From the microscopic to the macroscopic world: from nucleons to neutron stars

被引：27

作者：

Gandolfi, S. ^{[1
]}

Lippuner, J. ^{[2
,3
]}

Steiner, A. W. ^{[4
,5
]}

Tews, I ^{[1
]}

Du, X. ^{[4
]}

Al-Mamun, M. ^{[4
]}

机构：

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

[2] Los Alamos Natl Lab, Computat Phys & Methods, CCS 2, Los Alamos, NM 87545 USA

[3] Los Alamos Natl Lab, Ctr Theoret Astrophys, Los Alamos, NM 87545 USA

[4] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA

[5] Oak Ridge Natl Lab, Div Phys, Oak Ridge, TN 37831 USA

来源：

JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS | 2019年 / 46卷 / 10期

关键词：

neutron stars; equation of state of dense matter; gravitational waves; GW170817; EQUATION-OF-STATE; R-PROCESS NUCLEOSYNTHESIS; MONTE-CARLO CALCULATIONS; GAMMA-RAY BURSTS; MATTER; NEUTRINOS; MERGERS; EJECTA; SIGNATURES; ELEMENTS;

D O I：

10.1088/1361-6471/ab29b3

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：

Recent observations of neutron-star properties, in particular the recent detection of gravitational waves emitted from binary neutron stars, GW170817, open the way to put strong constraints on nuclear interactions. In this paper, we review the state of the art in calculating the equation of state of strongly interacting matter from first principle calculations starting from microscopic interactions among nucleons. We then review selected properties of neutron stars that can be directly compared with present and future observations.

引用

页数：21

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