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Influence of entrance-channel magicity and isospin on quasi-fission

Authors :
Duc Huy Luong
Cedric Simenel
R. du Rietz
Cheng-Jian Lin
Mahananda Dasgupta
Maurits Evers
Aditya Wakhle
David Hinde
Department of Nuclear Physics (DNP)
Australian National University (ANU)
Département de Physique Nucléaire (ex SPhN) (DPHN)
Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU)
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay
Source :
Physics Letters B, Physics Letters B, Elsevier, 2012, 710, pp.607. ⟨10.1016/j.physletb.2012.03.063⟩, Physics Letters B, 2012, 710, pp.607. ⟨10.1016/j.physletb.2012.03.063⟩
Publication Year :
2012
Publisher :
HAL CCSD, 2012.

Abstract

The role of spherical quantum shells in the competition between fusion and quasi-fission is studied for reactions forming heavy elements. Measurements of fission fragment mass distributions for different reactions leading to similar compound nuclei have been made near the fusion barrier. In general, more quasi-fission is observed for reactions with non-magic nuclei. However, the $^{40}$Ca+$^{208}$Pb reaction is an exception, showing strong evidence for quasi-fission, though both nuclei are doubly magic. Time-dependent Hartree-Fock calculations predict fast equilibration of $N/Z$ in the two fragments early in the collision. This transfer of nucleons breaks the shell effect, causing this reaction to behave more like a non-magic one in the competition between fusion and quasi-fission. Future measurements of fission in reactions with exotic beams should be able to test this idea with larger $N/Z$ asymmetries.<br />accepted for publication in Physics Letters B

Details

Language :
English
ISSN :
03702693
Database :
OpenAIRE
Journal :
Physics Letters B, Physics Letters B, Elsevier, 2012, 710, pp.607. ⟨10.1016/j.physletb.2012.03.063⟩, Physics Letters B, 2012, 710, pp.607. ⟨10.1016/j.physletb.2012.03.063⟩
Accession number :
edsair.doi.dedup.....71bfbb30c1743c81acff8c09b00d0a07
Full Text :
https://doi.org/10.1016/j.physletb.2012.03.063⟩