Abstract
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.
Original language | English |
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Article number | 093001 |
Journal | Journal of Physics G: Nuclear and Particle Physics |
Volume | 41 |
Issue number | 9 |
DOIs | |
State | Published - 1 Sep 2014 |
Externally published | Yes |
Bibliographical note
Publisher Copyright:© 2014 IOP Publishing Ltd.
Funding
Funders | Funder number |
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Division of Astronomical Sciences | |
Indiana University | DE-SC0008808 |
Japan Society for the Promotion of Science London | |
Ministry of Science ICT and Future Planning | |
National Research Foundation | |
National Stroke Foundation | PHY-0606007 |
U.S. Department of Energy | DE-SC0004835, DE-FD05-92ER40750, DE-FG02-87ER40365 |
National Science Foundation | 1109176, 1430152 |
Directorate for Mathematical and Physical Sciences | 0606007 |
Keywords
- heavy-ion collisions
- neutron stars
- symmetry energy