6533b82cfe1ef96bd128ecdc

RESEARCH PRODUCT

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

Maria ColonnaJi-youn HanLuisa ZettaF. RizzoG. CardellaF. PortoI. BerceanuS. PirroneS. SantoroF. AmoriniE. De FilippoP. RussottoGiuseppe VerdeLucrezia AuditoreI. LombardoAmalia PopTriestino MinnitiP. GuazzoniL. GrassiA. TrifiròE. PiaseckiE. GeraciV. BaranC. MaiolinoG. LanzaloneA. GrzeszczukM. PapaJ. WilczyńskiS. GianìMarina TrimarchiE. La GuidaraMariano VigilanteGiuseppe PolitiAngelo Pagano

subject

PhysicsHistoryRelative velocityFOS: Physical sciencesObservableKinematicsNuclear matterComputer Science ApplicationsEducationPhysics and Astronomy (all)Fragmentation (mass spectrometry)Mean field theoryExcited stateIsospinAtomic physicsNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear Experiment

description

We show new data from the $^{64}$Ni+$^{124}$Sn and $^{58}$Ni+$^{112}$Sn 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.

https://dx.doi.org/10.48550/arxiv.1209.6461