PaperPanorama

Nuclear Theory·nucl-th

Thursday·December 22, 2016

12 papers3 primary·9 cross-listed

  1. 01

    Pre-equilibrium effects in charge-asymmetric low-energy reactions

    H. Zheng · S. Burrello · M. Colonna · V. Baran

    We study the pre-equilibrium dipole response in the charge-asymmetric reaction Sn+Ni at MeV/A, within a semi-classical transport model employing effective interactions for the nuclear mean-field. In particular, we adopt the recently introduced SAMi-J Skyrme interactions, whose parameters are specifically tuned to improve the description of spin-isospin properties of nuclei. Within the same framework, we also discuss pre-equilibrium nucleon emission. Our results show that both mechanisms, i.e., pre-equilibrium dipole oscillations and nucleon emission, are sensitive to the symmetry energy below the saturation density (in the range ), to the effective mass and to the nucleon-nucleon cross section. Finally, a covariant analysis is applied to study the correlations between the model parameters and observables of experimental interest.

    nucl-thPLB(2017)·15 citations
  2. 02

    Comparison of equation of state models with different cluster dissolution mechanisms

    Helena Pais🇵🇹 · Stefan Typel🇩🇪

    The appearance of nuclear clusters in stellar matter at densities below nuclear saturation is an important feature in the modeling of the equation of state for astrophysical applications. There are different theoretical concepts to describe the dissolution of nuclei with increasing density and temperature. In this contribution, the predictions of two approaches are compared: the medium dependent change of the nuclear masses in a generalized relativistic density functional approach and the excluded-volume mechanism in a statistical model. Both approaches use the same description for the interaction between the nucleons. The composition of neutron star matter, in particular the occurrence of light and heavy nuclei, and its thermodynamic properties are studied.

    nucl-thastro-ph.SR9 citations
  3. 03

    Compact bifluid hybrid stars: Hadronic Matter mixed with self-interacting fermionic Asymmetric Dark Matter

    Somnath Mukhopadhyay🇮🇳 · Debasis Atta🇮🇳 · Kouser Imam🇮🇳 · D. N. Basu🇮🇳 · C. Samanta🇺🇸

    The masses and radii of non-rotating and rotating configurations of pure hadronic stars mixed with self-interacting fermionic Asymmetric Dark Matter are calculated within the two-fluid formalism of stellar structure equations in general relativity. The Equation of State (EoS) of nuclear matter is obtained from the density dependent M3Y effective nucleon-nucleon interaction. We consider dark matter particle mass of 1 GeV. The EoS of self-interacting dark matter is taken from two-body repulsive interactions of the scale of strong interactions. We explore the conditions of equal and different rotational frequencies of nuclear matter and dark matter and find that the maximum mass of differentially rotating stars with self-interacting dark matter to be with radius kms.

    nucl-thEPJC(2017)·52 citations

Affiliations

first authorsco-authorsvia INSPIRE