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Phys. Rev. C 54, 1700–1709 (1996)

Total reaction and 2n-removal cross sections of 20–60A MeV 4,6,8He, 6–9,11Li, and 10Be on Si

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R. E. Warner, R. A. Patty, P. M. Voyles, A. Nadasen, F. D. Becchetti, J. A. Brown, H. Esbensen, A. Galonsky, J. J. Kolata, J. Kruse, M. Y. Lee, R. M. Ronningen, P. Schwandt, J. von Schwarzenberg, B. M. Sherrill, K. Subotic, J. Wang, and P. Zecher
National Superconducting Cyclotron Laboratory, East Lansing, Michigan 48824
Oberlin College, Oberlin, Ohio 44074
University of Michigan, Dearborn, Michigan 48128
University of Michigan, Ann Arbor, Michigan 48109
Argonne National Laboratory, Argonne, Illinois 60439
University of Notre Dame, Notre Dame, Indiana 46556
Indiana University Cyclotron Facility, Bloomington, Indiana 47405
Institute of Nuclear Sciences, VINCA, Belgrade 11001, Yugoslavia

Received 1 March 1996; published in the issue dated October 1996

Total reaction cross sections, σR, of 20–60A MeV 4,6,8He, 6–9,11Li, and 10Be were measured by injecting magnetically separated, focused, monoenergetic, identified secondary beams of those projectiles into a Si detector telescope and measuring their energy-deposition spectra. These σR’s, accurate to about 3%, were compared with predictions of optical, strong absorption, and microscopic models. The latter gave the best overall fit to the data, providing long-tailed matter densities were assumed. The best available optical potentials generally overpredicted the data by about 10%. Strong absorption calculations, in which the isospin-dependent term is quite important, were often unsuccessful, especially for projectiles with large neutron excess. Two-neutron removal cross sections were measured for 6He and 11Li; the 11Li data were slightly overpredicted by a microscopic model which includes correlation effects for the 11Li valence neutrons. Both 2n and 4n removal from 8He were observed, in about a 2:1 ratio. Subtraction analysis of the data indicates that 4He is a good core within 6He and 8He, as is 9Li within 11Li. © 1996 The American Physical Society.

© 1996 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevC.54.1700
DOI:
10.1103/PhysRevC.54.1700
PACS:
25.60.Dz, 25.70.Mn, 24.10.-i, 27.20.+n