4,573 research outputs found

    Spin Structure of the Proton

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    By assuming that there is no significant intrinsic polarization of the gluon, we have computed the polarized quark contributions to the proton's spin under SU(3) flavor symmetry breaking for the polarized sea and have performed a global leading-order QCD fit to obtain the spin-dependent quark distributions, which could be used as input for analyzing lepton-hadron and hadron-hadron collisions.Comment: 13 pages, NCKU-HEP/94-0

    Probing gravitational non-minimal coupling with dark energy surveys

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    We investigate observational constraints on a specific one-parameter extension to the minimal quintessence model, where the quintessence field acquires a quadratic coupling to the scalar curvature through a coupling constant ξ\xi. The value of ξ\xi is highly suppressed in typical tracker models if the late-time cosmic acceleration is driven at some field values near the Planck scale. We test ξ\xi in a second class of models in which the field value today becomes a free model parameter. We use the combined data from type-Ia supernovae, cosmic microwave background, baryon acoustic oscillations and matter power spectrum, to weak lensing measurements and find a best-fit value ξ>0.289\xi > 0.289 where ξ=0\xi = 0 is excluded outside the 95 per cent confidence region. The effective gravitational constant GeffG_{\rm eff} subject to the hint of a non-zero ξ\xi is constrained to −0.003<1−Geff/G<0.033-0.003 < 1- G_{\rm eff}/G < 0.033 at the same confidence level on cosmological scales, and can be narrowed down to 1−Geff/G<2.2×10−51- G_{\rm eff}/G < 2.2 \times 10^{-5} when combining with Solar System tests.Comment: Context extended, figures and references added, title changed to match with accepted version for publicatio
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