PaperPanorama

Nuclear Theory·nucl-th

Tuesday·November 8, 2016

12 papers7 primary·5 cross-listed

  1. 01

    Uncertainty Quantification for Optical Model Parameters

    A.E. Lovell · F.M. Nunes · J. Sarich · S.M. Wild

    Although uncertainty quantification has been making its way into nuclear theory, these methods have yet to be explored in the context of reaction theory. For example, it is well known that different parameterizations of the optical potential can result in different cross sections, but these differences have not been systematically studied and quantified. The purpose of this work is to investigate the uncertainties in nuclear reactions that result from fitting a given model to elastic-scattering data, as well as to study how these uncertainties propagate to the inelastic and transfer channels. We use statistical methods to determine a best fit and create corresponding 95\% confidence bands. A simple model of the process is fit to elastic-scattering data and used to predict either inelastic or transfer cross sections. In this initial work, we assume that our model is correct, and the only uncertainties come from the variation of the fit parameters. We study a number of reactions involving neutron and deuteron projectiles with energies in the range of 5-25 MeV/u, on targets with mass =12-208. We investigate the correlations between the parameters in the fit. The case of deuterons on C is discussed in detail: the elastic-scattering fit and the prediction of C(d,p)C transfer angular distributions, using both uncorrelated and correlated minimization functions. The general features for all cases are compiled in a systematic manner to identify trends. Our work shows that, in many cases, the correlated functions (in comparison to the uncorrelated functions) provide a more natural parameterization of the process. These correlated functions do, however, produce broader confidence bands. Further optimization may require improvement in the models themselves and/or more information included in the fit.

    nucl-thPRC(2017)·38 citations
  2. 02

    Stellar electron capture rates on neutron-rich nuclei and their impact on core-collapse

    Ad. R. Raduta🇷🇴 · F. Gulminelli🇫🇷 · M. Oertel🇫🇷

    During the late stages of gravitational core-collapse of massive stars, extreme isospin asymmetries are reached within the core. Due to the lack of microscopic calculations of electron capture (EC) rates for all relevant nuclei, in general simple analytic parameterizations are employed. We study here several extensions of these parameterizations, allowing for a temperature, electron density and isospin dependence as well as for odd-even effects. The latter extra degrees of freedom considerably improve the agreement with large scale microscopic rate calculations. We find, in particular, that the isospin dependence leads to a significant reduction of the global EC rates during core collapse with respect to fiducial results, where rates optimized on calculations of stable -shell nuclei are used. Our results indicate that systematic microscopic calculations and experimental measurements in the neutron rich region are desirable for realistic simulations of the core-collapse.

    nucl-thPRC(2017)·27 citations
  3. 03

    Nuclear symmetry energy and the role of three-body forces

    S. Goudarzi · H. R. Moshfegh · P. Haensel

    Density dependence of nuclear symmetry energy as well as its partial wave decomposition is studied within the framework of lowest-order constrained variational (LOCV) method using AV18 two-body interaction supplemented by UIX three-body force. The main focus of the present work is to introduce a revised version of three-body force which is based on an isospin-dependent parametrization of coefficients in the UIX force, in order to overcome the inability to produce correct saturation-point parameters} in the framework of LOCV method. We find that employing the new model of {\ph three-body force} in the LOCV formalism leads to successfully reproducing the semi-empirical parameters of cold nuclear matter, including} , , and . All our models of three-body force combined with AV18 two-body force give maximum neutron star mass higher than . The fraction of protons in the nucleon cores of neutron stars strongly depends on the three-body force parametrization.

    nucl-thNPA(2018)·23 citations
  4. 04

    Symmetry Energy III: Isovector Skins

    Pawel Danielewicz (NSCL MSU) · Pardeep Singh (DCRUST) · Jenny Lee (U Hong Kong)

    Isoscalar density is a sum of neutron and proton densities and isovector is a normalized difference. Here, we report on the experimental evidence for the displacement of the isovector and isoscalar surfaces in nuclei, by from each other. We analyze data on quasielastic (QE) charge exchange (p,n) reactions, concurrently with proton and neutron elastic scattering data for the same target nuclei, following the concepts of the isoscalar and isovector potentials combined into Lane optical potential. The elastic data largely probe the geometry of the isoscalar potential and the (p,n) data largely probe a relation between the geometries of the isovector and isoscalar potentials. The targets include Ca, Zr, Sn and Pb and projectile incident energy values span the range of (10-50). In our fit to elastic and QE charge-exchange data, we allow the values of isoscalar and isovector radii, diffusivities and overall potential normalizations to float away from those in the popular Koning and Delaroche parametrization. We find that the best-fit isovector radii are consistently larger than isoscalar and the best-fit isovector surfaces are steeper. Upon identifying the displacement of the potential surfaces with the displacement of the surfaces for the densities in the Skyrme-Hartree-Fock calculations, and by supplementing the results with those from analysing excitation energies to isobaric analog states in the past, we arrive at the slope and value of the symmetry energy at normal density of and , respectively.

    nucl-thnucl-exNPA(2017)·90 citations
  5. 05

    Nuclear structure calculations in Ne with No-Core Configuration-Interaction model

    Maciej Konieczka · Wojciech Satuła

    Negative parity states in Ne and Gamow-Teller strength distribution for the ground-state beta-decay of Na are calculated for the very first time using recently developed No-Core Configuration-Interaction model. The approach is based on multi-reference density functional theory involving isospin and angular-momentum projections. Advantages and shortcomings of the method are briefly discussed.

    nucl-thActa Phys.Polon.B(2017)·1 citation
  6. 06

    Theoretical photo-disintegration of O

    M. Katsuma

    The photodisintegration of O is predicted to be dominated by 2 excitation in the vicinity of the -particle threshold. The reaction rates of C(,)O are expected to be determined from this reaction.

    nucl-thastro-ph.SRnucl-exJPS Conf.Proc.(2017)·2 citations
  7. 07

    Effect of the final state interaction of on the photoproduction off nucleon

    Shuntaro Sakai🇯🇵 · Atsushi Hosaka🇯🇵 · Hideko Nagahiro🇯🇵

    We investigate the photoproduction off the nucleon with a particular interest in the effect of the final-state interaction (FSI) of the meson and nucleon based on three-flavor linear sigma model. We find an enhancement in the cross section of the photoproduction near the -threshold energy owing to the FSI. With the meson at forward angles, the energy dependence near the threshold is well reproduced with the FSI. The cross section at backward angles can also be a good probe to investigate the strength of the interaction.

    nucl-thhep-phPRC(2017)·3 citations

Affiliations

first authorsco-authorsvia INSPIRE