Dynamical emission of heavy fragments in the 112,124Sn+58,64Ni reactions at 35 AMeV as seen with CHIMERA

A. Anzalone; A. Chbihi; A. Grzeszczuk; A. Pagano; A. Pop; A. Sochocka; A. Trifir`o; B. Borderie; C. Maiolino; D. Guinet; E. De Filippo; E. Galichet; E. Geraci; E. La Guidara; E. Piasecki; E. Rosato; F. Amorini; F. Giustolisi; F. Porto; F. Rizzo; G. Cardella; G. Lanzalone; G. Lanzan´o; G. Politi; I. Berceanu; I. Skwira Chalot; J. Blicharska; J. Brzychczyk; J. Frankland; J. P. Wieleczko; J. Wilczy´nski; K. Schmidt; K. Siwek Wilczy´nska; L. Auditore; L. Zetta; M. B. Chatterjee; M. Bruno; M. Colonna; M. Di Toro; M. D’Agostino; M. F. Rivet; M. Papa; M. Petrovici; M. Trimarchi; M. Vigilante; N. Le Neindre; P. Guazzoni; P. Russotto; R. Bougault; R. Dayras; R. Płaneta; S. Cavallaro; S. Kowalski; S. Pirrone; V. Baran; W. Gawlikowicz; W. Zipper; Z. Majka; Ł. ´ Swiderski

Dynamical emission of heavy fragments in the 112,124Sn+58,64Ni reactions at 35 AMeV as seen with CHIMERA

Abstract

A quantitative comparison regarding absolute cross sections associated to Statistical and Dynamical Fission in the system 124Sn+64Ni and112Sn+58Ni experimentally investigated at 35 AMeV beam energy is presented. It results that Dynamical Fission process is about two times more probable in the neutron rich 124Sn+64Ni system than in the 112Sn+58Ni neutron poor one. At this point of our analysis it is not clear if the observed difference is originated by different entrance channel Isospin (N/Z) content or by different size between the two investigated systems

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oai:air.unimi.it:2434/52548

Last time updated on 06/03/2019