Title
Near-Barrier Fusion of the (8)B+(58)Ni Proton-Halo System
Authors
E. F. Aguilera, Institute Nacl Invest Nuclear
P. Amador-Valenzuela, Institute Nacl Invest Nuclear
E. Martinez-Quiroz, Institute Nacl Invest Nuclear
D. Lizcano, Institute Nacl Invest Nuclear
P. Rosales, Institute Nacl Invest Nuclear
H. Garcia-Martinez, Institute Nacl Invest Nuclear
A. Gomez-Camacho, Institute Nacl Invest Nuclear
J. J. Kolata, University of Notre Dame
A. Roberts, University of Notre Dame
L. O. Lamm, University of Notre
G. Rogachev, University of Notre Dame
V. Guimaraes, University of Sao Paulo
F. D. Becchetti, University of Michigan - Ann Arbor
A. Villano, University of Michigan - Ann Arbor
M. Ojaruega, University of Michigan - Ann Arbor
M. Febbraro, University of Michigan - Ann Arbor
Y. Chen, University of Michigan - Ann Arbor
H. Jiang, University of Michigan - Ann Arbor
Paul DeYoung, Hope CollegeFollow
Graham F. Peaslee, Hope CollegeFollow
C. Guess, Hope College
U. Khadka, Hope College
J. Brown, Wabash College
J. D. Hinnefeld, Indiana University - South Bend
L. Acosta, Universidad de Huelva
E. S. Rossi Jr., UNIFIEO
J. F. P. Huiza, Universidade Estadual do Sudoeste da Bahia
T. L. Belyaeva, Universidad Autónoma del Estado de México
Publication Date
8-24-2011
Publication Source
Physical Review Letters
Publisher
American Physical Society
Abstract
Fusion cross sections were measured for the exotic proton-halo nucleus (8)B incident on a (58)Ni target at several energies near the Coulomb barrier. This is the first experiment to report on the fusion of a protonhalo nucleus. The resulting excitation function shows a striking enhancement with respect to expectations for normal projectiles. Evidence is presented that the sum of the fusion and breakup yields saturates the total reaction cross section.
Keywords
nuclear reactions, coulomb barrier, breakup, energies
Recommended Citation
Published in: Physical Review Letters, Volume 107, Issue 9, August 24, 2011. Copyright © 2011 American Physical Society, College Park, MD. The final published version is available at: http://dx.doi.org/10.1103/PhysRevLett.107.092701
