S. Carboni
University of Florence
Network
Latest external collaboration on country level. Dive into details by clicking on the dots.
Publication
Featured researches published by S. Carboni.
Physical Review C | 2013
S. Barlini; S. Piantelli; G. Casini; P. R. Maurenzig; A. Olmi; M. Bini; S. Carboni; G. Pasquali; G. Poggi; A.A. Stefanini; R. Bougault; E. Bonnet; B. Borderie; A. Chbihi; J.D. Frankland; D. Gruyer; O. Lopez; N. Le Neindre; M. Pârlog; M.F. Rivet; E. Vient; E. Rosato; G. Spadaccini; M. Vigilante; M. Bruno; T. Marchi; L. Morelli; M. Cinausero; M. Degerlier; F. Gramegna
Isospin transport phenomena in dissipative heavy ion collisions have been in- vestigated at Fermi energies with a beam of 84 Kr at 35AMeV. A comparison of theh Ni /Z of light and medium products forward-emitted in the centre of mass frame when the beam impinges on two different targets, the n-poor 112 Sn and the n-rich 124 Sn, is presented. Data were collected by means of a three-layer telescope with very good performances in terms of mass identification (full isotopic resolution up to Z�20 for ions punching through the first detector layer) built by the FAZIA Collaboration and located just beyond the grazing angle for both reactions. Theh Ni /Z of the products detected when the n-rich target is used is always higher than that associated to the n-poor one; since the detector was able to measure only fragments coming from the QuasiProjectile decay and/or neck emission, the observed behaviour can be ascribed to the isospin diffusion process, driven by the isospin gradient between QuasiProjectile and QuasiTarget. Moreover, for light fragments theh Ni /Z as a function of the lab velocity of the fragment is observed to increase when we move from the QuasiProjectile velocity to the centre of mass (neck zone). This effect can be interpreted as an evidence of isospin drift driven by the density gradient between the QuasiProjectile zone (at normal density) and the more diluted neck zone.
European Physical Journal A | 2013
M. Bruno; F. Gramegna; T. Marchi; L. Morelli; G. Pasquali; G. Casini; U. Abbondanno; G. Baiocco; L. Bardelli; S. Barlini; M. Bini; S. Carboni; M. Cinausero; M. D’Agostino; M. Degerlier; V. L. Kravchuk; E. Geraci; P. F. Mastinu; A. Ordine; S. Piantelli; G. Poggi; A. Moroni
An upgraded GARFIELD + Ring Counter (RCo) apparatus is presented with improved performances as far as electronics and detectors are concerned. On the one hand fast sampling digital read out has been extended to all detectors, allowing for an important simplification of the signal processing chain together with an enriched extracted information. On the other hand a relevant improvement has been made in the forward part of the set-up (RCo): an increased granularity of the CsI(Tl) crystals and a higher homogeneity in the silicon detector resistivity. The renewed performances of the GARFIELD + RCo array make it suitable for nuclear reaction measurements both with stable and with Radioactive Ion Beams (RIB), like the ones planned for the SPES facility, where the physics of isospin can be studied.
Physical Review C | 2013
S. Piantelli; G. Casini; P. R. Maurenzig; A. Olmi; S. Barlini; M. Bini; S. Carboni; G. Pasquali; G. Poggi; A.A. Stefanini; S. Valdré; R. Bougault; E. Bonnet; B. Borderie; A. Chbihi; J.D. Frankland; D. Gruyer; O. Lopez; N. Le Neindre; M. Pârlog; M.F. Rivet; E. Vient; E. Rosato; G. Spadaccini; M. Vigilante; M. Bruno; T. Marchi; L. Morelli; M. Cinausero; M. Degerlier
The odd-even staggering of the yield of final reaction products has been studied as a function of proton (Z) and neutron (N ) numbers for the collisions 84 Kr + 112 Sn and 84 Kr + 124 Sn at 35 MeV/nucleon in a wide range of elements (up to Z ≈ 20). The experimental data show that staggering effects rapidly decrease with increasing size of the fragments. Moreover the staggering in N is definitely larger than the one in Z. Similar general features are qualitatively reproduced by the GEMINI code. Concerning the comparison of the two systems, the staggering in N is in general rather similar, being slightly larger only for the lightest fragments produced in the n-rich system. In contrast the staggering in Z, although smaller than that in N , is sizably larger for the n-poor system with respect to the n-rich one.
arXiv: Instrumentation and Detectors | 2013
M.F. Rivet; E. Bonnet; B. Borderie; R. Bougault; P. Edelbruck; N. Le Neindre; S. Barlini; S. Carboni; G. Casini; E. Rosato; G. Tortone
FAZIA is designed for detailed studies of the isospin degree of freedom, extending to the limits the isotopic identification of charged products from nuclear collisions when using silicon detectors and CsI(Tl) scintillators. We show that the FAZIA telescopes give isotopic identification up to Z~25 with a ΔE-E technique. Digital Pulse Shape Analysis makes possible elemental identification up to Z=55 and isotopic identification for Z=1-10 when using the response of a single silicon detector. The project is now in the phase of building a demonstrator comprising about 200 telescopes.
