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      NNLO corrections to the total cross section for Higgs boson production in hadron-hadron collisions

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          Abstract

          We present the next-to-next-to-leading order (NNLO) corrections to the total cross section for (pseudo-) scalar Higgs boson production using an alternative method than those used in previous calculations. All QCD partonic subprocesses have been included and the computation is carried out in the effective Lagrangian approach which emerges from the standard model by taking the limit \(m_t \to \infty\) where \(m_t\) denotes the mass of the top quark. Our results agree with those published earlier in the literature. We estimate the theoretical uncertainties by comparing the \(K\)-factors and the variation with respect to the mass factorization/renormalization scales with the results obtained by lower order calculations. We also investigate the dependence of the cross section on several parton density sets provided by different groups. Further we study which part of the coefficient functions dominates the cross section. This is of interest for the resummation of large corrections which occur near the boundary of phase space. It turns out that depending on the definition of the total cross section the latter is dominated by the the soft-plus-virtual gluon corrections represented by \(\delta(1-x)\) and \((\ln^i(1-x)/(1-x))_+\) terms. PACS numbers: 12.38.-t, 12.38.Bx, 13.85.-t, 14.80.Gt.

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          Absence of Higher-Order Corrections in the Anomalous Axial-Vector Divergence Equation

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            Next-to-Next-to-Leading Order Higgs Production at Hadron Colliders

            The Higgs boson production cross section at pp and p\bar{p} colliders is calculated in QCD at next-to-next-to-leading order (NNLO). We find that the perturbative expansion of the production cross section is well behaved and that scale dependence is reduced relative to the NLO result. These findings give us confidence in the reliability of the prediction. We also report an error in the NNLO correction to Drell-Yan production.
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              Dynamical Parton Distributions Revisited

              Dynamical parton densities, generated radiatively from valence-like inputs at some low resolution scale, are confronted with recent small-x data on deep inelastic and other hard scattering processes. It is shown that within theoretical uncertainties our previous (1994) dynamical/radiative parton distributions are compatible with most recent data and still applicable within the restricted accuracy margins of the presently available next-to-leading order calculations. Due to recent high precision measurements we also present an updated, more accurate, version of our (valence-like) dynamical input distributions. Furthermore, our perturbatively stable parameter-free dynamical predictions are extended to the extremely small-x region, 10^-8 ~< x ~< 10^-5, relevant to questions concerning ultra-high-energy cosmic ray and neutrino astronomy.
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                Author and article information

                Journal
                17 February 2003
                2003-04-05
                Article
                10.1016/S0550-3213(03)00457-7
                hep-ph/0302135
                6351df5c-82de-4f25-8ee6-989769b4f08f
                History
                Custom metadata
                Nucl.Phys.B665:325-366,2003
                61 pages, LaTeX, 15 postscript figures. With respect to the previous version a more thorough comparison is made between two definitions of the soft plus virtual gluon approximation. Misprints are corrected and references are changed. Figs. 8a, 9a are changed into Figs. 8,9 respectively and Figs. 8b, 9b are dropped
                hep-ph

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