https://doi.org/10.1051/epjconf/20100214002
Influence Of The Neutron Richness On Binary Decays
1
GANIL, CEA et IN2P3-CNRS, B.P. 55027, Caen Cedex, France
2
Dipartimento di Scienze Fisiche, Università di Napoli ”Federico
II”, I 80126,
Napoli, Italy
3
Dipartimento di Scienze Ambiantali, Università di Napoli,
I 81100, Caserta, Italy
4
Physics Division, Oak Ridge National Laboratory,
Oak Ridge, TN
37831, USA
5
IPHC, IN2P3-CNRS, F
67037, Strasbourg
Cedex2, France
6
IPNO IN2P3-CNRS and Université Paris-Sud 11, F-91406, Orsay Cedex, France
7
LPC, IN2P3-CNRS, ENSICAEN and Université, F-14050, Caen
Cedex, France
8
CEA, IRFU, SPhN, CEA/Saclay, F-91191, Gif
sur Yvettes Cedex, France
9
NFN, LNL, I
35020
Legnaro (Padova)
Italy
10
IPNL, IN2P3-CNRS et Université, F-69622, Villeurbanne Cedex, France
11
Dipartimento di Scienze Fisiche, Università di Napoli ”Federico
II”, I 81100,
Caserta, Italy
12
Laboratoire de Physique Nucléaire Université de Laval,
Québec, Canada
a e-mail: ademard@ganil.fr
The influence of the neutron richness on binary decays is investigated in 78,82Kr+ 40Ca reactions at 5.5 MeV/A incident energy. Kinetic energy distributions and angular distributions of fragments with atomic number 6 ≤ Z ≤ 28 were measured using the 4π-INDRA array. Global features are compatible with an emission from a long-lived system. The yields around the symmetric splitting are about 30The persistence of strong structural effects is evidenced from elemental cross-sections of the light fragments. The cross-sections for odd-Z fragments are higher for the neutron rich CN while cross-sections for even-Z fragments are higher for the neutron poor CN. Calculations assuming two different potential energy surfaces are presented.
© Owned by the authors, published by EDP Sciences, 2010