PaperPanorama

Nuclear Theory·nucl-th

Friday·August 5, 2016

7 papers3 primary·4 cross-listed

  1. 01

    [Submitted on 3 Aug 2016]

    Improving Predictions with Reliable Extrapolation Schemes and Better Understanding of Factorization

    Sushant N. More🇺🇸

    We investigate two distinct sources of uncertainty in low-energy nuclear physics calculations and develop ways to account for them. Harmonic oscillator basis expansions are widely used in ab-initio nuclear structure calculations. Finite computational resources usually require that the basis be truncated before observables are fully converged, necessitating reliable extrapolation schemes. We show that a finite oscillator basis effectively imposes a hard-wall boundary condition. We accurately determine the position of the hard-wall as a function of oscillator space parameters, derive extrapolation formulas for the energy and other observables, and discuss the extension of this approach to higher angular momentum. Nucleon knockout reactions have been widely used to study and understand nuclear properties. Such an analysis implicitly assumes that the effects of the probe can be separated from the physics of the target nucleus. This factorization between nuclear structure and reaction components depends on the renormalization scale and scheme, and has not been well understood. But it is potentially critical for interpreting experiments and for extracting process-independent nuclear properties. We use similarity renormalization group (SRG) transformations to systematically study the scale dependence of factorization for the simplest knockout process of deuteron electrodisintegration. We find that the extent of scale dependence depends strongly on kinematics, but in a systematic way. Based on examination of the relevant overlap matrix elements, we are able to qualitatively explain and even predict the nature of scale dependence based on the kinematics under consideration.

    Comments:
    PhD thesis
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    1608.01385 [pdf]
    0 citations
  2. 02

    [Submitted on 4 Aug 2016]

    Deformation-induced splitting of isoscalar E0 giant resonance: Skyrme random-phase-approximation analysis

    J. Kvasil · V.O. Nesterenko · A. Repko · W. Kleinig · P.-G. Reinhard

    The deformation-induced splitting of isoscalar giant monopole resonance (ISGMR) is systematically analyzed in a wide range of masses covering medium, rare-earth, actinide, and superheavy axial deformed nuclei. The study is performed within the fully self-consistent quasiparticle random-phase-approximation (QRPA) method based on the Skyrme functional. Two Skyrme forces, one with a large (SV-bas) and one with a small (SkP) nuclear incompressibility, are considered. The calculations confirm earlier results that, due to the deformation-induced E0-E2 coupling, the isoscalar E0 resonance attains a double-peak structure and significant energy upshift. Our results are compared with available analytic estimations. Unlike earlier studies, we get a smaller energy difference between the lower and upper peaks and thus a stronger E0-E2 coupling. This in turn results in more pumping of E0 strength into the lower peak and more pronounced splitting of ISGMR. We also discuss widths of the peaks and their negligible correlation with deformation.

    Comments:
    11 pages, 10 figures
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    1608.01483 [pdf]
    PRC(2016)·26 citations
  3. 03

    [Submitted on 4 Aug 2016]

    The attribute of rotational profile to the hyperon puzzle in the prediction of heaviest compact star

    M. Bhuyan · B. V. Carlson · S.-G. Zhou · S. K. Patra

    In this theoretical study, we report an investigation of the equations of state (EoSs) ofhyper-nuclear matter and its composition as a function of density within the framework of effective field theory motivated relativistic mean field model. We have used G2 force parameter along with various hyperon-meson coupling ratios by allowing the mixing and the breaking of SU(6) symmetry to predict the EoSs, keeping the nucleonic coupling constant intact. We have estimated the properties of non-rotating and rapidly rotating configuration of compact stars by employing four different representative sets of equations of state. The obtained results of the mass and radius for the compact stars are compared with the recent mass observations. Further, we have studied the stability and sensitivity of rotational frequency (at sub-millisecond period) on the configuration of the compact stars, because the angular frequency is significantly smaller than the mass-shedding (Keplerian) frequency in slow rotation regime. Moreover, the yield of hyperon as a function of density for various hyperon-meson couplings are also estimated.

    Comments:
    19 pages, 6 figures, 2 tables
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    1608.01639 [pdf]
    IJMPE(2017)·8 citations

Affiliations

first authorsco-authorsvia INSPIRE