Quantum Monte Carlo methods for nuclear physics

被引：610

作者：

Carlson, J. ^{[1
]}

Gandolfi, S. ^{[1
]}

Pederiva, F. ^{[2
,3
]}

Pieper, Steven C. ^{[4
]}

Schiavilla, R. ^{[5
,6
]}

Schmidt, K. E. ^{[7
]}

Wiringa, R. B. ^{[8
]}

机构：

[1] Los Alamos Natl Lab, Div Theoret, POB 1663, Los Alamos, NM 87545 USA

[2] Univ Trento, Dipartimento Fis, I-38123 Trento, Italy

[3] INFN Trento Inst Fundamental Phys & Applicat, I-38123 Trento, Italy

[4] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA

[5] Jefferson Lab, Ctr Theory, Newport News, VA 23529 USA

[6] Old Dominion Univ, Dept Phys, Norfolk, VA 23529 USA

[7] Arizona State Univ, Dept Phys, Tempe, AZ 85287 USA

[8] Argonne Natl Lab, Div Phys, Argonne, IL 60439 USA

来源：

REVIEWS OF MODERN PHYSICS | 2015年 / 87卷 / 03期

基金：

美国国家科学基金会;

关键词：

EQUATION-OF-STATE; ELECTROMAGNETIC FORM-FACTORS; MESON-EXCHANGE CURRENTS; ENERGY-LEVELS; GROUND-STATE; SKYRME PARAMETRIZATION; 3-NUCLEON INTERACTION; ELECTRON-SCATTERING; CHIRAL LAGRANGIANS; PARITY VIOLATION;

D O I：

10.1103/RevModPhys.87.1067

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Quantum Monte Carlo methods have proved valuable to study the structure and reactions of light nuclei and nucleonic matter starting from realistic nuclear interactions and currents. These ab initio calculations reproduce many low-lying states, moments, and transitions in light nuclei, and simultaneously predict many properties of light nuclei and neutron matter over a rather wide range of energy and momenta. The nuclear interactions and currents are reviewed along with a description of the continuum quantum Monte Carlo methods used in nuclear physics. These methods are similar to those used in condensed matter and electronic structure but naturally include spin-isospin, tensor, spin-orbit, and three-body interactions. A variety of results are presented, including the low-lying spectra of light nuclei, nuclear form factors, and transition matrix elements. Low-energy scattering techniques, studies of the electroweak response of nuclei relevant in electron and neutrino scattering, and the properties of dense nucleonic matter as found in neutron stars are also described. A coherent picture of nuclear structure and dynamics emerges based upon rather simple but realistic interactions and currents.

引用

页码：1067 / 1118

页数：52

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