PaperPanorama

Nuclear Theory·nucl-th

Wednesday·March 23, 2016

8 papers5 primary·3 cross-listed

  1. 01

    [Submitted on 21 Mar 2016]

    Consequences of high- proton size fluctuations in small collision systems at RHIC

    D. McGlinchey🇺🇸 · J. L. Nagle🇺🇸 · D. V. Perepelitsa🇺🇸

    Recent measurements of jet production rates at large transverse momentum () in the collisions of small projectiles with large nuclei at RHIC and the LHC indicate that they have an unexpected relationship with estimates of the collision centrality. One compelling interpretation of the data is that it captures an -dependent decrease in the average interaction strength of the nucleon in the projectile undergoing a hard scattering. A weakly interacting or "shrinking" nucleon in the projectile strikes fewer nucleons in the nucleus, resulting in a particular pattern of centrality-dependent modifications to high- processes. We describe a simple one-parameter geometric implementation of this picture within a modified Monte Carlo Glauber model tuned to Au jet data, and explore two of its major consequences. First, the model predicts a particular projectile-species dependence to the centrality dependence at high-, opposite to that expected from an energy loss effect. Second, we find that some of the large centrality dependence observed for forward di-hadron production in Au collisions at RHIC may arise from the physics of the "shrinking" projectile nucleon, in addition to impact parameter-dependent shadowing or saturation effects at low nuclear-. We conclude that analogous measurements in recently collected Au and HeAu collision data at RHIC can provide a unique test of these predictions.

    Subjects:
    Nuclear Theory (nucl-th); Nuclear Experiment (nucl-ex)
    arXiv:
    1603.06607 [pdf]
    PRC(2016)·25 citations
  2. 02

    [Submitted on 22 Mar 2016]

    Polarized-Deuteron Stripping Reaction at Intermediate Energies

    Valery I. Kovalchuk

    A general analytical expressions for the cross-section and the polarization of nucleons arising in the inclusive deuteron stripping reaction have been derived in the diffraction approximation. The nucleon-nucleus phases were calculated in the framework of Glauber formalism and making use of the double-folding potential. The tabulated distributions of the target nucleus density and the realistic deuteron wave function with correct asymptotic at large nucleon-nucleon distances were used. The calculated angular dependences for the cross-sections and the analyzing powers of the reaction are in good agreement with corresponding experimental data.

    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    1603.06700 [pdf]
    IJMPE(2016)·1 citation
  3. 03

    [Submitted on 22 Mar 2016]

    New experiments demand for a more precise analysis of continuum spectrum in 6He: technical details and formalism

    Jagjit Singh · L. Fortunato

    A simple three-body model of 6He is extended to include sd-continuum states in the picture in addition to the already investigated p-states. The role of different continuum components in the weakly bound nucleus 6He is studied by coupling unbound spd-waves of 5He by using simple pairing contact-delta interaction. The main focus of this paper is to outline the procedure that allows the calculation of different configurations of 6He including continuum states and to set up basic ingredients for computations. The method and results discussed here will be used for the calculation of monopole, dipole, quadrupole and octupole response of 6He.

    Comments:
    6 pages, 2 figures, presented at XXXIV MAZURIAN LAKES CONFERENCE ON PHYSICS Frontiers in Nuclear Physics, Piaski, Poland, September 6-13, 2015. Acta Physica Polonica B (2016)
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    1603.06831 [pdf]
    Acta Phys.Polon.B(2016)·2 citations
  4. 04

    [Submitted on 22 Mar 2016]

    Role of spd- Continuum Components in the Halo Nucleus 6He

    Jagjit Singh

    Role of different continuum components in the weakly bound nucleus 6He is studied by coupling unbound spd-waves of 5He by using simple pairing contact-delta interaction. The results show that 6He ground state displays collective nature by taking contribution from five different oscillating continuum states that sum up to give an exponentially decaying bound wavefunction emerging from five different possible configurations i.e. , , , and . The ground state properties of 6He has been calculated.

    Comments:
    4 pages, 4 figures, presented at Nuclear Structure and Dynamics III, June 14 to 19, 2015, Portoroz, Slovenia
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    1603.06842 [pdf]
    AIP Conf.Proc.(2015)·2 citations
  5. 05

    [Submitted on 22 Mar 2016]

    Correlation of the neutron star crust-core properties with the slope of the symmetry energy and the lead skin thickness

    H. Pais · A. Sulaksono · B. K. Agrawal · C. Providência

    The correlations of the crust-core transition density and pressure in neutron stars with the slope of the symmetry energy and the neutron skin thickness are investigated, using different families of relativistic mean field parametrizations with constant couplings and non-linear terms mixing the , and -meson fields. It is shown that the modification of the density dependence of the symmetry energy, involving the or the meson, gives rise to different behaviors: the effect of the -meson may also be reproduced within non-relativistic phenomenological models, while the effect of the -meson is essentially relativistic. Depending on the parametrization with or mixing terms, different values of the slope of the symmetry energy at saturation must be considered in order to obtain a neutron matter equation of state compatible with results from chiral effective field theory. This difference leads to different pressures at the crust-core transition density. A linear correlation between the transition density and the symmetry energy slope or the neutron skin thickness of the Pb nucleus is obtained, only when the -meson is used to describe the density dependence of the symmetry energy. A comparison is made between the crust-core transition properties of neutron stars obtained by three different methods, the Relativistic Random Phase Approximation (RRPA), the Vlasov equation and Thermodynamical method. It is shown that the RRPA and the Vlasov methods predict similar transition densities for -equilibrium stellar matter.

    Comments:
    11 pages, 5 figures
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    1603.06899 [pdf]
    PRC(2016)·30 citations

Affiliations

first authorsco-authorsvia INSPIRE