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
相关论文
共 97 条
[1]   Equation of state of nucleon matter and neutron star structure [J].
Akmal, A ;
Pandharipande, VR ;
Ravenhall, DG .
PHYSICAL REVIEW C, 1998, 58 (03) :1804-1828
[2]   Identification of a Scalar Glueball [J].
Albaladejo, M. ;
Oller, J. A. .
PHYSICAL REVIEW LETTERS, 2008, 101 (25)
[3]  
BARGON G, 1965, INTRO DISPERSION TEC
[4]   Towards a perturbative theory of nuclear forces [J].
Beane, SR ;
Bedaque, PF ;
Savage, MJ ;
van Kolck, U .
NUCLEAR PHYSICS A, 2002, 700 (1-2) :377-402
[5]   CHIRAL DYNAMICS IN NUCLEONS AND NUCLEI [J].
BERNARD, V ;
KAISER, N ;
MEISSNER, UG .
INTERNATIONAL JOURNAL OF MODERN PHYSICS E, 1995, 4 (02) :193-344
[6]   Aspects of chiral pion-nucleon physics [J].
Bernard, V ;
Kaiser, N ;
Meissner, UG .
NUCLEAR PHYSICS A, 1997, 615 (04) :483-500
[7]   NUCLEAR COMPRESSIBILITIES [J].
BLAIZOT, JP .
PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1980, 64 (04) :171-248
[8]   MANDELSTAM REPRESENTATION FOR POTENTIAL SCATTERING [J].
BLANKENBECLER, R ;
GOLDBERGER, ML ;
KHURI, NN ;
TREIMAN, SB .
ANNALS OF PHYSICS, 1960, 10 (01) :62-93
[9]   Is nuclear matter perturbative with low-momentum interactions? [J].
Bogner, SK ;
Schwenk, A ;
Furnstahl, RJ ;
Nogga, A .
NUCLEAR PHYSICS A, 2005, 763 :59-79
[10]  
BOGNER SK, ARXIV09033366NUCLTH