We discuss results concerning the behavior of hot nuclear sources formed in 40 ,48Ca+40 ,48Ca reactions at 25 MeV/nucleon. A correlation between the neutron-to-proton ratio of the total systems and heavy residue production is found. This correlation underlines the strong role played by the neutron-to-proton ratio degree of freedom on the behavior of hot nuclei at intermediate energies. Comparisons of our data with Constrained Molecular Dynamics calculations confirm that a moderately stiff behavior of the symmetry potential must be used to reproduce experimental data. These findings open the way for future investigations with exotic beams at radioactive ion beam facilities. © 2012 American Physical Society.

Cardella, G., Giuliani, G., Lombardo, I., Papa, M., Acosta, L., Agodi, C., et al. (2012). Effects of neutron richness on the behavior of nuclear systems at intermediate energies. PHYSICAL REVIEW. C, NUCLEAR PHYSICS, 85(6) [10.1103/PhysRevC.85.064609].

Effects of neutron richness on the behavior of nuclear systems at intermediate energies

SANTORO, Simone;
2012-01-01

Abstract

We discuss results concerning the behavior of hot nuclear sources formed in 40 ,48Ca+40 ,48Ca reactions at 25 MeV/nucleon. A correlation between the neutron-to-proton ratio of the total systems and heavy residue production is found. This correlation underlines the strong role played by the neutron-to-proton ratio degree of freedom on the behavior of hot nuclei at intermediate energies. Comparisons of our data with Constrained Molecular Dynamics calculations confirm that a moderately stiff behavior of the symmetry potential must be used to reproduce experimental data. These findings open the way for future investigations with exotic beams at radioactive ion beam facilities. © 2012 American Physical Society.
2012
Cardella, G., Giuliani, G., Lombardo, I., Papa, M., Acosta, L., Agodi, C., et al. (2012). Effects of neutron richness on the behavior of nuclear systems at intermediate energies. PHYSICAL REVIEW. C, NUCLEAR PHYSICS, 85(6) [10.1103/PhysRevC.85.064609].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10447/116325
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