423 research outputs found

    Self-similar stable processes arising from high-density limits of occupation times of particle systems

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    We extend results on time-rescaled occupation time fluctuation limits of the (d,α,β)(d,\alpha, \beta)-branching particle system (0<α2,0<β1)(0<\alpha \leq 2, 0<\beta \leq 1) with Poisson initial condition. The earlier results in the homogeneous case (i.e., with Lebesgue initial intensity measure) were obtained for dimensions d>α/βd>\alpha / \beta only, since the particle system becomes locally extinct if dα/βd\le \alpha / \beta. In this paper we show that by introducing high density of the initial Poisson configuration, limits are obtained for all dimensions, and they coincide with the previous ones if d>α/βd>\alpha/\beta. We also give high-density limits for the systems with finite intensity measures (without high density no limits exist in this case due to extinction); the results are different and harder to obtain due to the non-invariance of the measure for the particle motion. In both cases, i.e., Lebesgue and finite intensity measures, for low dimensions (d<α(1+β)/βd<\alpha(1+\beta)/\beta and d<α(2+β)/(1+β)d<\alpha(2+\beta)/(1+\beta), respectively) the limits are determined by non-L\'evy self-similar stable processes. For the corresponding high dimensions the limits are qualitatively different: S(Rd){\cal S}'(R^d)-valued L\'evy processes in the Lebesgue case, stable processes constant in time on (0,)(0,\infty) in the finite measure case. For high dimensions, the laws of all limit processes are expressed in terms of Riesz potentials. If β=1\beta=1, the limits are Gaussian. Limits are also given for particle systems without branching, which yields in particular weighted fractional Brownian motions in low dimensions. The results are obtained in the setup of weak convergence of S'(R^d)$-valued processes.Comment: 28 page

    Analysis of the vector form factors fKπ+(Q2)f^+_{K\pi}(Q^2) and fKπ(Q2)f^-_{K\pi}(Q^2) with light-cone QCD sum rules

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    In this article, we calculate the vector form factors fKπ+(Q2)f^+_{K\pi}(Q^2) and fKπ(Q2)f^-_{K\pi}(Q^2) within the framework of the light-cone QCD sum rules approach. The numerical values of the fKπ+(Q2)f^+_{K\pi}(Q^2) are compatible with the existing theoretical calculations, the central value of the fKπ+(0)f^+_{K\pi}(0), fKπ+(0)=0.97f^+_{K\pi}(0)=0.97, is in excellent agreement with the values from the chiral perturbation theory and lattice QCD. The values of the fKπ(0)|f^-_{K\pi}(0)| are very large comparing with the theoretical calculations and experimental data, and can not give any reliable predictions. At large momentum transfers with Q2>5GeV2Q^2> 5GeV^2, the form factors fKπ+(Q2)f^+_{K\pi}(Q^2) and fKπ(Q2)|f^-_{K\pi}(Q^2)| can either take up the asymptotic behavior of 1Q2\frac{1}{Q^2} or decrease more quickly than 1Q2\frac{1}{Q^2}, more experimental data are needed to select the ideal sum rules.Comment: 22 pages, 16 figures, revised version, to appear in Eur. Phys. J.

    Search for direct production of charginos and neutralinos in events with three leptons and missing transverse momentum in √s = 7 TeV pp collisions with the ATLAS detector

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    A search for the direct production of charginos and neutralinos in final states with three electrons or muons and missing transverse momentum is presented. The analysis is based on 4.7 fb−1 of proton–proton collision data delivered by the Large Hadron Collider and recorded with the ATLAS detector. Observations are consistent with Standard Model expectations in three signal regions that are either depleted or enriched in Z-boson decays. Upper limits at 95% confidence level are set in R-parity conserving phenomenological minimal supersymmetric models and in simplified models, significantly extending previous results

    The Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the extended Baryon Oscillation Spectroscopic Survey and from the second phase of the Apache Point Observatory Galactic Evolution Experiment

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    The fourth generation of the Sloan Digital Sky Survey (SDSS-IV) has been in operation since July 2014. This paper describes the second data release from this phase, and the fourteenth from SDSS overall (making this, Data Release Fourteen or DR14). This release makes public data taken by SDSS-IV in its first two years of operation (July 2014-2016). Like all previous SDSS releases, DR14 is cumulative, including the most recent reductions and calibrations of all data taken by SDSS since the first phase began operations in 2000. New in DR14 is the first public release of data from the extended Baryon Oscillation Spectroscopic Survey (eBOSS); the first data from the second phase of the Apache Point Observatory (APO) Galactic Evolution Experiment (APOGEE-2), including stellar parameter estimates from an innovative data driven machine learning algorithm known as "The Cannon"; and almost twice as many data cubes from the Mapping Nearby Galaxies at APO (MaNGA) survey as were in the previous release (N = 2812 in total). This paper describes the location and format of the publicly available data from SDSS-IV surveys. We provide references to the important technical papers describing how these data have been taken (both targeting and observation details) and processed for scientific use. The SDSS website (www.sdss.org) has been updated for this release, and provides links to data downloads, as well as tutorials and examples of data use. SDSS-IV is planning to continue to collect astronomical data until 2020, and will be followed by SDSS-V.Comment: SDSS-IV collaboration alphabetical author data release paper. DR14 happened on 31st July 2017. 19 pages, 5 figures. Accepted by ApJS on 28th Nov 2017 (this is the "post-print" and "post-proofs" version; minor corrections only from v1, and most of errors found in proofs corrected

    Measurement of the tau lepton lifetime

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    Measurement of the D±^{*\pm} cross section in two photon collisions at LEP

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    Tau leptonic branching ratios

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    Measurement of the tau lepton lifetime

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    Measurement of the tau lepton lifetime

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    A multi-scale microstructure to address the strength-ductility trade off in high strength steel for fusion reactors

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    Fusion reactor materials for the first wall and blanket must have high strength, be radiation tolerant and be reduced activation (low post-use radioactivity), which has resulted in reduced activation ferritic/martensitic (RAFM) steels. The current steels suffer irradiation-induced hardening and embrittlement and are not adequate for planned commercial fusion reactors. Producing high strength, ductility and toughness is difficult, because inhibiting deformation to produce strength also reduces the amount of work hardening available, and thereby ductility. Here we solve this dichotomy to introduce a high strength and high ductility RAFM steel, produced by a modified thermomechanical process route. A unique multiscale microstructure is developed, comprising nanoscale and microscale ferrite, tempered martensite containing fine subgrains and a high density of nanoscale precipitates. High strength is attributed to the fine grain and subgrain and a higher proportion of metal carbides, while the high ductility results from a high mobile dislocation density in the ferrite, subgrain formation in the tempered martensite, and the bimodal microstructure, which improves ductility without impairing strength
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