1,942 research outputs found

    QCD Radiative Correction to Zero Recoil Sum Rules for Heavy Flavor Transitions in the Small Velocity Limit.

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    We consider the small velocity sum rules for heavy flavour semileptonic transitions that are used to estimate the zero recoil values of semileptonic heavy flavour form factors. We analyze the complete O(αS\alpha _S) radiative correction to these sum rules. The corrections are universal and influence all "model-independent" bounds previously derived for semileptonic form factors at zero recoil.Comment: 13 pages, LaTeX, 3 figures

    Precision study of positronium and precision tests of the bound state QED

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    Despite its very short lifetime positronium provides us with a number of accurate tests of the bound state QED. In this note a brief overview of QED theory and precision experiments on the spectrum and annihilation decay of the positronium atom is presented. Special attention is paid to the accuracy of theoretical predictions.Comment: A talk presented at 9th International Workshop on Slow Positron Beam Techniques for Solids and Surfaces (SLOPOS), Dresden, 200

    Two -loop O(GFMH2)O(G_F{M_H}^2) radiative corrections to the Higgs decay width H→γγH \to \gamma \gamma for large Higgs boson masses

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    This note is devoted to the calculation of the two-loop O(GFMH2)O(G_F {M_H}^2) radiative corrections to the Higgs decay width H→γγH \to \gamma \gamma for large values of the Higgs boson mass MHM_H within the Minimal Standard Model. The use of the Equivalence Theorem makes it possible to reduce the problem to the consideration of the physical Higgs boson field and the Goldstone bosons w+,w−,zw^{+},w^{-},z. We present analytical results for the various two- and three-particle absorptive parts of two-loop contributions, using dispersive techniques, analytic results for all but one of the dispersive contributions. The typical size of the correction is ∼ 30\sim ~30 percent for a Higgs boson mass of order 1 TeV1~TeV.Comment: 21 pages, 7 uuencoded figure

    Hadronic Light-by-Light Scattering in the Muonium Hyperfine Splitting

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    We consider an impact of hadronic light-by-light scattering on the muonium hyperfine structure. A shift of the hyperfine interval Δν(Mu)HLBL\Delta \nu({\rm Mu}) _{\rm\tiny HLBL} is calculated with the light-by-light scattering approximated by exchange of pseudoscalar and pseudovector mesons. Constraints from the operator product expansion in QCD are used to fix parameters of the model similar to the one used earlier for the hadronic light-by-light scattering in calculations of the muon anomalous magnetic moment. The pseudovector exchange is dominant in the resulting shift, Δν(Mu)HLBL=−0.0065(10)Hz\Delta \nu({\rm Mu})_{\rm\tiny HLBL}= -0.0065(10) {Hz}. Although the effect is tiny it is useful in understanding the level of hadronic uncertainties.Comment: 16 pages, 7 figures, a reference adde

    On Unitary Evolution of a Massless Scalar Field In A Schwarzschild Background: Hawking Radiation and the Information Paradox

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    We develop a Hamiltonian formalism which can be used to discuss the physics of a massless scalar field in a gravitational background of a Schwarzschild black hole. Using this formalism we show that the time evolution of the system is unitary and yet all known results such as the existence of Hawking radiation can be readily understood. We then point out that the Hamiltonian formalism leads to interesting observations about black hole entropy and the information paradox.Comment: 45 pages, revte
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