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相关论文: Phenomenological implications of the nucleon's mes…

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The predictions for the atmospheric neutrino flux at high energies strongly depend on the contribution of prompt neutrinos, which are determined by the production of charmed meson in the atmosphere at very forward rapidities. Here we…

高能物理 - 唯象学 · 物理学 2021-07-30 Rafal Maciula , Victor P. Goncalves , Antoni Szczurek

We investigate the charm sector of the nucleon structure phenomenologically, using the most up-to-date global QCD analysis. Going beyond the common assumption of purely radiatively generated charm, we explore possible degrees of freedom in…

高能物理 - 唯象学 · 物理学 2008-11-26 J. Pumplin , H. L. Lai , W. K. Tung

The predictions for the atmospheric neutrino flux at high energies strongly depend on the contribution of prompt neutrinos, which are determined by the production of charmed meson in the atmosphere at very forward rapidities. In this paper…

高能物理 - 唯象学 · 物理学 2022-04-13 Victor P. Goncalves , Rafal Maciula , Antoni Szczurek

We present the results of a recent analysis to study the nucleon's charm sigma term, $\sigma_{c\overline{c}}$. We construct a minimal model in terms of light-front variables and constrain the range of possibilities using extant knowledge…

高能物理 - 唯象学 · 物理学 2017-11-01 T. J. Hobbs , Mary Alberg , Gerald A. Miller

Over the past $\sim\!\! 10$ years, the topic of the nucleon's nonperturbative or $\textit{intrinsic}$ charm (IC) content has enjoyed something of a renaissance, largely motivated by theoretical developments involving quark modelers and PDF…

高能物理 - 唯象学 · 物理学 2017-07-07 T. J. Hobbs

We present a new global QCD analysis of parton distribution functions, allowing for possible intrinsic charm (IC) contributions in the nucleon inspired by light-front models. The analysis makes use of the full range of available high-energy…

高能物理 - 唯象学 · 物理学 2015-03-05 P. Jimenez-Delgado , T. J. Hobbs , J. T. Londergan , W. Melnitchouk

We use light-front Holography to estimate the valence quark and the meson cloud contributions to the nucleon axial form factor. The free couplings of the holographic model are determined by the empirical data and by the information…

高能物理 - 唯象学 · 物理学 2018-04-16 G. Ramalho

We perform a comprehensive analysis of the role of nonperturbative (or intrinsic) charm in the nucleon, generated through Fock state expansions of the nucleon wave function involving five-quark virtual states represented by charmed mesons…

高能物理 - 唯象学 · 物理学 2014-04-23 T. J. Hobbs , J. T. Londergan , W. Melnitchouk

Using a $\overline D$ meson cloud model we calculate the squared charm radius of the nucleon . The ratio between this squared radius and the ordinary baryon squared radius is identified with the probability of ``seeing'' the intrinsic charm…

高能物理 - 唯象学 · 物理学 2009-10-28 F. S. NAVARRA , M. NIELSEN , C. A. A. NUNES , M. TEIXEIRA

Nuclei are transparent for a heavy intrinsic charm (IC) component of the beam hadrons, what leads to an enhanced nuclear dependence of open charm production at large Feynman x_F. Indeed, such an effect was observed recently in the SELEX…

高能物理 - 唯象学 · 物理学 2010-03-22 B. Z. Kopeliovich , I. K. Potashnikova , Ivan Schmidt

We explore the meson cloud contribution to nucleon electromagnetic form factors in dispersion relation approach. In our calculations, experimental data on transition amplitudes for pion-nucleon scatterings are taken directly as inputs, with…

高能物理 - 唯象学 · 物理学 2024-09-27 Ek-ong Atthaphan , Attaphon Kaewsnod , Kai Xu , Moh Moh Aung , Warintorn Sreethawong , Ayut Limphirat , Yupeng Yan

In this thesis we explore a diverse array of issues that strike at the inherently nonperturbative structure of hadrons at momenta below the QCD confinement scale. In so doing, we mainly seek a better control over the partonic substructure…

高能物理 - 唯象学 · 物理学 2014-08-26 T. J. Hobbs

We consider an observable very sensitive to the non-zero intrinsic charm (IC) contribution to the proton density. It is the ratio between the differential cross sections of the photon or $Z$-boson and $c$-jet production in the $pp$…

高能物理 - 唯象学 · 物理学 2016-09-28 A. V. Lipatov , G. I. Lykasov , Yu. Yu. Stepanenko , V. A. Bednyakov

The quark-gluon properties of the nucleon are probed by a host of recent and planned experiments. These involve elastic, deep-inelastic, semi-inclusive deep-inelastic (SIDIS), and deeply-virtual Compton scattering. A light-front description…

核理论 · 物理学 2015-05-18 Gerald A. Miller

The all-sky very-high-energy ($10^4-10^6$ GeV) atmospheric muon flux measured by IceCube shows a spectral hardening at the highest energies, indicating the presence of a prompt component. IceCube has also measured the atmospheric muon…

高能物理 - 唯象学 · 物理学 2026-02-03 Laksha Pradip Das , Diksha Garg , Maria Vittoria Garzelli , Mary Hall Reno , Günter Sigl

In this work, we present a new investigation about the impact of intrinsic charm (IC) on the physical observables, in particular, on the heavy structure function $F_2^c$. Since IC distribution is dominant at large Bjorken variable $x$,…

高能物理 - 唯象学 · 物理学 2017-01-25 Alireza Aleedaneshvar , Muhammad Goharipour , Saeedeh Rostami

We study how the electromagnetic structure of the nucleon is influenced by a pion cloud. To this aim we make use of a constituent-quark model with instantaneous confinement and a pion that couples directly to the quarks. To derive the…

核理论 · 物理学 2014-01-30 Daniel Kupelwieser , Wolfgang Schweiger

The pion cloud is important in nuclear physics and in a variety of low-energy hadronic phenomena. We argue that it is natural to expect it to also be important in lepton-proton deep inelastic scattering and Drell-Yan studies of proton…

核理论 · 物理学 2022-07-12 Mary Alberg , Lucas Ehinger , Gerald A. Miller

We have applied the Meson Cloud Model (MCM) to calculate the charm and strange antiquark distribution in the nucleon. The resulting distribution, in the case of charm, is very similar to the intrinsic charm momentum distribution in the…

高能物理 - 唯象学 · 物理学 2009-10-28 S. Paiva , M. Nielsen , F. S. Navarra , F. O. Durães , L. L. Barz

The discovery of extraterrestrial neutrinos in the $\sim$ 30 TeV -- PeV energy range by IceCube provides new constraints on high energy astrophysics. An important background to the signal are the prompt neutrinos which originate from the…

高能物理 - 唯象学 · 物理学 2017-12-08 Ranjan Laha , Stanley J. Brodsky
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