61,932 research outputs found

    Demixing can occur in binary hard-sphere mixtures with negative non-additivity

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    A binary fluid mixture of non-additive hard spheres characterized by a size ratio γ=σ2/σ1<1\gamma=\sigma_2/\sigma_1<1 and a non-additivity parameter Δ=2σ12/(σ1+σ2)1\Delta=2\sigma_{12}/(\sigma_1+\sigma_2)-1 is considered in infinitely many dimensions. From the equation of state in the second virial approximation (which is exact in the limit dd\to\infty) a demixing transition with a critical consolute point at a packing fraction scaling as ηd2d\eta\sim d 2^{-d} is found, even for slightly negative non-additivity, if Δ>1/8(lnγ)2\Delta>-{1/8}(\ln\gamma)^2. Arguments concerning the stability of the demixing with respect to freezing are provided.Comment: 4 pages, 2 figures; title changed; final paragraph added; to be published in PRE as a Rapid Communicatio

    K X-Ray Energies and Transition Probabilities for He-, Li- and Be-like Praseodymium ions

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    Theoretical transition energies and probabilities for He-, Li- and Be-like Praseodymium ions are calculated in the framework of the multi-configuration Dirac-Fock method (MCDF), including QED corrections. These calculated values are compared to recent experimental data obtained in the Livermore SuperEBIT electron beam ion trap facility

    Strong flavour changing effective operator contributions to single top quark production

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    We study the effects of dimension six effective operators on the production of single top quarks at the LHC. The operator set considered includes terms with effective gluon interactions and four-fermion terms. Analytic expressions for the several partonic cross sections of single top production will be presented, as well as the results of their integration on the parton density functions.Comment: 20 pages, 7 fig

    The entropy of the noncommutative acoustic black hole based on generalized uncertainty principle

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    In this paper we investigate statistical entropy of a 3-dimensional rotating acoustic black hole based on generalized uncertainty principle. In our results we obtain an area entropy and a correction term associated with the noncommutative acoustic black hole when λ\lambda introduced in the generalized uncertainty principle takes a specific value. However, in this method, it is not needed to introduce the ultraviolet cut-off and divergences are eliminated. Moreover, the small mass approximation is not necessary in the original brick-wall model.Comment: 9 pages, no figures; version to appear in PLB. arXiv admin note: substantial text overlap with arXiv:1210.773

    Probing the Cosmological Principle in the counts of radio galaxies at different frequencies

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    According to the Cosmological Principle, the matter distribution on very large scales should have a kinematic dipole that is aligned with that of the CMB. We determine the dipole anisotropy in the number counts of two all-sky surveys of radio galaxies. For the first time, this analysis is presented for the TGSS survey, allowing us to check consistency of the radio dipole at low and high frequencies by comparing the results with the well-known NVSS survey. We match the flux thresholds of the catalogues, with flux limits chosen to minimise systematics, and adopt a strict masking scheme. We find dipole directions that are in good agreement with each other and with the CMB dipole. In order to compare the amplitude of the dipoles with theoretical predictions, we produce sets of lognormal realisations. Our realisations include the theoretical kinematic dipole, galaxy clustering, Poisson noise, simulated redshift distributions which fit the NVSS and TGSS source counts, and errors in flux calibration. The measured dipole for NVSS is  ⁣2\sim\!2 times larger than predicted by the mock data. For TGSS, the dipole is almost  ⁣5\sim\! 5 times larger than predicted, even after checking for completeness and taking account of errors in source fluxes and in flux calibration. Further work is required to understand the nature of the systematics that are the likely cause of the anomalously large TGSS dipole amplitude.Comment: 13 pages, 8 figures, 2 tables; Significant improvements. Version accepted by JCA
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