7,078 research outputs found

    Clebsch-Gordan Coefficients for the Extended Quantum-Mechanical Poincar\'e Group and Angular Correlations of Decay Products

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    This paper describes Clebsch-Gordan coefficients (CGCs) for unitary irreducible representations (UIRs) of the extended quantum mechanical Poincar\'e group \pt. `Extended' refers to the extension of the 10 parameter Lie group that is the Poincar\'e group by the discrete symmetries CC, PP, and TT; `quantum mechanical' refers to the fact that we consider projective representations of the group. The particular set of CGCs presented here are applicable to the problem of the reduction of the direct product of two massive, unitary irreducible representations (UIRs) of \pt with positive energy to irreducible components. Of the sixteen inequivalent representations of the discrete symmetries, the two standard representations with UCUP=±1U_C U_P = \pm 1 are considered. Also included in the analysis are additive internal quantum numbers specifying the superselection sector. As an example, these CGCs are applied to the decay process of the Υ(4S)\Upsilon(4S) meson.Comment: 26 pages, double spaced. Version 2: typos corrected, introduction change

    On the preservation of unitarity during black hole evolution and information extraction from its interior

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    For more than 30 years the discovery that black holes radiate like black bodies of specific temperature has triggered a multitude of puzzling questions concerning their nature and the fate of information that goes down the black hole during its lifetime. The most tricky issue in what is known as information loss paradox is the apparent violation of unitarity during the formation/evaporation process of black holes. A new idea is proposed based on the combination of our knowledge on Hawking radiation as well as the Einstein-Podolsky-Rosen phenomenon, that could resolve the paradox and spare physicists from the unpalatable idea that unitarity can ultimately be violated even under special conditions.Comment: 8 pages, no figure

    Classical solution of the wave equation

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    The classical limit of wave quantum mechanics is analyzed. It is shown that the general requirements of continuity and finiteness to the solution ψ(x)=Aeiϕ(x)+Beiϕ(x)\psi(x)=Ae^{i\phi(x)}+ Be^{-i\phi(x)}, where ϕ(x)=1W(x)\phi(x)=\frac 1\hbar W(x) and W(x)W(x) is the reduced classical action of the physical system, result in the asymptote of the exact solution and general quantization condition for W(x)W(x), which yields the exact eigenvalues of the system.Comment: 8 Pages, 10 Refs, LaTe

    The Causal Interpretation of Quantum Mechanics and The Singularity Problem in Quantum Cosmology

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    We apply the causal interpretation of quantum mechanics to homogeneous quantum cosmology and show that the quantum theory is independent of any time-gauge choice and there is no issue of time. We exemplify this result by studying a particular minisuperspace model where the quantum potential driven by a prescribed quantum state prevents the formation of the classical singularity, independently on the choice of the lapse function. This means that the fast-slow-time gauge conjecture is irrelevant within the framework of the causal interpretation of quantum cosmology.Comment: 18 pages, LaTe

    Typicality vs. probability in trajectory-based formulations of quantum mechanics

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    Bohmian mechanics represents the universe as a set of paths with a probability measure defined on it. The way in which a mathematical model of this kind can explain the observed phenomena of the universe is examined in general. It is shown that the explanation does not make use of the full probability measure, but rather of a suitable set function deriving from it, which defines relative typicality between single-time cylinder sets. Such a set function can also be derived directly from the standard quantum formalism, without the need of an underlying probability measure. The key concept for this derivation is the {\it quantum typicality rule}, which can be considered as a generalization of the Born rule. The result is a new formulation of quantum mechanics, in which particles follow definite trajectories, but which is only based on the standard formalism of quantum mechanics.Comment: 24 pages, no figures. To appear in Foundation of Physic

    The free energy in a class of quantum spin systems and interchange processes

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    We study a class of quantum spin systems in the mean-field setting of the complete graph. For spin S=12S=\tfrac12 the model is the Heisenberg ferromagnet, for general spin S12NS\in\tfrac12\mathbb{N} it has a probabilistic representation as a cycle-weighted interchange process. We determine the free energy and the critical temperature (recovering results by T\'oth and by Penrose when S=12S=\tfrac12). The critical temperature is shown to coincide (as a function of SS) with that of the q=2S+1q=2S+1 state classical Potts model, and the phase transition is discontinuous when S1S\geq1.Comment: 22 page

    Classical mechanics without determinism

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    Classical statistical particle mechanics in the configuration space can be represented by a nonlinear Schrodinger equation. Even without assuming the existence of deterministic particle trajectories, the resulting quantum-like statistical interpretation is sufficient to predict all measurable results of classical mechanics. In the classical case, the wave function that satisfies a linear equation is positive, which is the main source of the fundamental difference between classical and quantum mechanics.Comment: 11 pages, revised, to appear in Found. Phys. Let

    Relating the Lorentzian and exponential: Fermi's approximation,the Fourier transform and causality

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    The Fourier transform is often used to connect the Lorentzian energy distribution for resonance scattering to the exponential time dependence for decaying states. However, to apply the Fourier transform, one has to bend the rules of standard quantum mechanics; the Lorentzian energy distribution must be extended to the full real axis <E<-\infty<E<\infty instead of being bounded from below 0E<0\leq E <\infty (``Fermi's approximation''). Then the Fourier transform of the extended Lorentzian becomes the exponential, but only for times t0t\geq 0, a time asymmetry which is in conflict with the unitary group time evolution of standard quantum mechanics. Extending the Fourier transform from distributions to generalized vectors, we are led to Gamow kets, which possess a Lorentzian energy distribution with <E<-\infty<E<\infty and have exponential time evolution for tt0=0t\geq t_0 =0 only. This leads to probability predictions that do not violate causality.Comment: 23 pages, no figures, accepted by Phys. Rev.
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