Constraining the density dependence of t
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D.V. Shetty; S.J. Yennello; G.A. Souliotis
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Article
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2007
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Elsevier Science
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English
โ 296 KB
The density dependence of the symmetry energy in the equation of state of asymmetric nuclear matter (N/Z > 1) is important for understanding the structure of systems as diverse as the atomic nuclei and neutron stars. Due to a lack of understanding of the basic nucleon-nucleon interaction for matter