PaperPanorama

Nuclear Theory·nucl-th

Thursday·November 30, 2017

16 papers9 primary·7 cross-listed

  1. 01

    [Submitted on 28 Nov 2017]

    Initial state and hydrodynamic modeling of heavy-ion collisions at RHIC BES energies

    Chun Shen🇺🇸 · Björn Schenke🇺🇸

    We present a fully three-dimensional initial state model for relativistic heavy-ion collisions at RHIC Beam Energy Scan (BES) collision energies. The initial energy and net baryon density profiles are produced based on a classical string deceleration model. The baryon stopping and fluctuations during this early stage of the collision are investigated by studying the net baryon rapidity distribution and longitudinal decorrelation of the transverse geometry.

    Comments:
    7 pages, 5 figures, conference proceeding for the Critical Point and Onset of Deconfinement - CPOD2017
    Subjects:
    Nuclear Theory (nucl-th); High Energy Physics — Phenomenology (hep-ph); Nuclear Experiment (nucl-ex)
    arXiv:
    1711.10544 [pdf]
    PoS(2018)·19 citations
  2. 02

    [Submitted on 28 Nov 2017]

    Uncertainties and understanding of experimental and theoretical results regarding reactions forming heavy and superheavy nuclei

    G. Giardina · G. Mandaglio · A.K. Nasirov · A. Anastasi · F. Curciarello · G. Fazio

    Experimental and theoretical results of the fusion probability of reactants in the entrance channel and the survival probability against fission at deexcitation of the compound nucleus formed in heavy-ion collisions are discussed. The theoretical results for a set of nuclear reactions leading to formation of compound nuclei (CNs) with the charge number reveal a strong sensitivity of to the characteristics of colliding nuclei in the entrance channel, dynamics of the reaction mechanism, and excitation energy of the system. We discuss the validity of assumptions and procedures for analysis of experimental data, and also the limits of validity of theoretical results obtained by the use of phenomenological models. The comparison of results obtained in many investigated reactions reveals serious limits of validity of the data analysis and calculation procedures.

    Comments:
    23 pages, 22 figurea, 1 table, in press in Nucl. Phys. A
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    1711.10603 [pdf]
    NPA(2018)·15 citations
  3. 03

    [Submitted on 29 Nov 2017]

    Formation and distribution of fragments in the spontaneous fission of 240Pu

    Jhilam Sadhukhan · Chunli Zhang · Witold Nazarewicz · Nicolas Schunck

    The goal of this paper is to better understand the structure of fission fragment distributions by investigating the competition between the static structure of the collective manifold and stochastic dynamics. In particular, we study the characteristics of the tails of yield distributions, which correspond to very asymmetric fission. We use the stochastic Langevin framework to simulate the nuclear evolution after the system tunnels through the multi-dimensional potential barrier. For a representative sample of different initial configurations along the outer turning-point line, we define effective fission paths by computing a large number of Langevin trajectories. We extract the relative contribution of each such path to the fragment distribution. We then use nucleon localization functions along effective fission pathways to analyze the characteristics of prefragments at pre-scission configurations. We find that non-Newtonian Langevin trajectories, strongly impacted by the random force, produce the tails of the fission fragment distribution. The prefragments deduced from nucleon localizations are formed early and change little as the nucleus evolves towards scission. On the other hand, the system contains many nucleons that are not localized in the prefragments, even near the scission point. Such nucleons are rapidly distributed at scission to form the final fragments. Our study shows that only theoretical models of fission that account for some form of dissipative/stochastic dynamics can give an accurate description of the structure of fragment distributions. In particular, it should be nearly impossible to predict the tails of these distributions within the standard formulation of time-dependent density functional theory. At the same time, the large number of non-localized nucleons during fission suggests that adiabatic approaches are ill-suited to describe fission fragment properties.

    Comments:
    6 pages, 7 figures, submitted to Phys. Rev. C
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    1711.10681 [pdf]
    PRC(2017)·42 citations
  4. 04

    [Submitted on 29 Nov 2017]

    Hadrons in Nuclei

    Laura Tolos🇩🇪

    A review on the state-of-the-art of heavy hadrons in nuclei is presented. In particular, the properties of mesons with strangeness and charm in matter are discussed, paying a special attention to the formation of exotic bound states in nuclei.

    Comments:
    11 pages, 3 figures, contribution based on an invited plenary talk at the XVII International Conference on Hadron Spectroscopy and Structure - Hadron2017, 25-29 September, 2017, Salamanca (Spain)
    Subjects:
    Nuclear Theory (nucl-th); High Energy Physics — Experiment (hep-ex); High Energy Physics — Phenomenology (hep-ph)
    arXiv:
    1711.10711 [pdf]
    PoS(2018)·0 citations
  5. 05

    [Submitted on 29 Nov 2017]

    Accelerating hydrodynamic description of pseudorapidity density and the initial energy density in p+p, Cu+Cu, Au+Au, and Pb+Pb collisions at RHIC and LHC

    Jiang Ze-Fang🇨🇳 · Yang Chun-Bin🇨🇳 · Mate Csanad🇭🇺 · Tamas Csorgo🇭🇺

    A known class of analytic, exact, accelerating solutions of prefect relativistic hydrodynamics with longitudinal acceleration is utilized to describe results on the pseudorapidity distributions for different collision systems. These results include measured in p+p, Cu+Cu, Au+Au, and Pb+Pb collisions at RHIC and LHC, in a broad centrality range. Going beyond the traditional Bjorken model, from the accelerating hydrodynamic description we determine the initial energy density and other thermodynamic quantities in those collisions.

