Non-perturbative methods for a chiral effective field theory of finite density nuclear systems

被引:62
作者
Lacour, A. [2 ]
Oller, J. A. [1 ]
Meissner, U. -G. [2 ,3 ]
机构
[1] Univ Murcia, Dept Fis, E-30071 Murcia, Spain
[2] Univ Bonn, Bethe Ctr Theoret Phys, Helmholtz Inst Strahlen & Kernphys Theorie, D-53115 Bonn, Germany
[3] Forschungszentrum Julich, Julich Ctr Hadron Phys, Inst Kernphys, Inst Adv Simulat, D-52425 Julich, Germany
关键词
Chiral perturbation theory; Chiral effective field theories for nuclear matter; Non-perturbative methods; Partial wave expansion; Nuclear matter energy; TO-LEADING ORDER; PERTURBATION-THEORY; DELTA-EXCITATIONS; PIONIC ATOMS; MATTER; FORCES; SCATTERING; DYNAMICS; LAGRANGIANS; MESON;
D O I
10.1016/j.aop.2010.06.012
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Recently we have developed a novel chiral power counting scheme for an effective field theory of nuclear matter with nucleons and pions as degrees of freedom [1]. It allows for a systematic expansion taking into account both local as well as pion-mediated multi-nucleon interactions. We apply this power counting in the present study to the evaluation of the pion self-energy and the energy density in nuclear and neutron matter at next-to-leading order. To implement this power counting in actual calculations we develop here a non-perturbative method based on Unitary Chiral Perturbation Theory for performing the required resummations. We show explicitly that the contributions to the pion self-energy with in-medium nucleon-nucleon interactions to this order cancel. The main trends for the energy density of symmetric nuclear and neutron matter are already reproduced at next-to-leading order. In addition, an accurate description of the neutron matter equation of state, as compared with sophisticated many-body calculations, is obtained by varying only slightly a subtraction constant around its expected value. The case of symmetric nuclear matter requires the introduction of an additional fine-tuned subtraction constant, parameterizing the effects from higher order contributions. With that, the empirical saturation point and the nuclear matter compressibility are well reproduced while the energy per nucleon as a function of density closely agrees with sophisticated calculations in the literature. (C) 2010 Elsevier Inc. All rights reserved.
引用
收藏
页码:241 / 306
页数:66
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