Exploring the Symmetry Energy of Asymmetric Nuclear Matter with Heavy Ion Reactions

Details Exploring the Symmetry Energy of Asymmetric Nuclear Matter with Heavy Ion Reactions Exploring the Symmetry Energy of Asymmetric Nuclear Matter with Heavy Ion Reactions

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008pun..conf..212t&link_type=abstract

PHYSICS OF UNSTABLE NUCLEI. Proceedings of the International Symposium on the ISPUN07. Held 3-7 July 2007 in Hoi An, Vietnam. Ed

Physics

Scientific paper

The nuclear symmetry energy governs many properties of neutron-rich nuclei and of neutron stars. Neutron star radii, moments of inertia, phase transitions in the stellar interior and the cooling of proto-neutron stars are among the stellar properties that are most strongly affected. A number of interesting experimental observables have been identified that provide opportunities to probe the density dependence of the symmetry energy via nucleus-nucleus collisions. In this talk, we discuss measurements and simulations of the isospin diffusion and neutron to proton emission observable over a wide incident energy range. This work is supported by the National Science Foundation under Grant Nos. PHY-01-10253, PHY-0606007.

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