Interactions of Relativistic Heavy Ions in Thick Heavy Element Targets and Some Unresolved Problems
Brandt R., Ditlov V.A., Dwivedi K.K., Ensinger W., Ganssauge E. Guo Shi-Lun,
Haiduc M., Hashemi-Nezhad S.R., Khan H.A., Krivopustov M.I., Odoj R., Pozharova E.A.,
Smirnitzki V.A., Sosnin A.N., Westmeier W., Zamani-Valasiadou M.
Interactions of relativistic heavy ions with total energies above 30 GeV in thick Cu and Pb targets
( 2 cm) have been studied with various techniques. Radiochemical irradiation experiments using thick
Cu targets, both in a compact form or as diluted "2p-Cu targets", have been carried out with several relativistic
heavy ions, such as 44 GeV 12C (JINR, Dubna) and 72 GeV 40Ar (LBL, Berkeley, USA). Neutron measuring experiments using
thick targets irradiated with various relativistic heavy ions up to 44 GeV 12C have been performed at the JINR. In addition,
the number of "black prongs" in nuclear interactions (due to protons with energies less than 30 MeV and emitted from the target-like
interaction partner at rest) produced with 72 GeV 22Ne ions in nuclear emulsion plates has been measured in the first nuclear interaction of the
primary 22Ne ions and in the following second nuclear interaction of the secondary heavy (Z > 1) ions. Some essential results
have been obtained. 1) Spallation products produced by relativistic secondary fragments in interactions ([44 GeV 12C or 72 GeV 40Ar] + Cu)
within thick copper yield less products close to the target and much more products far away from the target as compared to primary beam interactions.
This applies also to secondary particles emitted at large angles (Q > 10°).
2) The neutron production of 44 GeV 12C within thick Cu and Pb targets is beyond the estimated yield as based on experiments
with 12 GeV 12C. These rather independent experimental results cannot be understood with well-accepted nuclear reaction models.
They appear to present unresolved problems.
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