Isoscalar compression modes in relativistic random phase approximation

被引:110
作者
Ma, ZY
Van Giai, N [1 ]
Wandelt, A
Vretenar, D
Ring, P
机构
[1] CNRS, IN2P3, Inst Phys Nucl, F-91406 Orsay, France
[2] Inst Atom Energy, Beijing 102413, Peoples R China
[3] Tech Univ Munich, Dept Phys, D-85748 Garching, Germany
基金
中国国家自然科学基金;
关键词
relativistic random phase approximation; relativistic mean-field; giant resonances; compression modulus;
D O I
10.1016/S0375-9474(00)00523-6
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
Monopole and dipole compression modes in nuclei are analyzed in the framework of a fully consistent relativistic random phase approximation (RRPA), based on effective mean-field Lagrangians with nonlinear meson self-interaction terms. The large effect of Dirac sea states on isoscalar strength distribution functions is illustrated for the monopole mode, The main contribution of Fermi and Dirac sea pair states arises through the exchange of the scalar meson. The effect of vector meson exchange is much smaller, For the monopole mode, RRPA results are compared with constrained relativistic mean-field calculations. A comparison between experimental and calculated energies of isoscalar giant monopole resonances points to a value of 250-270 MeV for the nuclear matter incompressibility. A large discrepancy remains between theoretical predictions and experimental data for the dipole compression mode, (C) 2001 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:173 / 186
页数:14
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