Influence of fast emissions and statistical de-excitation on the isospin transport ratio
arXiv:2010.00242 · doi:10.1103/PhysRevC.102.044607
Abstract
Isospin transport ratio is a powerful method to estimate the neutron-proton (n-p) equilibration in heavy-ion collisions, and extensively used to obtain information on the asy-stiffness of the nuclear Equation of State. In fact such a ratio is expected to bypass any perturbations introducing a linear transformation of the chosen observable. In particular, it is supposed to overcome contributions due to emission, either of dynamical or statistical nature, from the primary fragments formed during the collisions. In this paper we explore the validity of this assumption, looking at the quasi-projectile n-p ratio () in peripheral and semi-peripheral events for Ca+Ca reactions at 35\amev{}, simulated via the Antisymmetrized Molecular Dynamics transport model, coupled to different statistical decay codes. The statistical de-excitation of the primary fragments introduces a linear transformation at relatively high excitation energies (above 2\amev{}) when the residue approaches the Evaporation Attractor Line, while some effect is produced at lower excitation energies due to the occurrence of some non-linearities. As for fast emissions after the end of the projectile-target interaction it is shown that they introduce a non-linear transformation too.
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- Isospin diffusion measurement from the direct detection of a Quasi-Projectile remnant
- First results from the INDRA-FAZIA apparatus on isospin diffusion in Ni+Ni systems at Fermi energies
- Examination of cluster production in excited light systems at Fermi energies from new experimental data and comparison with transport model calculations
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