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dc.contributor.author Tsang, M.B. en
dc.contributor.author Stone, J.R. en
dc.contributor.author Camera, F. en
dc.contributor.author Danielewicz, P. en
dc.contributor.author Gandolfi, S. en
dc.contributor.author Hebeler, K. en
dc.contributor.author Horowitz, C.J. en
dc.contributor.author Lee, J. en
dc.contributor.author Lynch, W.G. en
dc.contributor.author Kohley, Z. en
dc.contributor.author Lemmon, R. en
dc.contributor.author Moller, P. en
dc.contributor.author Murakami, T. en
dc.contributor.author Riordan, S. en
dc.contributor.author Roca-Maza, X. en
dc.contributor.author Sammarruca, F. en
dc.contributor.author Steiner, A.W. en
dc.contributor.author Vidana, I. en
dc.contributor.author Yennello, S.J. en
dc.date.accessioned 2014-08-01T19:12:43Z en
dc.date.available 2014-08-01T19:12:43Z en
dc.date.issued 2012 en
dc.identifier.citation Tsang, M. B., Stone, J. R., Camera, F., Danielewicz, P., Gandolfi, S., Hebeler, K., . . . Yennello, S. J. (2012). Constraints on the symmetry energy and neutron skins from experiments and theory. Physical Review C - Nuclear Physics, 86(1), 015803. http://dx.doi.org/10.1103/PhysRevC.86.015803 en
dc.identifier.uri http://hdl.handle.net/2022/18523
dc.description.abstract The symmetry energy contribution to the nuclear equation of state impacts various phenomena in nuclear astrophysics, nuclear structure, and nuclear reactions. Its determination is a key objective of contemporary nuclear physics, with consequences for theunderstanding of dense matter within neutron stars. We examine the results of laboratory experiments that have provided initialconstraints on the nuclear symmetry energy and on its density dependence at and somewhat below normal nuclear matter density. Even though some of these constraints have been derived from properties of nuclei while others have been derived from thenuclear response to electroweak and hadronic probes, within experimental uncertainties-they are consistent with each other. We also examine the most frequently used theoretical models that predict the symmetry energy and its slope parameter. By comparing existing constraints on the symmetry pressure to theories, we demonstrate how contributions of three-body forces, which are essential ingredients in neutron matter models, can be determined. en
dc.language.iso en_US en
dc.publisher American Physical Society en
dc.relation.isversionof https://doi.org/10.1103/PhysRevC.86.015803 en
dc.rights © 2012 American Physical Society. en
dc.title Constraints on the symmetry energy and neutron skins from experiments and theory en
dc.type Article en


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