We show new data from the 64Ni+124Sn and 58Ni+112Sn reactions studied in direct kinematics with the CHIMERA detector at INFN-LNS and compared with the reverse kinematics reactions at the same incident beam energy (35 A MeV). Analyzing the data with the method of relative velocity correlations, fragments coming from statistical decay of an excited projectile-like (PLF) or target-like (TLF) fragments are discriminated from the ones coming from dynamical emission in the early stages of the reaction. By comparing data of the reverse kinematics experiment with a stochastic mean field (SMF) + GEMINI calculations our results show that observables from neck fragmentation mechanism add valuable constraints on the density dependence of symmetry energy. An indication is found for a moderately stiff symmetry energy potential term of EOS.

We show new data from the 64Ni+124$Sn and 58Ni+112Snreactions studied in direct kinematics with the CHIMERA detector at INFN-LNSand compared with the reverse kinematics reactions at the same incident beamenergy (35 A MeV). Analyzing the data with the method of relative velocitycorrelations, fragments coming from statistical decay of an excitedprojectile-like (PLF) or target-like (TLF) fragments are discriminated from theones coming from dynamical emission in the early stages of the reaction. Bycomparing data of the reverse kinematics experiment with a stochastic meanfield (SMF) + GEMINI calculations our results show that observables from neckfragmentation mechanism add valuable constraints on the density dependence ofsymmetry energy. An indication is found for a moderately stiff symmetry energypotential term of EOS.

Correlations between isospin dynamics and Intermediate Mass Fragments emission time scales: a probe for the symmetry energy in asymmetric nuclear matter

Geraci E;Lombardo I;MINNITI, TRIESTINO;PAGANO, ANGELO;POLITI, Giuseppe;RIZZO, Francesca;
2013-01-01

Abstract

We show new data from the 64Ni+124$Sn and 58Ni+112Snreactions studied in direct kinematics with the CHIMERA detector at INFN-LNSand compared with the reverse kinematics reactions at the same incident beamenergy (35 A MeV). Analyzing the data with the method of relative velocitycorrelations, fragments coming from statistical decay of an excitedprojectile-like (PLF) or target-like (TLF) fragments are discriminated from theones coming from dynamical emission in the early stages of the reaction. Bycomparing data of the reverse kinematics experiment with a stochastic meanfield (SMF) + GEMINI calculations our results show that observables from neckfragmentation mechanism add valuable constraints on the density dependence ofsymmetry energy. An indication is found for a moderately stiff symmetry energypotential term of EOS.
2013
We show new data from the 64Ni+124Sn and 58Ni+112Sn reactions studied in direct kinematics with the CHIMERA detector at INFN-LNS and compared with the reverse kinematics reactions at the same incident beam energy (35 A MeV). Analyzing the data with the method of relative velocity correlations, fragments coming from statistical decay of an excited projectile-like (PLF) or target-like (TLF) fragments are discriminated from the ones coming from dynamical emission in the early stages of the reaction. By comparing data of the reverse kinematics experiment with a stochastic mean field (SMF) + GEMINI calculations our results show that observables from neck fragmentation mechanism add valuable constraints on the density dependence of symmetry energy. An indication is found for a moderately stiff symmetry energy potential term of EOS.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11769/61836
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