The isovector imaginary neutron potential: A key ingredient for the r-process nucleosynthesis

被引:42
作者
Goriely, S.
Delaroche, J.-P.
机构
[1] Univ Libre Brussels, Inst Astron & Astrophys, Brussels, Belgium
[2] CEA, DAM Ile De France, DPTA, Serv Phys, F-91680 Bruyeres Le Chatel, France
关键词
neutron optical potential; Hauser-Feshbach cross section; r-process;
D O I
10.1016/j.physletb.2007.07.046
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The isovector contribution to the imaginary component of the microscopic optical model potential is adjusted on experimental neutron strength function data. Within the Bruckner-Hartree-Fock approximation of Jeukenne-Lejeune-Mahaux, it is shown that experimental data favours a strong isovector component that can have a drastic impact on the radiative neutron capture cross section for neutron-rich nuclei. If confirmed, this result strongly inhibits the resonant capture by exotic nuclei, so that the traditional r-process picture of the fast neutron captures during the nucleosynthesis r-process needs to be revisited in depth. (c) 2007 Elsevier B.V. All rights reserved.
引用
收藏
页码:178 / 183
页数:6
相关论文
共 21 条
[1]   Microscopic nuclear models for astrophysics: The Brussels BRUSLIB nuclear library and beyond [J].
Arnould, M. ;
Goriely, S. .
NUCLEAR PHYSICS A, 2006, 777 :157-187
[2]  
ARNOULD S, 2007, IN PRESS PHYS REP
[3]   Nucleon-nucleus optical potential in the particle-hole approach [J].
Barbieri, C ;
Jennings, BK .
PHYSICAL REVIEW C, 2005, 72 (01)
[4]   Lane-consistent, semimicroscopic nucleon-nucleus optical model [J].
Bauge, E ;
Delaroche, JP ;
Girod, M .
PHYSICAL REVIEW C, 2001, 63 (02) :17
[5]   Semimicroscopic nucleon-nucleus spherical optical model for nuclei with A≥40 at energies up to 200 MeV [J].
Bauge, E ;
Delaroche, JP ;
Girod, M .
PHYSICAL REVIEW C, 1998, 58 (02) :1118-1145
[6]  
BAUGE E, COMMUNICATION
[7]  
DELAROCHE JP, 1976, CONS M US NUCL THEOR, V1, P251
[8]   Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas; VI: Weakened pairing [J].
Goriely, S. ;
Samyn, M. ;
Pearson, J. M. .
NUCLEAR PHYSICS A, 2006, 773 (3-4) :279-299
[9]   Microscopic HFB plus QRPA predictions of dipole strength for astrophysics applications [J].
Goriely, S ;
Khan, E ;
Samyn, M .
NUCLEAR PHYSICS A, 2004, 739 (3-4) :331-352
[10]  
Goriely S, 1997, ASTRON ASTROPHYS, V325, P414