodesics in a \((3N+2)\)-dimensional Lorentzian, Ricci-flat, spacetime with a covariantly constant null vector. Such a spacetime admits a Bargmann structure and corresponds physically to a generalized pp-wave. Bargmann electromagnetism in five dimensions comprises the two Galilean electro-magnetic theories (Le Bellac and L\'evy-Leblond). At the quantum level, the \(N\)-body Schr\"odinger equation retains the form of a massless wave equation. We exploit the conformal symmetries of such spacetimes to discuss some properties of the Newtonian \(N\)-body problem: homographic solutions, the virial theorem, Kepler's third law, the Lagrange-Laplace-Runge-Lenz vector arising from three conformal Killing 2-tensors, and motions under inverse square law forces with a gravitational constant \(G(t)\) varying inversely as time (Dirac). The latter problem is reduced to one with time independent forces for a rescaled position vector and a new time variable; this transformation (Vinti and Lynden-Bell) arises from a conformal transformation preserving the Ricci-flatness (Brinkmann). A Ricci-flat metric representing \(N\) non-relativistic gravitational dyons is also pointed out. Our results for general time-dependent \(G(t)\) are applicable to the motion of point particles in an expanding universe. Finally we extend these results to the quantum regime.
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                Author and article information

                Journal
                12 October 2010
                2010-11-10
                Article
                10.1016/j.aop.2011.03.003
                1010.2455
                32e1e519-cce0-4eef-b9d5-b318d59f645c

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                DAMTP-2010-67, MIFPA-10-42
                Annals Phys.326:1760-1774,2011
                Typos corrected, references added
                hep-th cond-mat.str-el cond-mat.supr-con gr-qc

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