@article{278690a6d4614e6cb1352c1a7e54951d,
title = "Isospin transport phenomena for the systems Kr 80 + Ca 40,48 at 35 MeV/nucleon",
abstract = "Experimental data concerning isospin transport phenomena for the systems Kr80+Ca40,48 at 35 MeV/nucleon are presented. Data have been collected with four FAZIA blocks; this data set is the same analyzed in S. Piantelli, Phys. Rev. C 101, 034613 (2020)2469-998510.1103/PhysRevC.101.034613. The isotopic composition of the QuasiProjectile residue (up to Z around 25) and of its decay products in the two reactions are compared, finding a neutron enrichment when the target is Ca48. The isotopic composition of the emitted light charged particles (LCP) and intermediate mass fragments (IMF) was also investigated in different windows of velocity. The obtained results have been compared with the prediction of the transport model AMD followed by the statistical code GEMINI (used as an afterburner), with different recipes for the density dependence of the symmetry energy term in the nuclear equation of state. A weak indication in favor of a stiff symmetry energy emerges when the fragments emitted at midvelocity are examined.",
author = "{FAZIA Collaboration} and S. Piantelli and G. Casini and A. Ono and G. Poggi and G. Pastore and S. Barlini and M. Bini and A. Boiano and E. Bonnet and B. Borderie and R. Bougault and M. Bruno and A. Buccola and A. Camaiani and A. Chbihi and C. Ciampi and M. Cicerchia and M. Cinausero and M. Degerlier and Due{\~n}as, {J. A.} and Q. Fable and D. Fabris and Frankland, {J. D.} and C. Frosin and F. Gramegna and D. Gruyer and A. Kordyasz and T. Kozik and J. Lemari{\'e} and {Le Neindre}, N. and I. Lombardo and O. Lopez and G. Mantovani and T. Marchi and M. Henri and L. Morelli and A. Olmi and P. Ottanelli and M. P{\^a}rlog and G. Pasquali and J. Quicray and Stefanini, {A. A.} and G. Tortone and S. Upadhyaya and S. Valdr{\'e} and G. Verde and E. Vient and M. Vigilante",
note = "Funding Information: This work required the use of a lot of computation time for the production of the simulated data. We thank the GARR Consortium for the kind use of the cloud computing infrastructure on the platform cloud.garr.it. We thank also the INFN-CNAF for the use of its cloud computing infrastructure. A. Ono acknowledges support from Japan Society for the Promotion of Science KAKENHI Grant No. JP17K05432. This work was supported by the Polish National Science Centre under Contract No. 2014/14/M/ST2/00738 (COPIN-INFN Collaboration). The research leading to these results has received funding from the European Union HORIZON2020 reasearch and innovation programme under Grant Agreement No. 654002-ENSAR2. We acknowledge M. Bruno, who strongly contributed to the success of FAZIA. Publisher Copyright: {\textcopyright} 2021 American Physical Society.",
year = "2021",
month = jan,
day = "8",
doi = "10.1103/PhysRevC.103.014603",
language = "English",
volume = "103",
journal = "Physical Review C",
issn = "2469-9985",
publisher = "American Physical Society",
number = "1",
}