266 research outputs found

    QCD Radiative Correction to the Hadronic Annihilation Rate of 1+−1^{+-} Heavy Quarkonium

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    Hadronic annihilation rate of 1+−1^{+-} heavy quarkonium is given to next-to-leading order in αs\alpha_s and leading order in v2v^2 using a recently developed factorization formalism which is based on NRQCD. The result includes both the annihilation of P-wave color-singlet QQˉQ\bar{Q} component, and the annihilation of S-wave color-octet QQˉQ\bar{Q} component of the quarkonium. The notorious infrared divergences due to soft gluons, i.e., the Logarithms associated with the binding energy, encountered in previous perturbative calculations of 1+−1^{+-} quarkonium decays are found to be explicitly cancelled, and a finite result for the decay width to order αs3\alpha_s^3 is then obtained.Comment: 15 pages latex (6 figures included). In this revised version a update reference and acknowledgement are include

    X(3872) and its production at hadron colliders

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    We evaluate the production cross sections of X(3872)X(3872) at the LHC and Tevatron at NLO in αs\alpha_s in NRQCD by assuming that the short-distance production proceeds dominantly through its χc1′\chi_{c1}' component in our \chi_{c1}'\mbox{-}D^0\bar{D}^{*0} mixing model for X(3872)X(3872). The outcomes of the fits to the CMS pTp_T distribution can well account for the recent ATLAS data in a much larger range of transverse momenta (10~\mbox{GeV}), and the CDF total cross section data, and are also consistent with the value of k=Zccˉ⋅Br(X→J/ψπ+π−)k=Z_{c\bar c}\cdot Br(X\to J/\psi\pi^+\pi^-) constrained by the BB-meson decay data. %It can also well describe the behavior of the CDF ψ(2S)\psi(2S) data, which show a strong %resemblance to that of the X(3872). For LHCb the predicted X(3872) total cross section is larger than the data by a factor of 2, which is due to the problem of the fixed-order NRQCD calculation that may not be applicable for the region with small pTp_T (p_T\sim 5 ~\mbox{GeV}) and large forward rapidity (2.5<y<4.5)(2.5<y<4.5). In comparison, the prediction of molecule production mechanism for X(3872)X(3872) is inconsistent with both pTp_T distributions and total cross sections of CMS and ATLAS, and the total cross section of CDF.Comment: Version published in PRD. More explanations added for the LHCb data. More references added for recent experimental and theoretical results: the ATLAS measurement on the X(3872) pT distribution in 10-70 GeV; the LHCb measurement on the X(3872) radiative decays; the lattice calculation on X(3872); the small xx resummation method, etc. No changes for the calculated result and the conclusio

    Relativistic Correction to J/\psi Production at Hadron Colliders

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    Relativistic corrections to the color-singlet J/\psi hadroproduction at the Tevatron and LHC are calculated up to O(v^2) in nonrelativistic QCD (NRQCD). The short distance coefficients are obtained by matching full QCD with NRQCD results for the subprocess g+g\to J/\psi+g. The long distance matrix elements are extracted from observed J/\psi hadronic and leptonic decay widths up to O}(v^2). Using the CTEQ6 parton distribution functions, we calculate the LO production cross sections and relativistic corrections for the process p+\bar{p}(p)\to J/\psi+X at the Tevatron and LHC. We find that the enhancement of O(v^2) relativistic corrections to the cross sections over a wide range of large transverse momentum p_t is negligible, only at a level of about 1 %. This tiny effect is due to the smallness of the correction to short distance coefficients and the suppression from long distance matrix elements. These results indicate that relativistic corrections can not help to resolve the large discrepancy between leading order prediction and experimental data for J/\psi production at the Tevatron.Comment: 9 pages, 5 figure

    Cancellation of Infrared Divergences in Hadronic Annihilation Decays of Heavy Quarkonia

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    In the framework of a newly developed factorization formalism which is based on NRQCD, explicit cancellations are shown for the infrared divergences that appeared in the previously calculated hadronic annihilation decay rates of P-wave and D-wave heavy quarkonia. We extend them to a more general case that to leading order in v2v^2 and next-to-leading order in αs\alpha_s, the infrared divergences in the annihilation amplitudes of color-singlet QQˉ(2S+1LJ)Q\bar{Q}(^{2S+1}L_J) pair can be removed by including the contributions of color-octet operators QQˉ(2S+1(L−1)J′)Q\bar{Q}(^{2S+1}(L-1)_{J'}), QQˉ(2S+1(L−3)J′′)Q\bar{Q}(^{2S+1}(L-3)_{J''}), ... in NRQCD. We also give the decay widths of 3DJ→LH^3D_J\rightarrow LH at leading order in αs\alpha_s.Comment: 8 pages, LaTex(3 figures included), to be publishe

    ηc\eta_c production at LHC and indications on the understanding of J/ψJ/\psi production

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    We present a complete evaluation for the prompt ηc\eta_c production at the LHC at next-to-leading order in αs\alpha_s in nonrelativistic QCD. By assuming heavy quark spin symmetry, the recently observed ηc\eta_c production data by LHCb results in a very strong constraint on the upper bound of the color-octet long distance matrix element 1S01S0 of J/ψJ/\psi. We find this upper bound is consistent with our previous study of the J/ψJ/\psi yield and polarization and can give good descriptions for the measurements, but inconsistent with some other theoretical estimates. This may provide important information for understanding the nonrelativistic QCD factorization formulism.Comment: 5 pages, 2 figures, published version in PR

    Regional Ionosphere Mapping and Autonomous Uplink (RIMAU) Satellite Constellation for Space Weather monitoring and nowcasting over Singapore

