PaperPanorama

Nuclear Theory·nucl-th

Thursday·March 17, 2016

7 papers5 primary·2 cross-listed

  1. 01

    Mean-field study of C+C fusion

    Le Hoang Chien · Do Cong Cuong · Dao T. Khoa

    The nuclear mean-field potential arising from the C+C interaction at the low energies relevant for the astrophysical carbon burning process has been constructed within the double-folding model, using the realistic nuclear ground-state density of the C nucleus and the effective M3Y nucleon-nucleon (NN) interaction constructed from the G-matrix of the Paris (free) NN potential. To explore the nuclear medium effect, both the original density independent M3Y-Paris interaction and its density dependent CDM3Y6 version have been used in the folding model calculation of the C+C potential. The folded potentials at the different energies were used in the optical model description of the elastic C+C scattering at the energies around and below the Coulomb barrier, as well as in the barrier penetration model to estimate the fusion cross section and astrophysical factor of the C+C reactions at the low energies. The obtained results are in good agreement with experimental data over a wide range of energies.

    nucl-thastro-ph.SRnucl-exCommun.in Phys.(2015)·1 citation
  2. 02

    Event shape analysis in ultrarelativistic nuclear collisions

    Renata Kopecna🇨🇿 · Boris Tomasik🇨🇿

    We present a novel method for sorting events. So far, single variables like flow vector magnitude were used for sorting events. Our approach takes into account the whole azimuthal angle distribution rather than a single variable. This method allows us to determine the good measure of the event shape, providing a multiplicity-independent insight. We discuss the advantages and disadvantages of this approach, the possible usage in femtoscopy, and other more exclusive experimental studies.

    nucl-thhep-phnucl-exActa Phys.Polon.Supp.(2016)·0 citations
  3. 03

    Is the magnetic field making the inner crust of neutron stars more heterogeneous?

    Jianjun Fang · Sidney Avancini · Helena Pais · Constança Providência

    We study the effect of strong magnetic fields, of the order of G, on the extension of the crust of magnetized neutron stars. The dynamical instability region of neutron-proton-electron () matter at subsaturation densities and the mode with the largest growth rate are determined within a relativistic mean field model. It is shown that a strong magnetic field has a large effect on the instability region, defining the crust-core transition as a wide density range.

    nucl-thPRC(2016)·24 citations
  4. 04

    Counterintuitive Behaviors in Configuration Mixing

    Xiaofei Yu · Larry Zamick · Shadow Robinson

    By starting with a simple configurations of 2 neutrons in a single j shell we hare able to learn the effects of high lying configurations on physical properties such as nuclear magnetic g factors. Some counterintuitive results are found when both high lying spin orbit partners are allowed to admix with the basic configuration.

    nucl-thnucl-exphysics.atom-ph0 citations
  5. 05

    New parametrization of the deuteron wave function and calculations of the tensor polarization

    V. I. Zhaba

    The coefficients of new analytical forms for the deuteron wave function in coordinate space for NijmI, NijmII, Nijm93, Reid93 and Argonne v18 potentials have been numerically calculated. The obtained wave functions do not contain any superfluous knots. The designed parameters of the deuteron are in good agreement with the experimental and theoretical data. The new parameterization of the deuteron wave function in momentum space is obtained. The tensor polarization t20 calculated based on the wave functions is proportionate to the earlier published results.

    nucl-th4 citations

Affiliations

first authorsco-authorsvia INSPIRE