Abstract
We show new data from the $^{64}$Ni+$^{124}$Sn and $^{58}$Ni+$^{112}$Snreactions 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.
Original language | English |
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Title of host publication | 11th International Conference on Nucleus-Nucleus Collisions (NN2012), San Antonio, Texas, USA, May 27-June 1, 2012 |
Number of pages | 9 |
Publication status | Published - 2012 |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy