PaperPanorama

Nuclear Theory·nucl-th

Tuesday·April 20, 2021

9 papers2 primary·7 cross-listed

  1. 01

    Proton correlations and apparent intermittency in the UrQMD model with hadronic potentials

    Pengcheng Li🇨🇳 · Yongjia Wang🇨🇳 · Jan Steinheimer🇩🇪 · Qingfeng Li🇨🇳 · Hongfei Zhang🇨🇳

    It is shown that the inclusion of hadronic interactions, and in particular nuclear potentials, in simulations of heavy ion collisions at the SPS energy range can lead to obvious correlations of protons. These correlations contribute significantly to an intermittency analysis as performed at the NA61 experiment. The beam energy and system size dependence is studied by comparing the resulting intermittency index for heavy ion collisions of different nuclei at beam energies of , and GeV. The resulting intermittency index from our simulations is similar to the reported values of the NA61 collaboration, if nuclear interactions are included. The observed apparent intermittency signal is the result of the correlated proton pairs with small relative transverse momentum , which would be enhanced by hadronic potentials, and this correlation between the protons is slightly influenced by the coalescence parameters and the relative invariant four-momentum cut.

    nucl-thPLB(2021)·15 citations
  2. 02

    Equation of state of asymmetric nuclear matter and the tidal deformability of neutron star

    Ngo Hai Tan🇻🇳 · Dao T. Khoa🇻🇳 · Doan Thi Loan🇻🇳

    Neutron star (NS) is a unique astronomical compact object where the four fundamental interactions have been revealed from the observation and studied in different ways. While the macroscopic properties of NS like mass and radius can be determined within the General Relativity using a realistic equation of state (EOS) of NS matter, such an EOS is usually generated by a nuclear structure model like, e.g., the nuclear mean-field approach to asymmetric nuclear matter. Given the radius of NS extended to above 10 km and its mass up to twice the solar mass, NS is expected to be tidally deformed when it is embedded in a strong tidal field. Such a tidal effect was confirmed unambiguously in the gravitation wave signals detected recently by the LIGO and Virgo laser interferometers from GW170817, the first ever direct observation of a binary NS merger. A nonrelativistic mean-field study is carried out in the present work within the Hartree-Fock formalism to construct the EOS of NS matter, which is then used to determine the tidal deformability, gravitational mass, and radius of NS. The mean-field results are compared with the constraints imposed for these quantities by the global analysis of the observed GW170817 data, and a strong impact by the incompressibility of nuclear matter on the hydrostatic configuration of NS is shown.

    nucl-thnucl-exEPJA(2021)·7 citations

Affiliations

first authorsco-authorsvia INSPIRE