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    The Regional Ionosphere Mapping and Autonomous Uplink (RIMAU) mission is a constellation of six CubeSats in an equatorial orbit, making Radio Occultation (RO) measurements of the atmosphere and in-situ Ionospheric measurements to characterize the ionosphere over equatorial South-East Asia in near real time. RIMAU builds on the success of the VELOX-CI mission developed and operated at the Satellite Research Centre (SaRC) at Nanyang Technological University, which carried a commercial-off-the-shelf GPS receiver and have been operating successfully since December 2015. RIMAU will carry GPS receivers for RO and an Ionospheric payload, the Compact Ionosphere Probe (CIP) developed by National Central University of Taiwan, consisting of a planar Langmuir probe, retarding potential analyser and Ion trap/drift meter. RIMAU-1 is scheduled to be in operation by 2021 with the full constellation scheduled for flight by 2023. A secondary objective of RIMAU is to provide a Low Earth Orbiting nanosatellite platform for communication with remote sensors in the region. RIMAU-1 will demonstrate communication with remote water sensors monitoring water pollutants and uplink from ground based GPS sensors to adjust the sampling rate for the Ionospheric probe during periods of high scintillation. Understanding the occurrence and impact of Ionospheric irregularities is critically needed for equatorial countries like Singapore. In this paper, we present a novel idea to combine ground based and space based Ionospheric observations to monitor in near-real time the Ionosphere over the Singapore region to characterize Ionospheric disturbances and their impact on communication and navigation systems. The main data products from these measurements will be vertical profiles of the Total Electron Content (TEC) in the ionosphere, atmospheric temperature and humidity profiles in the troposphere. RIMAU TEC measurements will be combined with ground based TEC measurements from ~ 60 GPS receivers in the SE Asia region, operated by the Earth Observatory of Singapore to produce 3D maps of the Ionosphere

    Regional Ionosphere Mapping and Autonomous Uplink (RIMAU) Satellite Constellation for Space Weather monitoring and nowcasting over Singapore

    Get PDF
    The Regional Ionosphere Mapping and Autonomous Uplink (RIMAU) mission is a constellation of six CubeSats in an equatorial orbit, making Radio Occultation (RO) measurements of the atmosphere and in-situ Ionospheric measurements to characterize the ionosphere over equatorial South-East Asia in near real time. RIMAU builds on the success of the VELOX-CI mission developed and operated at the Satellite Research Centre (SaRC) at Nanyang Technological University, which carried a commercial-off-the-shelf GPS receiver and have been operating successfully since December 2015. RIMAU will carry GPS receivers for RO and an Ionospheric payload, the Compact Ionosphere Probe (CIP) developed by National Central University of Taiwan, consisting of a planar Langmuir probe, retarding potential analyser and Ion trap/drift meter. RIMAU-1 is scheduled to be in operation by 2021 with the full constellation scheduled for flight by 2023. A secondary objective of RIMAU is to provide a Low Earth Orbiting nanosatellite platform for communication with remote sensors in the region. RIMAU-1 will demonstrate communication with remote water sensors monitoring water pollutants and uplink from ground based GPS sensors to adjust the sampling rate for the Ionospheric probe during periods of high scintillation. Understanding the occurrence and impact of Ionospheric irregularities is critically needed for equatorial countries like Singapore. In this paper, we present a novel idea to combine ground based and space based Ionospheric observations to monitor in near-real time the Ionosphere over the Singapore region to characterize Ionospheric disturbances and their impact on communication and navigation systems. The main data products from these measurements will be vertical profiles of the Total Electron Content (TEC) in the ionosphere, atmospheric temperature and humidity profiles in the troposphere. RIMAU TEC measurements will be combined with ground based TEC measurements from ~ 60 GPS receivers in the SE Asia region, operated by the Earth Observatory of Singapore to produce 3D maps of the Ionosphere

    Gluonic and leptonic decays of heavy quarkonia and the determination of αs(mc)\alpha_s(m_c) and αs(mb)\alpha_s(m_b)

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    QCD running coupling constant αs(mc)\alpha_s(m_c) and αs(mb)\alpha_s(m_b) are determined from heavy quarkonia cc‾c\overline{c} and bb‾b\overline{b} decays. The decay rates of V→3gV\rightarrow 3g and V→e+e−V\rightarrow e^+ e^- for V=J/ψV=J/\psi and Υ\Upsilon are estimated by taking into account both relativistic and QCD radiative corrections. The decay amplitudes are derived in the Bethe-Salpeter formalism, and the decay rates are estimated by using the meson wavefunctions which are obtained with a QCD-inspired inter-quark potential. For the V→3gV\rightarrow 3g decay we find the relativistic correction to be very large and to severely suppress the decay rate. Using the experimental values of ratio R_g\equiv \frac {\Gamma (V\longrightarrow 3g)}% {\Gamma (V\longrightarrow e^{+}e^{-})}\approx 10,~32 for V=J/ψ, ΥV=J/\psi, ~\Upsilon respectively, and the calculated widths , we find αs(mc)=0.29±0.02\alpha_{s}(m_c)=0.29\pm 0.02 and αs(mb)=0.20±0.02\alpha_s(m_b)=0.20\pm 0.02. These values for the QCD running coupling constant are substantially enhanced, as compared with the ones obtained without relativistic corrections, and are consistent with the QCD scale parameter ΛMS‾(4)\Lambda_{\overline {MS}}^{(4)}% \approx 200MeV. We also find that these results are mainly due to kinematic corrections and not sensitive to the dynamical models.Comment: 15 pages in Late
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