Probing the density dependence of the symmetry energy by nucleon flow

被引:8
作者
Fan, Xiao-Hua [1 ,2 ,3 ]
Yong, Gao-Chan [1 ,3 ]
Zuo, Wei [1 ,3 ]
机构
[1] Chinese Acad Sci, Inst Modern Phys, Lanzhou 730000, Gansu, Peoples R China
[2] Lanzhou Univ, Sch Phys Sci & Technol, Lanzhou 730000, Gansu, Peoples R China
[3] Univ Chinese Acad Sci, Sch Nucl Sci & Technol, Beijing 100049, Peoples R China
基金
中国国家自然科学基金;
关键词
HEAVY-ION COLLISIONS; ISOSPIN-SENSITIVE OBSERVABLES; NEUTRON-STARS; HIGH-MOMENTUM; EQUATION; STATE; MATTER; FRACTIONATION; PHYSICS; RADII;
D O I
10.1103/PhysRevC.97.034604
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
In the framework of the isospin-dependent Boltzmann-Uehling-Uhlenbeck transport model, sensitive regions of some nucleon observables to the nuclear symmetry energy are studied. It is found that the symmetry-energy-sensitive observable n/p ratio in the Sn-132 + Sn-124 reaction at 0.3 GeV/nucleon in fact just probes the density-dependent symmetry energy below the density of 1.5 rho(0) and effectively probes the density-dependent symmetry energy around or somewhat below the saturation density. Nucleon elliptic flow can probe the symmetry energy from the low-density region to the high-density region when changing the incident beam energies from 0.3 to 0.6 GeV/nucleon in the semi-central Sn-132 + Sn-124 reaction. And nucleon transverse and elliptic flows in the semi-central Au-197 + Au-197 reaction at 0.6 GeV/nucleon are more sensitive to the high-density behavior of the nuclear symmetry energy. One thus concludes that nucleon observables in the heavy reaction system and with higher incident beam energy are more suitable to be used to probe the high-density behavior of the symmetry energy. The present study may help one to get more specific information about the density-dependent symmetry energy from nucleon flow observable in heavy-ion collisions at intermediate energies.
引用
收藏
页数:5
相关论文
共 54 条
  • [1] Isospin effects in nuclear fragmentation
    Baran, V
    Colonna, M
    Di Toro, M
    Greco, V
    Zielinska-Pfabé, M
    Wolter, HH
    [J]. NUCLEAR PHYSICS A, 2002, 703 (3-4) : 603 - 632
  • [2] A GUIDE TO MICROSCOPIC MODELS FOR INTERMEDIATE ENERGY HEAVY-ION COLLISIONS
    BERTSCH, GF
    DASGUPTA, S
    [J]. PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1988, 160 (04): : 189 - 233
  • [3] SUPERNOVA MECHANISMS
    BETHE, HA
    [J]. REVIEWS OF MODERN PHYSICS, 1990, 62 (04) : 801 - 866
  • [4] Neutron radii in nuclei and the neutron equation of state
    Brown, BA
    [J]. PHYSICAL REVIEW LETTERS, 2000, 85 (25) : 5296 - 5299
  • [5] [Chen Liewen 陈列文], 2014, [原子核物理评论, Nuclear Physics Review], V31, P273
  • [6] Determination of the stiffness of the nuclear symmetry energy from isospin diffusion
    Chen, LW
    Ko, CM
    Li, BA
    [J]. PHYSICAL REVIEW LETTERS, 2005, 94 (03)
  • [7] Disappearance of elliptic flow: A new probe for the nuclear equation of state
    Danielewicz, P
    Lacey, RA
    Gossiaux, PB
    Pinkenburg, C
    Chung, P
    Alexander, JM
    McGrath, RL
    [J]. PHYSICAL REVIEW LETTERS, 1998, 81 (12) : 2438 - 2441
  • [8] Correlation between α-Decay Energies of Superheavy Nuclei Involving the Effects of Symmetry Energy
    Dong, Jianmin
    Zuo, Wei
    Scheid, Werner
    [J]. PHYSICAL REVIEW LETTERS, 2011, 107 (01)
  • [9] Density-dependent symmetry energy at subsaturation densities from nuclear mass differences
    Fan, Xiaohua
    Dong, Jianmin
    Zuo, Wei
    [J]. PHYSICAL REVIEW C, 2014, 89 (01):
  • [10] Constraining the high-density behavior of the nuclear symmetry energy with the tidal polarizability of neutron stars
    Fattoyev, F. J.
    Carvajal, J.
    Newton, W. G.
    Li, Bao-An
    [J]. PHYSICAL REVIEW C, 2013, 87 (01):