Isospin-Asymmetric Cold Nuclear Matter in the Relativistic Mean-Field Theory with a Scalar-Isovector Interaction Channel

被引:0
|
作者
Alaverdyan, G. B. [1 ]
Alaverdyan, A. G. [1 ]
机构
[1] Erevan State Univ, Yerevan, Armenia
关键词
Mean field; nucleon matter; neutron star matter; symmetry energy; effective mass; binding energy; EQUATION-OF-STATE; PHASE-TRANSITION; PROGRESS; ENERGY;
D O I
10.1007/s10511-024-09829-y
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The properties of isospin-asymmetric cold nuclear matter are studied in terms of the relativistic mean-field theory in which, besides the fields of sigma, omega, and rho mesons, and the isovector, Lorentz-scalar field of the delta-meson is also taken into account. The properties of purely nucleonic np matter are studied as a function of the baryon density n(B) and the asymmetry parameter alpha, as well as the properties of electrically neutral beta-equilibrium npe mu matter as a function of the baryon density n(B). For different values of n(B) and a, such characteristics of np matter as the energy per baryon, the specific energy owing to isospin asymmetry, the effective proton and neutron masses, and the specific binding energy, are determined. It is shown that the energy owing to the asymmetry for a fixed value of alpha is a monotonically increasing function of the baryon density n(B). For npem matter, the effective proton and neutron masses M-p((eff)), M-n((eff)), the specific binding energy E-bind, the symmetry energy E-sym, the quantitative fraction of protons Y-p = n(p)/n(B) are studied, as well as the average meson fields (sigma) over tilde, (omega) over tilde, (delta) over tilde, and (rho) over tilde as functions of the baryon density n(B).
引用
收藏
页码:215 / 230
页数:16
相关论文
共 23 条
  • [1] Equation of state of isospin-asymmetric nuclear matter in relativistic mean-field models with chiral limits
    Jiang, Wei-Zhou
    Li, Bao-An
    Chen, Lie-Wen
    PHYSICS LETTERS B, 2007, 653 (2-4) : 184 - 189
  • [2] Self-consistent dynamical mean-field investigation of exotic structures in isospin-asymmetric nuclear matter
    Sebille, F.
    Figerou, S.
    de la Mota, V.
    NUCLEAR PHYSICS A, 2009, 822 : 51 - 73
  • [3] Thermodynamics of isospin-asymmetric nuclear matter from chiral effective field theory
    Wellenhofer, Corbinian
    Holt, Jeremy W.
    Kaiser, Norbert
    PHYSICAL REVIEW C, 2015, 92 (01):
  • [4] Asymmetric Nuclear Matter in Relativistic Mean-field Models with Isoscalar- and Isovector-meson Mixing
    Miyatsu, Tsuyoshi
    Cheoun, Myung-Ki
    Saito, Koichi
    ASTROPHYSICAL JOURNAL, 2022, 929 (01)
  • [6] Isovector scalar field effects in asymmetric nuclear matter
    Liu Bo
    Shen Cai-Wan
    Di Toro, M.
    Zhao En-Guang
    COMMUNICATIONS IN THEORETICAL PHYSICS, 2008, 49 (01) : 199 - 206
  • [7] Moments of inertia of neutron stars in relativistic mean field theory: The role of the isovector scalar channel
    Qian, Zhuang
    Xin, RuoYu
    Sun, BaoYuan
    SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2018, 61 (08)
  • [8] Nuclear matter with a Bose condensate of dibaryons in relativistic mean-field theory
    Faessler, A
    Buchmann, AJ
    Krivoruchenko, MI
    Martemyanov, BV
    PHYSICS LETTERS B, 1997, 391 (3-4) : 255 - 260
  • [9] ISOSPIN DEPENDENCE OF THE SATURATION PROPERTIES OF ASYMMETRIC NUCLEAR MATTER IN NONRELATIVISTIC MEAN FIELD MODEL
    Chakraborty, S.
    Sahoo, B.
    Sahoo, S.
    INTERNATIONAL JOURNAL OF MODERN PHYSICS E-NUCLEAR PHYSICS, 2012, 21 (09)
  • [10] Momentum and density dependence of the isospin part of nuclear mean field and equation of state of asymmetric nuclear matter
    Behera, B
    Routray, TR
    Pradhan, A
    Patra, SK
    Sahu, PK
    NUCLEAR PHYSICS A, 2005, 753 (3-4) : 367 - 386