PaperPanorama

Nuclear Theory·nucl-th

Wednesday·August 16, 2017

8 papers5 primary·3 cross-listed

  1. 01

    [Submitted on 15 Aug 2017]

    The symmetry energy in nucleon and quark matter

    Lie-Wen Chen🇨🇳

    The symmetry energy characterizes the isospin dependent part of the equation of state of isospin asymmetric strong interaction matter and it plays a critical role in many issues of nuclear physics and astrophysics. In this talk, we briefly review the current status on the determination of the symmetry energy in nucleon (nuclear) and quark matter. For nuclear matter, while the subsaturation density behaviors of the symmetry energy are relatively well-determined and significant progress has been made on the symmetry energy around saturation density, the determination of the suprasaturation density behaviors of the symmetry energy remains a big challenge. For quark matter, which is expected to appear in dense matter at high baryon densities, we briefly review the recent work about the effects of quark matter symmetry energy on the properties of quark stars and the implication of possible existence of heavy quark stars on quark matter symmetry energy. The results indicate that the and quarks could feel very different interactions in isospin asymmetric quark matter, which may have important implications on the isospin effects of partonic dynamics in relativistic heavy-ion collisions.

    Comments:
    8 pages, 5 figures. Invited talk given at 2016 Dalian International Workshop on Nuclear Physics (2016DIWNP), July 20-23, 2016, Dalian, China
    Subjects:
    Nuclear Theory (nucl-th); High Energy Astrophysical Phenomena (astro-ph.HE); High Energy Physics — Phenomenology (hep-ph); Nuclear Experiment (nucl-ex)
    arXiv:
    1708.04433 [pdf]
    Nucl.Phys.Rev.(2017)·32 citations
  2. 02

    [Submitted on 15 Aug 2017]

    From quark and nucleon correlations to discrete symmetry and clustering in nuclei

    Genis Musulmanbekov🇷🇺

    Starting with a quark model of nucleon structure in which the valence quarks are strongly correlated within a nucleon, the light nuclei are constructed by assuming similar correlations of the quarks of neighboring nucleons. Applying the model to larger collections of nucleons reveals the emergence of the face-centered cubic (FCC) symmetry at the nuclear level. Nuclei with closed shells possess octahedral symmetry. Binding of nucleons are provided by quark loops formed by three and four nucleon correlations. Quark loops are responsible for formation of exotic (borromean) nuclei, as well. The model unifies independent particle (shell) model, liquid-drop and cluster models.

    Comments:
    12 pages, 4 figures. Presented at Int. Symp. "Exotic Nuclei - Exon 2016"
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    1708.04437 [pdf]
    Exotic Nuclei (World Scientific, 2016), p…·0 citations
  3. 03

    [Submitted on 15 Aug 2017]

    Open charm production in central Pb+Pb collisions at the CERN SPS: statistical model estimates

    R. V. Poberezhnyuk🇺🇦 · M. Gazdzicki🇵🇱 · M. I. Gorenstein🇺🇦

    Charm particle production in nucleus-nucleus collisions at the CERN SPS energies is considered within a statistical approach. Namely, the Statistical Model of the Early Stage is used to calculate mean multiplicity of charm particles in central Pb+Pb collisions. A small number of produced charm particles necessitates the use of the exact charm conservation law. The model predicts a rapid increase of mean charm multiplicity as a function of collision energy. The mean multiplicity calculated for central Pb+Pb collisions at the center of mass energy per nucleon pair GeV exceeds significantly the experimental upper limit. Thus, in order to describe open charm production model parameters and/or assumptions should be revised.

    Comments:
    8 pages, 7 figures
    Subjects:
    Nuclear Theory (nucl-th); High Energy Physics — Phenomenology (hep-ph)
    arXiv:
    1708.04491 [pdf]
    Acta Phys.Polon.B(2017)·12 citations
  4. 04

    [Submitted on 11 Aug 2017]

    Addendum: Muon-neutrino-induced charged current pion production

    U. Mosel🇩🇪 · K. Gallmeister🇩🇪

    This short paper is an addendum to a recent publication on charged current neutrino-induced pion production (Phys.\ Rev.\ C96 (2017) no.1, 015503). It presents comparisons of pion production cross sections measured at the T2K near detector for a CH target.

    Comments:
    Addendum to, "Muon-neutrino-induced charged current pion production on nuclei". U. Mosel, K. Gallmeister. Version 1 of this present addendum was uploaded to the arXiv in August 2017. Now data points, that have become available in the meantime, have been added into the figures. Title changed for version accepted for publication in Phys. Rev. C
    Subjects:
    Nuclear Theory (nucl-th); High Energy Physics — Experiment (hep-ex); Nuclear Experiment (nucl-ex)
    arXiv:
    1708.04528 [pdf]
    PRC(2017)·31 citations
  5. 05

    [Submitted on 12 Aug 2017]