Physical Review C | 2016
S. Valdré; S. Piantelli; G. Casini; S. Barlini; S. Carboni; M. Ciemała; M. Kmiecik; A. Maj; K. Mazurek; M. Cinausero; F. Gramegna; V. L. Kravchuk; L. Morelli; T. Marchi; G. Baiocco; L. Bardelli; P. Bednarczyk; G. Benzoni; M. Bini; N. Blasi; A. Bracco; S. Brambilla; M. Bruno; F. Camera; A. Chbihi; A. Corsi; F. C. L. Crespi; M. D'Agostino; M. Degerlier; D. Fabris
A study of fusion-evaporation and (partly) fusion-fission channels for the
EPJ Web of Conferences | 2014
S. Valdré; S. Barlini; G. Casini; G. Pasquali; S. Piantelli; S. Carboni; M. Cinausero; F. Gramegna; T. Marchi; G. Baiocco; L. Bardelli; G. Benzoni; M. Bini; N. Blasi; A. Bracco; S. Brambilla; M. Bruno; F. Camera; A. Corsi; F. C. L. Crespi; M. D’Agostino; M. Degerlier; V. L. Kravchuk; S. Leoni; B. Million; D. Montanari; L. Morelli; A. Nannini; R. Nicolini; G. Poggi
^{88}
Acta Physica Polonica B | 2014
S. Barlini; S. Piantelli; G. Casini; P. R. Maurenzig; A. Olmi; M. Bini; S. Carboni; G. Pasquali; G. Poggi; A.A. Stefanini; E. Scarlini; R. Bougault; O. Lopez; N. Le Neindre; M. Parlog; E. Vient; E. Bonnet; A. Chbihi; J.D. Frankland; D. Gruyer; M.F. Rivet; B. Borderie; E. Rosato; G. Spadaccini; M. Vigilante; F. Bruno; L. Morelli; M. Cinausero; M. Degerlier; F. Gramegna
Mo compound nucleus, produced at different excitation energies in the reaction
25th International Nuclear Physics Conference (INPC 2013) | 2014
G. Casini; S. Barlini; G. Pasquali; G. Pastore; M. Bini; S. Carboni; A. Olmi; S. Piantelli; G. Poggi; A. A. Stefanini; S. Valdré; E. Bonnet; B. Borderie; R. Bougault; M. Bruno; A. Chbihi; M. Cinausero; M. Degerlier; P. Edelbruck; J.D. Frankland; F. Gramegna; D. Gruyer; M. Guerzoni; A. Kordjasz; T. Kozik; N. Le Neindre; O. Lopez; T. Marchi; P. Marini; L. Morelli
^{48}
2013 International Nuclear Physics Conference, INPC 2013 | 2014
S. Piantelli; G. Casini; A. Olmi; S. Barlini; M. Bini; S. Carboni; P. R. Maurenzig; G. Pasquali; G. Poggi; A.A. Stefanini; R. Bougault; N. Le Neindre; O. Lopez; M. Parlog; E. Vient; E. Bonnet; A. Chbihi; J.D. Frankland; D. Gruyer; E. Rosato; G. Spadaccini; M. Vigilante; B. Borderie; M.F. Rivet; M. Bruno; L. Morelli; M. Cinausero; M. Degerlier; F. Gramegna; T. Marchi
Ti +
19th International School on Nuclear Physics, Neutron Physics and Applications, VARNA 2011 | 2012
A. Giaz; A. Corsi; F. Camera; A. Bracco; F. C. L. Crespi; S. Leoni; R. Nicolini; V. Vandone; G. Benzoni; N. Blasi; S. Brambilla; B. Million; O. Wieland; M. Cinausero; M. Degelier; F. Gramegna; V. L. Kravchuk; T. Marchi; V. Rizzi; L. Bardelli; S. Barlini; M. Bini; S. Carboni; G. Casini; M. Chiari; A. Nannini; G. Pasquali; S. Piantelli; G. Poggi; G. Baiocco
^{40}