PaperPanorama

Nuclear Theory·nucl-th

Thursday·February 9, 2023

7 papers3 primary·4 cross-listed

  1. 04

    Hadronic structure on the light-front VII. Pions and kaons and their partonic distributions

    Wei-Yang Liu🇺🇸 · Edward Shuryak🇺🇸 · Ismail Zahed🇺🇸

    This work is a continuation in our series of papers, that addresses quark models of hadronic structure on the light front, motivated by the QCD vacuum structure and lattice results. The spontaneous breaking of chiral symmetry on the light front, is shown to parallel that in the rest frame, where the non-local instanton induced t Hooft interaction plays a central role. By rewriting this interaction solely in terms of the good component of the fermionic field, a scalar chiral condensate emerges in the mean-field approximation, which is identical to the one obtained in the rest frame. The pions and kaons emerge as deeply bound Goldstone modes in the chiral limit, with the scalar-isoscalar sigma meson mode as a threshold state with zero binding. We explicitly derive the light front distribution amplitudes (DAs) and partonic functions (PDFs) for these mesons. The DAs and PDFs are in good agreement with those extracted from the QCD instanton vacuum in the rest frame, using the large momentum effective theory (LaMET). The QCD evolved DAs and PDFs compare well with available measurements, as well as recent lattice results.

    hep-phnucl-thPRD(2023)·18 citations
  2. 05

    -mode of neutron stars in pseudo-Newtonian gravity

    Hong-Bo Li · Yong Gao · Lijing Shao · Renxin Xu

    The equation of state (EOS) of nuclear dense matter plays a crucial role in many astrophysical phenomena associated with neutron stars (NSs). Fluid oscillations are one of the most fundamental properties therein. NSs support a family of gravity -modes, which are related to buoyancy. We study the gravity -modes caused by composition gradient and density discontinuity in the framework of pseudo-Newtonian gravity. The mode frequencies are calculated in detail and compared with Newtonian and general-relativistic (GR) solutions. We find that the -mode frequencies in one of the pseudo-Newtonian treatments can approximate remarkably well the GR solutions, with relative errors in the order of . Our findings suggest that, with much less computational cost, pseudo-Newtonian gravity can be utilized to accurately analyze oscillation of NSs constructed from an EOS with a first-order phase transition between nuclear and quark matter, as well as to provide an excellent approximation of GR effects in core-collapse supernova (CCSN) simulations.

    gr-qcastro-ph.HEnucl-thPRD(2023)·4 citations
  3. 06

    Thermodynamic and hydrodynamic characteristics of interacting system formed in relativistic heavy ion collisions

    Xu-Hong Zhang🇨🇳 · Hao-Ning Wang🇨🇳 · Fu-Hu Liu🇨🇳 · Khusniddin K. Olimov🇺🇿

    To study the energy-dependent characteristics of thermodynamic and hydrodynamic parameters, based on the framework of a multi-source thermal model, we analyze the soft transverse momentum () spectra of the charged particles (, , , , , and ) produced in gold-gold (Au-Au) collisions at the center-of-mass energies , 11.5, 14.5, 19.6, 27, 39, 62.4, and 200 GeV from the STAR Collaboration and in lead-lead (Pb-Pb) collisions at and 5.02 TeV from the ALICE Collaboration. In the rest framework of emission source, the probability density function obeyed by meson momenta satisfies the Bose-Einstein distribution, and that obeyed by baryon momenta satisfies the Fermi-Dirac distribution. To simulate the of the charged particles, the kinetic freeze-out temperature and transverse expansion velocity of emission source are introduced into the relativistic ideal gas model. Our results, based on the Monte Carlo method for numerical calculation, show a good agreement with the experimental data. The excitation functions of thermodynamic parameter and hydrodynamic parameter are then obtained from the analyses, which shows an increase tendency from 7.7 GeV to 5.02 TeV in collisions with different centralities.

    hep-phhep-exnucl-exnucl-thIJMPE(2023)·1 citation
  4. 07

    Study of with unitarized coupled channel scattering amplitudes

    Shi-Qing Kuang🇨🇳 · Qi Zhou🇨🇳 · Di Guo🇨🇳 · Qin-He Yang🇨🇳 · Ling-Yun Dai🇨🇳

    In this paper, we study the resonant state . The scattering amplitudes of coupled channels, --, are constructed with the interaction of four vector mesons described by effective Lagrangians. The amplitudes are calculated up to one loop, decomposed by partial wave projection, and unitarized by Pad approximation. These amplitudes are fitted to the latest experimental data sets of di- and invariant mass spectra of LHCb, CMS, and ATLAS. High-quality solutions are obtained. With these partial wave amplitudes, we extract the pole parameters of the . Its quantum number is likely to be . According to the pole counting rule as well as analysis of the phase shifts of the partial waves, it supports our previous conclusion that the prefers to be a compact tetra-quark.

    hep-phnucl-thEPJC(2023)·30 citations

Affiliations

first authorsco-authorsvia INSPIRE