    Existence of inelastic supernumerary nuclear rainbow in O+C scattering

    S. Ohkubo · Y. Hirabayashi · A. A. Ogloblin

    The existence of a supernumerary nuclear rainbow in inelastic scattering is reported. This is done by studying inelastic O scattering from C, exciting the (4.44 MeV) state of C and elastic scattering at the incident energies in the range 124 to 200 MeV, using the coupled channels method. An extended double folding potential is used. This is derived from realistic wave functions for C and O calculated with a microscopic cluster model and a finite-range density-dependent nucleon-nucleon force. Excitations to the (4.44 MeV), 3 (9.64 MeV) and (14.08 MeV) states of C, and the (6.13 MeV) and (6.92 MeV) states of O are included in the coupled channels calculations. The emergence of the supernumerary bow is understood by the properties of both the Luneburg-lens-like potential in the internal region and diffuse attraction in the outer region. The existence of a supernumerary rainbow for inelastic scattering in addition to the existence of a dynamically created secondary rainbow and a dynamically refracted primary rainbow for elastic scattering, which are not observed in meteorological rainbows, further deepens the understanding of nuclear rainbows.

    Comments:
    6 pages, 5 figures. arXiv admin note: text overlap with arXiv:1412.7239
    Subjects:
    Nuclear Theory (nucl-th); Nuclear Experiment (nucl-ex)
    arXiv:
    1708.04533 [pdf]
    PRC(2017)·3 citations
  6. 06

    [Submitted on 14 Aug 2017] (cross-list from cond-mat.mes-hall)

    Anomalous thermoelectric phenomena in lattice models of multi-Weyl semimetals

    E. V. Gorbar · V. A. Miransky · I. A. Shovkovy · P. O. Sukhachov

    The thermoelectric transport coefficients are calculated in a generic lattice model of multi-Weyl semimetals with a broken time-reversal symmetry by using the Kubo's linear response theory. The contributions connected with the Berry curvature-induced electromagnetic orbital and heat magnetizations are systematically taken into account. It is shown that the thermoelectric transport is profoundly affected by the nontrivial topology of multi-Weyl semimetals. In particular, the calculation reveals a number of thermal coefficients of the topological origin which describe the anomalous Nernst and thermal Hall effects in the absence of background magnetic fields. Similarly to the anomalous Hall effect, all anomalous thermoelectric coefficients are proportional to the integer topological charge of the Weyl nodes. The dependence of the thermoelectric coefficients on the chemical potential and temperature is also studied.

    Comments:
    20 pages, 13 multi-panel figures; published version
    Subjects:
    Mesoscale and Nanoscale Physics (cond-mat.mes-hall); Nuclear Theory (nucl-th)
    arXiv:
    1708.04248 [pdf]
    PRB(2017)·34 citations
  7. 07

    [Submitted on 14 Aug 2017] (cross-list from hep-ph)

    The Role of QCD Monopoles in Jet Quenching

    Adith Ramamurti🇺🇸 · Edward Shuryak🇺🇸

    QCD monopoles are magnetically charged quasiparticles whose Bose-Einstein condensation (BEC) at creates electric confinement and flux tubes. The "magnetic scenario" of QCD proposes that scattering on the non-condensed component of the monopole ensemble at is responsible for the unusual kinetic properties of QGP. In this paper, we study the contribution of the monopoles to jet quenching phenomenon, using the BDMPS framework and hydrodynamic backgrounds. In the lowest order for cross sections, we calculate the nuclear modification factor, and azimuthal anisotropy, , of jets, as well as the dijet asymmetry, , and compare those to the available data. We find relatively good agreement with experiment when using realistic hydrodynamic backgrounds. In addition, we find that event-by-event fluctuations are not necessary to reproduce and data, but play a role in . Since the monopole-induced effects are maximal at , we predict that their role should be significantly larger, relative to quarks and gluons, at lower RHIC energies.

    Comments:
    17 pages, 15 figures
    Subjects:
    High Energy Physics — Phenomenology (hep-ph); Nuclear Theory (nucl-th)
    arXiv:
    1708.04254 [pdf]
    PRD(2018)·14 citations
  8. 08

    [Submitted on 15 Aug 2017] (cross-list from hep-ph)

    Mass spectra and radiative transitions of doubly heavy baryons in a relativized quark model

    Qi-Fang Lü🇨🇳 · Kai-Lei Wang🇨🇳 · Li-Ye Xiao🇨🇳 · Xian-Hui Zhong🇨🇳

    We study the mass spectra and radiative decays of doubly heavy baryons within the diquark picture in a relativized quark model. The mass of the ground state is predicted to be 3606 MeV, which is consistent with the mass of newly observed by the LHCb collaboration. The predicted mass gap between two wave states, () and (), is 69 MeV. Furthermore, the radiative transitions of doubly heavy baryons are also estimated by using the realistic wave functions obtained from relativized quark model. The radiative decay widths of and are predicted to be about 7 and 4 keV, respectively. These predictions of doubly heavy baryons can provide helpful information for future experimental searches.

    Comments:
    8 pages, 2 figure. The size effects of the diquarks are considered. Version accepted by Phys. Rev. D
    Subjects:
    High Energy Physics — Phenomenology (hep-ph); High Energy Physics — Experiment (hep-ex); Nuclear Theory (nucl-th)
    arXiv:
    1708.04468 [pdf]
    PRD(2017)·119 citations

Affiliations

first authorsco-authorsvia INSPIRE