1. Probing properties of neutron stars with terrestrial nuclear reactions.
- Author
-
Li, Bao-An, Chen, Lie-Wen, Ko, Che Ming, Steiner, Andrew W., and Yong, Gao-Chan
- Subjects
HEAVY ions ,NEUTRONS ,NUCLEAR matter ,ISOBARIC spin ,NEUTRON stars - Abstract
Heavy-ion reactions induced by neutron-rich nuclei provide the unique opportunity in terrestrial laboratories to constrain the nuclear symmetry energy Esym in a broad density range. A conservative constraint, 32(ρ/ρ0)0.7 < Esym(ρ) < 32(ρ/ρ0)1.1, around the nuclear matter saturation density ρ0 has recently been obtained from analyzing the isospin diffusion data within a transport model for intermediate energy heavy-ion reactions. This subsequently puts a stringent constraint on properties of neutron stars, especially their radii and cooling mechanisms. © 2006 American Institute of Physics [ABSTRACT FROM AUTHOR]
- Published
- 2006
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