9,762 research outputs found

    Chiral low-energy constants from tau data

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    We analyze how the recent precise hadronic tau-decay data on the V-A spectral function and general properties of QCD such as analyticity, the operator product expansion and chiral perturbation theory (ChPT), can be used to improve the knowledge of some of the low-energy constants of ChPT. In particular we find the most precise values of L_{9,10} (or equivalently l_{5,6}) at order p^4 and p^6 and the first phenomenological determination of C_87 (c_50).Comment: Proceedings of the 6th International Workshop on Chiral Dynamics (Bern, Switzerland, July 6-10, 2009). 9 pages, 3 figure

    The Kink variety in systems of two coupled scalar fields in two space-time dimensions

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    In this paper we describe the moduli space of kinks in a class of systems of two coupled real scalar fields in (1+1) Minkowskian space-time. The main feature of the class is the spontaneous breaking of a discrete symmetry of (real) Ginzburg-Landau type that guarantees the existence of kink topological defects.Comment: 12 pages, 5 figures. To appear in Phys. Rev.

    Weighted random--geometric and random--rectangular graphs: Spectral and eigenfunction properties of the adjacency matrix

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    Within a random-matrix-theory approach, we use the nearest-neighbor energy level spacing distribution P(s)P(s) and the entropic eigenfunction localization length ℓ\ell to study spectral and eigenfunction properties (of adjacency matrices) of weighted random--geometric and random--rectangular graphs. A random--geometric graph (RGG) considers a set of vertices uniformly and independently distributed on the unit square, while for a random--rectangular graph (RRG) the embedding geometry is a rectangle. The RRG model depends on three parameters: The rectangle side lengths aa and 1/a1/a, the connection radius rr, and the number of vertices NN. We then study in detail the case a=1a=1 which corresponds to weighted RGGs and explore weighted RRGs characterized by a∼1a\sim 1, i.e.~two-dimensional geometries, but also approach the limit of quasi-one-dimensional wires when a≫1a\gg1. In general we look for the scaling properties of P(s)P(s) and ℓ\ell as a function of aa, rr and NN. We find that the ratio r/Nγr/N^\gamma, with γ(a)≈−1/2\gamma(a)\approx -1/2, fixes the properties of both RGGs and RRGs. Moreover, when a≥10a\ge 10 we show that spectral and eigenfunction properties of weighted RRGs are universal for the fixed ratio r/CNγr/{\cal C}N^\gamma, with C≈a{\cal C}\approx a.Comment: 8 pages, 6 figure

    Reinforcing the link between the double red clump and the X-shaped bulge of the Milky Way

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    The finding of a double red clump in the luminosity function of the Milky Way bulge has been interpreted as evidence for an X-shaped structure. Recently, an alternative explanation has been suggested, where the double red clump is an effect of multiple stellar populations in a classical spheroid. In this Letter we provide an observational assessment of this scenario and show that it is not consistent with the behaviour of the red clump across different lines of sight, particularly at high distances from the Galactic plane. Instead, we confirm that the shape of the red clump magnitude distribution closely follows the distance distribution expected for an X-shaped bulge at critical Galactic latitudes. We also emphasize some key observational properties of the bulge red clump that should not be neglected in the search for alternative scenarios

    On the semiclassical mass of S2{\mathbb S}^2-kinks

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    One-loop mass shifts to the classical masses of stable kinks arising in a massive non-linear S2{\mathbb S}^2-sigma model are computed. Ultraviolet divergences are controlled using the heat kernel/zeta function regularization method. A comparison between the results achieved from exact and high-temperature asymptotic heat traces is analyzed in depth.Comment: RevTex file, 15 pages, 2 figures. Version to appear in Journal of Physics
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