366 research outputs found

    The Gluonic Operator Matrix Elements at O(\alpha_s^2) for DIS Heavy Flavor Production

    Full text link
    We calculate the O(αs2)O(\alpha_s^2) gluonic operator matrix elements for the twist--2 operators, which contribute to the heavy flavor Wilson coefficients in unpolarized deeply inelastic scattering in the region Q2m2Q^2 \gg m^2, up to the linear terms in the dimensional parameter ε\varepsilon, (D=4+εD= 4 + \varepsilon). These quantities are required for the description of parton distribution functions in the variable flavor number scheme (VFNS). The O(αs2ε)O(\alpha_s^2 \varepsilon) terms contribute at the level of the O(αs3)O(\alpha_s^3) corrections through renormalization. We also comment on additional terms, which have to be considered in the fixed (FFNV) and variable flavor number scheme, adopting the MS\overline{\rm MS} scheme for the running coupling constant.Comment: 12 pages Latex, 1 style fil

    Production of massless charm jets in pp collisions at next-to-leading order of QCD

    Full text link
    We present predictions for the inclusive production of charm jets in proton-proton collisions at 7 TeV. Several CTEQ parton distribution functions (PDFs) of the CTEQ6.6M type are employed, where two of the CTEQ6.6 PDFs have intrinsic charm. At large enough jet transverse momentum and large jet rapidity, the intrinsic charm content can be tested.Comment: 11 pages, 4 figure

    Dynamical NNLO parton distributions

    Full text link
    Utilizing recent DIS measurements (\sigma_r, F_{2,3,L}) and data on hadronic dilepton production we determine at NNLO (3-loop) of QCD the dynamical parton distributions of the nucleon generated radiatively from valencelike positive input distributions at an optimally chosen low resolution scale (Q_0^2 < 1 GeV^2). These are compared with `standard' NNLO distributions generated from positive input distributions at some fixed and higher resolution scale (Q_0^2 > 1 GeV^2). Although the NNLO corrections imply in both approaches an improved value of \chi^2, typically \chi^2_{NNLO} \simeq 0.9 \chi^2_{NLO}, present DIS data are still not sufficiently accurate to distinguish between NLO results and the minute NNLO effects of a few percent, despite of the fact that the dynamical NNLO uncertainties are somewhat smaller than the NLO ones and both are, as expected, smaller than those of their `standard' counterparts. The dynamical predictions for F_L(x,Q^2) become perturbatively stable already at Q^2 = 2-3 GeV^2 where precision measurements could even delineate NNLO effects in the very small-x region. This is in contrast to the common `standard' approach but NNLO/NLO differences are here less distinguishable due to the much larger 1\sigma uncertainty bands. Within the dynamical approach we obtain \alpha_s(M_Z^2)=0.1124 \pm 0.0020, whereas the somewhat less constrained `standard' fit gives \alpha_s(M_Z^2)=0.1158 \pm 0.0035.Comment: 44 pages, 15 figures; minor changes, footnote adde

    First O(αs3)O(\alpha_s^3) heavy flavor contributions to deeply inelastic scattering

    Full text link
    In the asymptotic limit Q2m2Q^2 \gg m^2, the heavy flavor Wilson coefficients for deep--inelastic scattering factorize into the massless Wilson coefficients and the universal heavy flavor operator matrix elements resulting from light--cone expansion. In this way, one can calculate all but the power corrections in (m2/Q2)k,k>0(m^2/Q^2)^k, k > 0. The heavy flavor operator matrix elements are known to NLO{\sf NLO}. We present the last 2--loop result missing in the unpolarized case for the renormalization at 3--loops and first 3--loop results for terms proportional to the color factor TF2T_F^2 in Mellin--space. In this calculation, the corresponding parts of the NNLO{\sf NNLO} anomalous dimensions \cite{LARIN,MVVandim} are obtained as well.Comment: 6 pages, Contribution to the Proceedings of "Loops and Legs in Quantum Field Theory", 2008, Sondershausen, Germany, and DIS 2008, London, U

    What is the trouble with Dyson--Schwinger equations?

    Full text link
    We discuss similarities and differences between Green Functions in Quantum Field Theory and polylogarithms. Both can be obtained as solutions of fixpoint equations which originate from an underlying Hopf algebra structure. Typically, the equation is linear for the polylog, and non-linear for Green Functions. We argue though that the crucial difference lies not in the non-linearity of the latter, but in the appearance of non-trivial representation theory related to transcendental extensions of the number field which governs the linear solution. An example is studied to illuminate this point.Comment: 5 pages contributed to the proceedings "Loops and Legs 2004", April 2004, Zinnowitz, German

    EOSC-hub Configuration Management Plan

    Get PDF

    Identification of Cost Effective Energy Conservation Methods

    Get PDF
    In addition to a successful program of readily implemented conservation actions for reducing building energy consumption at Kennedy Space Center, recent detailed analyses have identified further substantial savings for buildings representative of technical facilities designed when energy costs were low. The techniques employed for determination of these energy savings consisted of facility configuration analysis, power and lighting measurements, detailed computer simulations and simulation verifications. Use of these methods resulted in identification of projected energy savings as large as $330,000 a year (approximately fwo year breakeven period) in a single building. Application of these techniques to other commercial buildings is discussed
    corecore