PaperPanorama

Nuclear Theory·nucl-th

Wednesday·August 8, 2018

9 papers4 primary·5 cross-listed

  1. 01

    Estimating initial state and quark-gluon plasma medium properties using a hybrid model with nucleon substructure calibrated to -Pb and Pb-Pb collisions at TeV

    J. Scott Moreland🇺🇸 · Jonah E. Bernhard🇺🇸 · Steffen A. Bass🇺🇸

    We posit a unified hydrodynamic and microscopic description of the quark-gluon plasma (QGP) produced in ultrarelativistic -Pb and Pb-Pb collisions at TeV and evaluate our assertion using Bayesian inference. Specifically, we model the dynamics of both collision systems using initial conditions with parametric nucleon substructure, a pre-equilibrium free-streaming stage, event-by-event viscous hydrodynamics, and a microscopic hadronic afterburner. Free parameters of the model which describe the initial state and QGP medium are then simultaneously calibrated to fit charged particle yields, mean , and flow cumulants. We argue that the global agreement of the calibrated model with the experimental data strongly supports the existence of hydrodynamic flow in small collision systems at ultrarelativistic energies, and that the flow produced develops at length scales smaller than a single proton. Posterior estimates for the model's input parameters are obtained, and new insights into the temperature dependence of the QGP transport coefficients and event-by-event structure of the proton are discussed.

    nucl-thnucl-exPRC(2020)·168 citations
  2. 02

    Strangeness and resonance in compact stars with relativistic-mean-field models

    Ting-Ting Sun🇨🇳 · Shi-Sheng Zhang🇨🇳 · Qiu-Lan Zhang🇨🇳 · Cheng-Jun Xia🇨🇳

    We explore the effects of strangeness and resonance in baryonic matter and compact stars within the relativistic-mean-field (RMF) models. The covariant density functional PKDD is adopted for - interaction, parameters fixed based on finite hypernuclei and neutron stars are taken for the hyperon-meson couplings, and the universal baryon-meson coupling scheme is adopted for the -meson couplings. In light of the recent observations of GW170817 with the dimensionless combined tidal deformability , we find it is essential to include the resonances in compact stars, and small - coupling is favored if the mass of PSR J2215+5135 is confirmed.

    nucl-thastro-ph.HEPRD(2019)·42 citations
  3. 03

    Short-range and tensor correlations in 4He and 8Be studied with antisymmetrized quasi cluster model

    N. Itagaki🇯🇵 · H. Matsuno🇯🇵 · Y. Kanada-En'yo🇯🇵

    We apply tensor version of antisymmetrized quasi cluster model (AQCM-T) to 4He and 8Be while focusing on the NN correlations in alpha clusters. We adopt the NN interactions including realistic ones containing a repulsive core for the central part in addition to the tensor part. In 4He, the pn pair in the 3D channel has been known to play a decisive role in the tensor correlation and the framework is capable of treating not only this channel but also the NN correlations in the 1S and 3S channels. In 8Be, when two alpha clusters approach, the 3D pair is suppressed because of the Pauli blocking effect, which induces the decrease of the 3S component through the 3S-3D coupling. This effect results in the reduction of the attractive effect of the central-even interaction in the middle-range region.

    nucl-thPTEP(2019)·4 citations
  4. 04

    Nuclear systems under extreme conditions: isospin asymmetry and strong B-fields

    Martin Stein🇩🇪

    This thesis explores nuclear systems under extreme conditions of isospin asymmetry and strong magnetic fields. Its first chapter is devoted to the phase diagram of isospin-asymmetrical nuclear matter in the density-temperature plane. Four competing phases of matter are included into the consideration: the unpaired phase, the ordinary Bardeen-Cooper-Schrieffer (BCS) phase, a phase where normal fluid and superfluid separate into distinct domains and the superfluid phase with a non-zero total momentum of Cooper pairs. The evolution of these phases from the weakly BCS limit to the strongly coupled Bose-Einstein-Condensate limit is studied by varying the density from high to low values at various temperatures and asymmetries. The emergence of tri-critical points (including a Lifshitz point) and various intrinsic properties of the condensate (pair wave-function, occupation numbers, quasiparticle spectra) are discussed. The second chapter studies the nuclei C, O, and Ne in a magnetic field G by utilizing the SKY3D code, suitably extended to include the magnetic field. Our solutions of time-independent Hartree-Fock equations on a Cartesian three-dimensional grid with a Skyrme interaction demonstrate a number of interesting phenomena, such as level splitting in the magnetic field, spontaneous rearrangement of energy levels, changes in the nuclear shape, etc. The third chapter studies the pairing in low-density neutron matter in the presence of a strong magnetic field. In particular, we find the limiting field for the destruction of the superfluidity of neutrons in the crust and outer core of magnetars. This field is density-dependent but is generally of the order of G. The phase diagram of spin-polarized neutron matter is constructed in the case where only the BCS phase is allowed along with the (spin-polarized) normal phase.

    nucl-th0 citations

Affiliations

first authorsco-authorsvia INSPIRE