    Comments:
    21 pages, 7 figures
    Subjects:
    Nuclear Theory (nucl-th); High Energy Physics — Phenomenology (hep-ph)
    arXiv:
    1711.10740 [pdf]
    PRC(2018)·20 citations
  6. 06

    [Submitted on 29 Nov 2017]

    Thermal noise in a boost-invariant matter expansion in relativistic heavy-ion collisions

    Chandrodoy Chattopadhyay🇮🇳 · Rajeev S. Bhalerao🇮🇳 · Subrata Pal🇮🇳

    We formulate a general theory of thermal fluctuations within causal second-order viscous hydrodynamic evolution of matter formed in relativistic heavy-ion collisions. The fluctuation is treated perturbatively on top of a boost-invariant longitudinal expansion. Numerical simulation of thermal noise is performed for a lattice QCD equation of state and for various second-order dissipative evolution equations. Phenomenological effects of thermal fluctuations on the two-particle rapidity correlations are studied.

    Comments:
    11 pages, 5 figures
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    1711.10759 [pdf]
    PRC(2018)·12 citations
  7. 07

    [Submitted on 29 Nov 2017]

    Gravitational waves from isolated neutron stars: mass dependence of r-mode instability

    Somnath Mukhopadhyay🇮🇳 · Joydev Lahiri🇮🇳 · Debasis Atta🇮🇳 · Kouser Imam🇺🇸 · D. N. Basu🇮🇳

    In this work we study the r-mode instability windows and the gravitational wave signatures of neutron stars in the slow rotation approximation using the equation of state obtained from the density dependent M3Y effective interaction. We consider the neutron star matter to be -equilibrated neutron-proton-electron matter at the core with a rigid crust. The fiducial gravitational and viscous timescales, the critical frequencies and the time evolutions of the frequencies and the rates of frequency change are calculated for a range of neutron star masses. We show that the young and hot rotating neutron stars lie in the r-mode instability region. We also emphasize that if the dominant dissipative mechanism of the r-mode is the shear viscosity along the boundary layer of the crust-core interface, then the neutron stars with low value lie in the r-mode instability region and hence emit gravitational radiation.

    Comments:
    15 pages including 4 tables & 11 figures; In this version Eq.(22) & Eq.(24) and correspondingly Figs.9-11 are corrected. arXiv admin note: text overlap with arXiv:1404.4360
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    1711.10794 [pdf]
    PRC(2018)·18 citations
  8. 08

    [Submitted on 28 Nov 2017]

    Calculations of the Decay Transitions of the Modified Poschl-Teller Potential Model via Bohr Hamiltonian Technique

    Nahid Soheibi · Majid Hamzavi · Mahdi Eshghi · Sameer M. Ikhdair

    We calculate the eigenvalues and their corresponding eigenfunctions of the Bohrs collective Hamiltonian with the help of the modified Poschl-Teller potential model within -unstable structure. Our numerical results for the ground state beta and gamma band heads together with the electric quadrupole B(E2) transition rates are displayed and compared with those available experimental data.

    Comments:
    13 pages, 3 figures
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    1711.10892 [pdf]
    IJMPE(2017)·9 citations
  9. 09

    [Submitted on 29 Nov 2017]

    Relativistic interpretation on the nature of nuclear tensor force

    Yao Yao Zong · Bao Yuan Sun

    The spin-dependent nature of the nuclear tensor force is studied in details within the relativistic Hartree-Fock approach. The relativistic formalism for the tensor force is supplemented with an additional Lorentz-invariant tensor formalism in -scalar channel, so as to take into account almost fully the nature of the tensor force brought about by the Fock diagrams in realistic nuclei. Specifically, the tensor sum rules are tested for the spin and pseudo-spin partners with/without nodes, to further understand the tensor force nature within relativistic model. It is shown that the interference between two components of nucleon spinors brings distinct violations on the tensor sum rules in realistic nuclei , which is mainly due to the opposite sign on quantities of the upper and lower components as well as the nodal difference. Even though, the sum rules can be precisely reproduced if taking the same radial wave functions for the spin/pseudo-spin partners in addition to neglecting the lower/upper components, revealing clearly the nature of tensor force.

    Comments:
    10 pages, 4 figures, 6 tables, to be published in Chinese Physics C
    Subjects:
    Nuclear Theory (nucl-th)
    arXiv:
    1711.10950 [pdf]
    CPC(2018)·29 citations

Affiliations

first authorsco-authorsvia INSPIRE