Isotopically resolved fragments with Z < 20 have been studied with a high-resolution telescope in a test run for the FAZIA Collaboration. The fragments were produced by the collision of a 84Kr beam at 35 MeV/nucleon with a neutron-rich (124Sn) and a neutron-poor (112Sn) target. The fragments, detected close to the grazing angle, are mainly emitted from the phase-space region of the projectile. The fragment isotopic content clearly depends on the neutron richness of the target and this is direct evidence of isospin diffusion between projectile and target. The observed enhanced neutron richness of light fragments emitted from the phase-space region close to the center of mass of the system can be interpreted as an effect of isospin drift in the diluted neck region

S. Barlini, S. Piantelli, G. Casini, P. R. Maurenzig, A. Olmi, M. Bini, et al. (2013). Isospin transport in 84Kr+112,124Sn collisions at Fermi energies. PHYSICAL REVIEW. C, NUCLEAR PHYSICS, 87, 1-7 [10.1103/PhysRevC.87.054607].

Isospin transport in 84Kr+112,124Sn collisions at Fermi energies

BRUNO, MAURO;MORELLI, LUCA;
2013

Abstract

Isotopically resolved fragments with Z < 20 have been studied with a high-resolution telescope in a test run for the FAZIA Collaboration. The fragments were produced by the collision of a 84Kr beam at 35 MeV/nucleon with a neutron-rich (124Sn) and a neutron-poor (112Sn) target. The fragments, detected close to the grazing angle, are mainly emitted from the phase-space region of the projectile. The fragment isotopic content clearly depends on the neutron richness of the target and this is direct evidence of isospin diffusion between projectile and target. The observed enhanced neutron richness of light fragments emitted from the phase-space region close to the center of mass of the system can be interpreted as an effect of isospin drift in the diluted neck region
2013
S. Barlini, S. Piantelli, G. Casini, P. R. Maurenzig, A. Olmi, M. Bini, et al. (2013). Isospin transport in 84Kr+112,124Sn collisions at Fermi energies. PHYSICAL REVIEW. C, NUCLEAR PHYSICS, 87, 1-7 [10.1103/PhysRevC.87.054607].
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....espandi
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/200329
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