10,007 research outputs found

    Quantum counterpart of spontaneously broken classical PT symmetry

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    The classical trajectories of a particle governed by the PT-symmetric Hamiltonian H=p2+x2(ix)ϵH=p^2+x^2(ix)^\epsilon (ϵ≥0\epsilon\geq0) have been studied in depth. It is known that almost all trajectories that begin at a classical turning point oscillate periodically between this turning point and the corresponding PT-symmetric turning point. It is also known that there are regions in ϵ\epsilon for which the periods of these orbits vary rapidly as functions of ϵ\epsilon and that in these regions there are isolated values of ϵ\epsilon for which the classical trajectories exhibit spontaneously broken PT symmetry. The current paper examines the corresponding quantum-mechanical systems. The eigenvalues of these quantum systems exhibit characteristic behaviors that are correlated with those of the associated classical system.Comment: 11 pages, 7 figure

    PT-symmetric quantum field theory in D dimensions

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    PT-symmetric quantum mechanics began with a study of the Hamiltonian H=p2+x2(ix)εH=p^2+x^2(ix)^\varepsilon. A surprising feature of this non-Hermitian Hamiltonian is that its eigenvalues are discrete, real, and positive when ε≥0\varepsilon\geq0. This paper examines the corresponding quantum-field-theoretic Hamiltonian H=12(∇ϕ)2+12ϕ2(iϕ)εH=\frac{1}{2}(\nabla\phi)^2+\frac{1}{2}\phi^2(i\phi)^\varepsilon in DD-dimensional spacetime, where ϕ\phi is a pseudoscalar field. It is shown how to calculate the Green's functions as series in powers of ε\varepsilon directly from the Euclidean partition function. Exact finite expressions for the vacuum energy density, all of the connected nn-point Green's functions, and the renormalized mass to order ε\varepsilon are derived for 0≤D<20\leq D<2. For D≥2D\geq2 the one-point Green's function and the renormalized mass are divergent, but perturbative renormalization can be performed. The remarkable spectral properties of PT-symmetric quantum mechanics appear to persist in PT-symmetric quantum field theory.Comment: 8 page

    A Class of Exactly-Solvable Eigenvalue Problems

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    The class of differential-equation eigenvalue problems −y′′(x)+x2N+2y(x)=xNEy(x)-y''(x)+x^{2N+2}y(x)=x^N Ey(x) (N=−1,0,1,2,3,...N=-1,0,1,2,3,...) on the interval −∞<x<∞-\infty<x<\infty can be solved in closed form for all the eigenvalues EE and the corresponding eigenfunctions y(x)y(x). The eigenvalues are all integers and the eigenfunctions are all confluent hypergeometric functions. The eigenfunctions can be rewritten as products of polynomials and functions that decay exponentially as x→±∞x\to\pm \infty. For odd NN the polynomials that are obtained in this way are new and interesting classes of orthogonal polynomials. For example, when N=1, the eigenfunctions are orthogonal polynomials in x3x^3 multiplying Airy functions of x2x^2. The properties of the polynomials for all NN are described in detail.Comment: REVTeX, 16 pages, no figur

    PT-Symmetric Representations of Fermionic Algebras

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    A recent paper by Jones-Smith and Mathur extends PT-symmetric quantum mechanics from bosonic systems (systems for which T2=1T^2=1) to fermionic systems (systems for which T2=−1T^2=-1). The current paper shows how the formalism developed by Jones-Smith and Mathur can be used to construct PT-symmetric matrix representations for operator algebras of the form η2=0\eta^2=0, ηˉ2=0\bar{\eta}^2=0, ηηˉ+ηˉ=α1\eta\bar{\eta}+\bar {\eta} =\alpha 1, where etaˉ=ηPT=PTηT−1P−1\bar{eta}=\eta^{PT} =PT \eta T^{-1}P^{-1}. It is easy to construct matrix representations for the Grassmann algebra (α=0\alpha=0). However, one can only construct matrix representations for the fermionic operator algebra (α≠0\alpha\neq0) if α=−1\alpha= -1; a matrix representation does not exist for the conventional value α=1\alpha=1.Comment: 5 pages, 2 figure
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