PaperPanorama

Nuclear Theory·nucl-th

Friday·August 9, 2024

7 papers2 primary·5 cross-listed

  1. 01

    Charmed hypernuclei within density-dependent relativistic mean-field theory

    Wei Yang🇨🇳 · Shi Yuan Ding🇨🇳 · Bao Yuan Sun🇨🇳

    The charmed hypernuclei are investigated within the framework of the density-dependent relativistic mean-field (DDRMF) theory. Starting from the empirical hyperon potential in symmetric nuclear matter, obtained through microscopic first-principle calculations, two sets of effective interactions were derived by fitting the potentials with minimal uncertainty (Fermi momentum ) and near saturation density (). These DDRMF models were then used to explore the effective interaction uncertainties on the description of hypernuclear bulk and single-particle properties. A systematic investigation was conducted on the existence of bound hypernuclei. The dominant factors affecting the existence and stability of hypernuclei were analyzed from the perspective of the potential. It is found that the hyperon potential is not only influenced by the Coulomb repulsion, but by an extra contribution from the rearrangement terms due to the density dependence of the meson-baryon coupling strengths. Therefore, the rearrangement term significantly impacts the stability description for light hypernuclei, while for heavier hypernuclei, the contribution from Coulomb repulsion becomes increasingly significant and eventually dominant. The discussion then delves into the bulk and single-particle properties of charmed hypernuclei using these models. It is found that even when different models yield similar hyperon potentials for nuclear matter, different treatments of nuclear medium effects could lead to disparities in the theoretical description of hypernuclear structures. This study indicates that constraints on the interaction at finite densities are crucial for the study of hypernuclear structures.

    nucl-thPRC(2024)·4 citations
  2. 02

    Convergence properties of -Expansion Scheme: Hadron Resonance Gas and Cluster Expansion Model

    Micheal Kahangirwe🇺🇸 · Irene Gonzalez🇺🇸 · Jorge A. Muñoz🇺🇸 · Claudia Ratti🇺🇸 · Volodymyr Vovchenko🇺🇸

    In this study, we assess the effectiveness and robustness of the recently proposed -expansion scheme for expanding the equation of state of strongly interacting matter to finite density, by comparing its performance relative to the conventional Taylor expansion method in various effective QCD models. We use baryon number density and its susceptibilities to calculate the expansion coefficients in the -expansion scheme with and without the Stefan-Boltzmann limit correction. Our methodology involves comparing truncation orders to exact solutions to assess the scheme's accuracy. We utilize Ideal, Excluded Volume, and van der Waals formulations of the Hadron Resonance Gas (HRG) model at low temperatures, and the Cluster Expansion Model at higher temperatures. Our findings indicate that the -expansion scheme offers superior convergence properties near and above the chiral crossover temperature, where the chiral-criticality-inspired scaling holds. However, it shows limited improvement in the HRG models, indicating that it may not be the most suitable choice for describing the hadronic phase.

    nucl-thPRD(2025)·10 citations

Affiliations

first authorsco-authorsvia INSPIRE