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Isospin diffusion from Ca 40,48 + Ca 40,48 experimental data at Fermi energies: Direct comparisons with transport model calculations

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Title
Isospin diffusion from Ca 40,48 + Ca 40,48 experimental data at Fermi energies: Direct comparisons with transport model calculations
Author(s)
Fable, Q.; Baldesi, L.; Barlini, S.; Bonnet, E.; Borderie, B.; Bougault, R.; Camaiani, A.; Casini, G.; Chbihi, A.; Ciampi, C.; Duenas, J.A.; Frankland, J.D.; Genard, T.; Gruyer, D.; Henri, M.; Hong, B.; S. Kim; Kordyasz, A.J.; Kozik, T.; Le, Fevre A.; Le, Neindre N.; Lombardo, I.; Lopez, O.; Marchi, T.; Marini, P.; Nam, S.H.; Ono, A.; Park, J.; Parlog, M.; Piantelli, S.; Rebillard-Soulie, A.; Verde, G.; Vient, E.
Publication Date
2024-06
Journal
Physical Review c, v.109, no.6
Publisher
AMER PHYSICAL SOC
Abstract
This article presents an investigation of isospin equilibration in cross-bombarding Ca40,48+Ca40,48 reactions at 35 MeV/nucleon, by comparing experimental data with filtered transport model calculations. Isospin diffusion is studied using the evolution of the isospin transport ratio with centrality. The asymmetry parameter δ=(N-Z)/A of the quasiprojectile (QP) residue is used as isospin-sensitive observable, while a recent method for impact parameter reconstruction is used for centrality sorting. A benchmark of global observables is proposed to assess the relevance of the antisymmetrized molecular dynamics (amd) model, coupled to gemini++, in the study of dissipative collisions. Our results demonstrate the importance of considering cluster formation to reproduce observables used for isospin transport and centrality studies. Within the amd model, we prove the applicability of the impact parameter reconstruction method, enabling a direct comparison to the experimental data for the investigation of isospin diffusion. For both, we evidence a tendency to isospin equilibration with an impact parameter decreasing from 9 to 3 fm, while the full equilibration is not reached. A weak sensitivity to the stiffness of the equation of state employed in the model is also observed, with a better reproduction of the experimental trend for the neutron-rich reactions. © 2024 American Physical Society.
URI
https://pr.ibs.re.kr/handle/8788114/15826
DOI
10.1103/PhysRevC.109.064605
ISSN
2469-9985
Appears in Collections:
Center for Exotic Nuclear Studies(희귀 핵 연구단) > 1. Journal Papers (저널논문)
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