Correlations between emission timescale of fragments and isospin dynamics in 124Sn+64Ni and112Sn+58Ni reactions at 35A MeV

De Filippo, E.; Pagano, A.; Russotto, P.; Amorini, F.; Anzalone, A.; Auditore, L.; Baran, V.; Berceanu, I.; Borderie, B.; Bougault, R.; Bruno, M.; Cap, T.; Cardella, G.; Cavallaro, S.; Chatterjee, M. B.; Chbihi, A.; Colonna, M.; D'Agostino, M.; Dayras, R.; Di Toro, M.; Frankland, J.; Galichet, E.; Gawlikowicz, W.; Geraci, E.; Grzeszczuk, A.; Guazzoni, P.; Kowalski, S.; La Guidara, E.; Lanzalone, G.; Lanzanò, G.; Le Neindre, N.; Lombardo, Ivano; Maiolino, C.; Papa, M.; Piasecki, E.; Pirrone, S.; Płaneta, R.; Politi, G.; Pop, A.; Porto, F.; Rivet, M. F.; Rizzo, F.; Rosato, Elio; Schmidt, K.; Siwek Wilczyńska, K.; Skwira Chalot, I.; Trifirò, A.; Trimarchi, M.; Verde, G.; Vigilante, Mariano; Wieleczko, J. P.; Wilczyński, J.; Zetta, L.; Zipper, W.

doi:10.1103/PhysRevC.86.014610

We present a new experimental method to correlate the isotopic composition of intermediate mass fragments (IMF) emitted at midrapidity in semiperipheral collisions with the emission timescale: IMFs emitted in the early stage of the reaction show larger values of N/Z isospin asymmetry, stronger angular anisotropies, and reduced odd-even staggering effects in neutron to proton ratio N/Z distributions than those produced in sequential statistical emission. All these effects support the concept of isospin “migration”, that is sensitive to the density gradient between participant and quasispectator nuclear matter, in the so called neck fragmentation mechanism. By comparing the data to a stochastic mean field (SMF) simulation we show that this method gives valuable constraints on the symmetry energy term of nuclear equation of state at subsaturation densities. An indication emerges for a linear density dependence of the symmetry energy.

Correlations between emission timescale of fragments and isospin dynamics in 124Sn+64Ni and112Sn+58Ni reactions at 35A MeV / E., De Filippo; A., Pagano; P., Russotto; F., Amorini; A., Anzalone; L., Auditore; V., Baran; I., Berceanu; B., Borderie; R., Bougault; M., Bruno; T., Cap; G., Cardella; S., Cavallaro; M. B., Chatterjee; A., Chbihi; M., Colonna; M., D'Agostino; R., Dayras; M., Di Toro; J., Frankland; E., Galichet; W., Gawlikowicz; E., Geraci; A., Grzeszczuk; P., Guazzoni; S., Kowalski; E., La Guidara; G., Lanzalone; G., Lanzanò; N., Le Neindre; Lombardo, Ivano; C., Maiolino; M., Papa; E., Piasecki; S., Pirrone; R., Płaneta; G., Politi; A., Pop; F., Porto; M. F., Rivet; F., Rizzo; Rosato, Elio; K., Schmidt; K., Siwek Wilczyńska; I., Skwira Chalot; A., Trifirò; M., Trimarchi; G., Verde; Vigilante, Mariano; J. P., Wieleczko; J., Wilczyński; L., Zetta; W., Zipper. - In: PHYSICAL REVIEW. C, NUCLEAR PHYSICS. - ISSN 0556-2813. - STAMPA. - 86:1(2012), pp. 1-7. [10.1103/PhysRevC.86.014610]