期刊
JOURNAL OF PHYSICS G-NUCLEAR AND PARTICLE PHYSICS
卷 41, 期 9, 页码 -出版社
IOP PUBLISHING LTD
DOI: 10.1088/0954-3899/41/9/093001
关键词
symmetry energy; neutron stars; heavy-ion collisions
资金
- NSCL/FRIB
- JSPS [24105001, 24105008, 2404]
- DOE grant [DE-FG02-87ER40365, DE-SC0008808, DE-SC0004835]
- NSF AST grant [11-09176]
- Rare Isotope Science Project - Ministry of Science, ICT and Future Planning (MSIP)
- National Research Foundation (NRF) of KOREA
- NSF [PHY-0606007]
- DOE [FD05-92ER40750]
- Excellence Cluster 'Origin and Structure of the Universe' of the German Research Foundation (DFG)
- Division Of Astronomical Sciences
- Direct For Mathematical & Physical Scien [1109176] Funding Source: National Science Foundation
- Division Of Physics
- Direct For Mathematical & Physical Scien [1430152] Funding Source: National Science Foundation
- Grants-in-Aid for Scientific Research [2404, 24105001, 24105008] Funding Source: KAKEN
- U.S. Department of Energy (DOE) [DE-SC0004835, DE-FG02-87ER40365, DE-SC0008808] Funding Source: U.S. Department of Energy (DOE)
The symmetry energy describes how the energy of nuclear matter rises as one goes away from equal numbers of neutrons and protons. This is very important to describe neutron rich matter in astrophysics. This article reviews our knowledge of the symmetry energy from theoretical calculations, nuclear structure measurements, heavy-ion collisions, and astronomical observations. We then present a roadmap to make progress in areas of relevance to the symmetry energy that promotes collaboration between the astrophysics and the nuclear physics communities.
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