A way forward in the study of the symmetry energy: Experiment, theory, and observation

C. J. Horowitz, E. F. Brown, Y. Kim, W. G. Lynch, R. Michaels, A. Ono, J. Piekarewicz, M. B. Tsang, H. H. Wolter

Research output: Contribution to journalArticlepeer-review

245 Scopus citations

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 languageEnglish
Article number093001
JournalJournal of Physics G: Nuclear and Particle Physics
Volume41
Issue number9
DOIs
StatePublished - 1 Sep 2014
Externally publishedYes

Bibliographical note

Publisher Copyright:
© 2014 IOP Publishing Ltd.

Funding

FundersFunder number
Division of Astronomical Sciences
Indiana UniversityDE-SC0008808
Japan Society for the Promotion of Science London
Ministry of Science ICT and Future Planning
National Research Foundation
National Stroke FoundationPHY-0606007
U.S. Department of EnergyDE-SC0004835, DE-FD05-92ER40750, DE-FG02-87ER40365
National Science Foundation1109176, 1430152
Directorate for Mathematical and Physical Sciences0606007

    Keywords

    • heavy-ion collisions
    • neutron stars
    • symmetry energy

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