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Stopping relativistic Xe, Ho, Au and U nuclei in nuclear emulsionsNuclei of Xe-54, Ho-67, Au-79 and U-92 accelerated at the Bevalac to energies between 1200 and 900 MeV/n were stopped in nuclear emulsions. The observed residual ranges were compared with those calculated from various models of energy loss and shown to be most consistent with a calculation that includes those higher order correction terms proposed previously to describe the energy loss of highly charged particles, for which the first Born approximation is not valid.
Document ID
19850027563
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Waddington, C. J.
(Minnesota Univ. Minneapolis, MN, United States)
Fixsen, D. J.
(Minnesota Univ. Minneapolis, MN, United States)
Freier, P. S.
(Minnesota Univ. Minneapolis, MN, United States)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 6
Subject Category
Nuclear And High-Energy Physics
Accession Number
85N35876
Funding Number(s)
CONTRACT_GRANT: NGR-24-005-050
CONTRACT_GRANT: NAG8-500
CONTRACT_GRANT: NSF PHY-84-05852
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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