PaperPanorama

Nuclear Theory·nucl-th

Wednesday·December 9, 2015

4 papers3 primary·1 cross-listed

  1. 01

    QMC approach based on the Bogoliubov independent quark model of the nucleon

    Henrik Bohr🇩🇰 · Steven A. Moszkowski🇺🇸 · Prafulla K. Panda🇮🇳 · Constanca Providencia🇵🇹 · Joao da Providencia🇵🇹

    The quark-meson coupling model due to Guichon is formulated on the basis of the independent quark model of the nucleon proposed by Bogoliubov and is applied to the phenomenological descriptions of symmetric and asymmetric nuclear matter. For symmetric matter, the model predicts, at saturation density, the incompressibility MeV, the quark effective mass MeV, and the effective nucleon mass where is the nucleon mass in vacuum. Neutron star massesabove two solar masses are obtained.

    nucl-thIJMPE(2016)·10 citations
  2. 02

    Nuclear symmetry energy in a modified quark meson coupling model

    R.N. Mishra🇮🇳 · H.S. Sahoo🇮🇳 · P.K. Panda🇮🇳 · N. Barik🇮🇳 · T. Frederico🇧🇷

    We study nuclear symmetry energy and the thermodynamic instabilities of asymmetric nuclear matter in a self-consistent manner by using a modified quark-meson coupling model where the confining interaction for quarks inside a nucleon is represented by a phenomenologically averaged potential in an equally mixed scalar-vector harmonic form. The nucleon-nucleon interaction in nuclear matter is then realized by introducing additional quark couplings to , , and mesons through mean-field approximations. We find an analytic expression for the symmetry energy as a function of its slope . Our result establishes a linear correlation between and . We also analyze the constraint on neutron star radii in matter with equilibrium.

    nucl-thPRC(2015)·28 citations

Affiliations

first authorsco-authorsvia INSPIRE