Stopping relativistic Xe, Ho, Au and U nuclei in nuclear emulsions

Details Stopping relativistic Xe, Ho, Au and U nuclei in nuclear emulsions Stopping relativistic Xe, Ho, Au and U nuclei in nuclear emulsions

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....6..104w&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 6 p 104-107 (SEE N85-35848 24-93)

Physics

Nuclear Physics

Gold, Holmium, Isotopes, Nuclear Emulsions, Nuclei (Nuclear Physics), Uranium, Xenon, Born Approximation, Energy Dissipation, Particle Accelerators

Scientific paper

Nuclei 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.

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