260,273 research outputs found

    A generalized structure of Bell inequalities for bipartite arbitrary dimensional systems

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    We propose a generalized structure of Bell inequalities for arbitrary d-dimensional bipartite systems, which includes the existing two types of Bell inequalities introduced by Collins-Gisin-Linden-Massar-Popescu [Phys. Rev. Lett. 88, 040404 (2002)] and Son-Lee-Kim [Phys. Rev. Lett. 96, 060406 (2006)]. We analyze Bell inequalities in terms of correlation functions and joint probabilities, and show that the coefficients of correlation functions and those of joint probabilities are in Fourier transform relations. We finally show that the coefficients in the generalized structure determine the characteristics of quantum violation and tightness.Comment: 6 pages, 1 figur

    Relativistic r-modes in Slowly Rotating Neutron Stars: Numerical Analysis in the Cowling Approximation

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    We investigate the properties of relativistic rr-modes of slowly rotating neutron stars by using a relativistic version of the Cowling approximation. In our formalism, we take into account the influence of the Coriolis like force on the stellar oscillations, but ignore the effects of the centrifugal like force. For three neutron star models, we calculated the fundamental rr-modes with l′=m=2l'=m=2 and 3. We found that the oscillation frequency σˉ\bar\sigma of the fundamental rr-mode is in a good approximation given by σˉ≈κ0Ω\bar\sigma\approx \kappa_0 \Omega, where σˉ\bar\sigma is defined in the corotating frame at the spatial infinity, and Ω\Omega is the angular frequency of rotation of the star. The proportional coefficient κ0\kappa_0 is only weakly dependent on Ω\Omega, but it strongly depends on the relativistic parameter GM/c2RGM/c^2R, where MM and RR are the mass and the radius of the star. All the fundamental rr-modes with l′=ml'=m computed in this study are discrete modes with distinct regular eigenfunctions, and they all fall in the continuous part of the frequency spectrum associated with Kojima's equation (Kojima 1998). These relativistic rr-modes are obtained by including the effects of rotation higher than the first order of Ω\Omega so that the buoyant force plays a role, the situation of which is quite similar to that for the Newtonian rr-modes.Comment: 22 pages, 8 figures, accepted for publication in Ap

    Liquid-Gas Phase Transition in Nuclear Equation of State

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    A canonical ensemble model is used to describe a caloric curve of nuclear liquid-gas phase transition. Allowing a discontinuity in the freeze out density from one spinodal density to another for a given initial temperature, the nuclear liquid-gas phase transition can be described as first order. Averaging over various freeze out densities of all the possible initial temperatures for a given total reaction energy, the first order characteristics of liquid-gas phase transition is smeared out to a smooth transition. Two experiments, one at low beam energy and one at high beam energy show different caloric behaviors and are discussed.Comment: 12 pages in Revtex including two Postscript figure

    Nuclear Incompressibility at Finite Temperature and Entropy

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    Features of the nuclear isothermal incompressibility κ\kappa and adiabatic incompressibility κQ\kappa_Q are investigated. The calculations are done at zero and finite temperatures and non zero entropy and for several equations of state. It is shown that κQ\kappa_Q decreases with increasing entropy while the isothermal κ\kappa increases with increasing TT. A duality is found between the adiabatic κQ\kappa_Q and the T=0 isothermal κ\kappa. Our isothermal results are compared with a recent lattice Monte Carlo calculation done at finite TT. The necessity of including correlations is shown if κ\kappa is to have a peak with increasing TT as seen in the Monte Carlo calculations. A peak in κ\kappa is linked to attractive scattering correlations in two nucleons channel in the virial expansion in our approach which are Pauli blocked at low TT.Comment: 5 page

    Characterization of the residual stresses in spray-formed steels using neutron diffraction

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    Neutron diffraction was used to characterize the residual stresses in an as-sprayed tube-shaped steel preform. The measured residual stress distributions were compared with those simulated using finite element method by taking into account the effects of the thermal history, porosity and different phases of the sprayed preform. The porosity was measured using X-ray microcomputed tomography. The study revealed for the first time the correlation between the distribution of porosity and residual stress developed in the as-sprayed preform
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