PaperPanorama

Nuclear Theory·nucl-th

Thursday·August 18, 2016

9 papers4 primary·5 cross-listed

  1. 01

    Leading-twist distribution amplitudes of scalar- and vector-mesons

    Bo-Lin Li🇨🇳 · Lei Chang🇨🇳 · Minghui Ding🇨🇳 · Craig D. Roberts🇺🇸 · Hong-Shi Zong🇨🇳

    A symmetry-preserving truncation of the two-body light-quark bound-state problem in relativistic quantum field theory is used to calculate the leading-twist parton distribution amplitudes (PDAs) of scalar systems, both ground-state and radial excitations, and the radial excitations of vector mesons. Owing to the fact that the scale-independent leptonic decay constant of a scalar meson constituted from equal-mass valence-constituents vanishes, it is found that the PDA of a given scalar system possesses one more zero than that of an analogous vector meson. Consequently, whereas the mean light-front relative momentum of the valence-constituents within a vector meson is zero, that within a scalar meson is large, an outcome which hints at a greater role for light-front angular momentum in systems classified as -wave in quantum mechanical models. Values for the scale-dependent decay constants of ground-state scalar and vector systems are a by-product of this analysis, and they turn out to be roughly equal, viz. GeV at an hadronic scale. In addition, it is confirmed that the dilation characterising ground-state PDAs is manifest in the PDAs of radial excitations too. The impact of -flavour symmetry breaking is also considered. When compared with pseudoscalar states, it is a little stronger in scalar systems, but the size is nevertheless determined by the flavour-dependence of dynamical chiral symmetry breaking and the PDAs are still skewed toward the heavier valence-quark in asymmetric systems.

    nucl-thhep-lathep-phnucl-exPRD(2016)·26 citations
  2. 02

    Pion transverse-momentum spectrum, elliptic flow, and Hanbury-Brown-Twiss interferometry in a viscous granular source model

    Jing Yang🇨🇳 · Wei-Ning Zhang🇨🇳 · Yan-Yu Ren🇨🇳

    We examine the evolution of quark-gluon plasma (QGP) droplets with viscous hydrodynamics and analyze the pion transverse-momentum spectrum, elliptic flow, and Hanbury-Brown-Twiss (HBT) interferometry in a granular source model consisting of viscous QGP droplets. The shear viscosity of the QGP droplet speeds up and slows down the droplet evolution in the central and peripheral regions of the droplet, respectively. The effect of the bulk viscosity on the evolution is negligible. Although there are viscous effects on the droplet evolution, the pion momentum spectrum and elliptic flow change little for granular sources with and without viscosity. On the other hand, the influence of viscosity on HBT radius is considerable. It makes decrease in the granular source model. We determine the model parameters of granular sources using the experimental data of pion transverse-momentum spectrum, elliptic flow, and HBT radii together, and investigate the effects of viscosity on the model parameters. The results indicate that the granular source model may reproduce the experimental data of pion transverse-momentum spectrum, elliptic flow, and HBT radii in heavy-ion collisions of Au-Au at GeV and Pb-Pb at TeV in different centrality intervals. The viscosity of the droplet leads to an increase in the initial droplet radius and a decrease of the source shell parameter in the granular source model.

    nucl-thCPC(2017)·3 citations
  3. 03

    Impact of Nucleon-Nucleon Bremsstrahlung Rates Beyond One-Pion Exchange

    Alexander Bartl · Robert Bollig · Hans-Thomas Janka · Achim Schwenk

    Neutrino-pair production and annihilation through nucleon-nucleon bremsstrahlung is included in current supernova simulations by rates that are based on the one-pion-exchange approximation. Here we explore the consequences of bremsstrahlung rates based on a modern nuclear interactions for proto-neutron star cooling and the corresponding neutrino emission. We find that despite a reduction of the bremsstrahlung emission by a factor of 2-5 in the neutrinospheric region, models with the improved treatment exhibit only 5% changes of the neutrino luminosities and an increase of 0.7 MeV of the average energies of the radiated neutrino spectra, with the largest effects for the antineutrinos of all flavors and at late times. Overall, the proto-neutron star cooling evolution is slowed down modestly by 0.5-1 s.

    nucl-thastro-ph.HEastro-ph.SRPRD(2016)·38 citations
  4. 04

    A dynamical -cluster model of O

    C. J. Halcrow · C. King · N. S. Manton

    We calculate the low-lying spectrum of the O nucleus using an -cluster model which includes the important tetrahedral and square configurations. Our approach is motivated by the dynamics of -particle scattering in the Skyrme model. We are able to replicate the large energy splitting that is observed between states of identical spin but opposite parities, as well as introduce states that were previously not found in other cluster models, such as a state. We also provide a novel interpretation of the first excited state of O and make predictions for the energies of states that have yet to be observed experimentally.

    nucl-thhep-thPRC(2017)·71 citations

Affiliations

first authorsco-authorsvia INSPIRE