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

Journal Article · Fri Nov 01 04:00:00 EST 1985 · Phys. Rev. A; (United States)

DOI:https://doi.org/10.1103/PhysRevA.32.3102· OSTI ID:5006092

Waddington, C J; Fixsen, D J; Freier, P S

Nuclei of /sub 54/Xe, /sub 67/Ho, /sub 79/Au, and /sub 92/U accelerated at the Lawrence Berkeley Laboratory Bevalac to energies between 1200 and 900 MeV/n have been stopped in nuclear emulsions. The observed residual ranges have been 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.

• Research Organization: School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455
• OSTI ID: 5006092
• Journal Information: Phys. Rev. A; (United States), Journal Name: Phys. Rev. A; (United States) Vol. 32:5; ISSN PLRAA
• Country of Publication: United States
• Language: English

Related Subjects

654001* -- Radiation & Shielding Physics-- Radiation Physics
Shielding Calculations & Experiments
73 NUCLEAR PHYSICS AND RADIATION PHYSICS
ACTINIDE ISOTOPES
ACTINIDE NUCLEI
ALPHA DECAY RADIOISOTOPES
CHARGED-PARTICLE TRANSPORT
ENERGY LOSSES
ENERGY RANGE
EVEN-EVEN NUCLEI
EVEN-ODD NUCLEI
GEV RANGE
GEV RANGE 100-1000
GOLD 197
GOLD ISOTOPES
HEAVY NUCLEI
HOLMIUM 165
HOLMIUM ISOTOPES
INTERMEDIATE MASS NUCLEI
ISOMERIC TRANSITION ISOTOPES
ISOTOPES
LOSSES
NUCLEAR EMULSIONS
NUCLEI
ODD-EVEN NUCLEI
RADIATION TRANSPORT
RADIOISOTOPES
RANGE
RARE EARTH ISOTOPES
RARE EARTH NUCLEI
SECONDS LIVING RADIOISOTOPES
STABLE ISOTOPES
URANIUM 238
URANIUM ISOTOPES
XENON 132
XENON ISOTOPES
YEARS LIVING RADIOISOTOPES