EARLY HISTORYMy story (which only concerns experiments with which 1 have been associated) starts in the late 60's at the Bevatron, where I was studying high energy proton-nucleus collisions such as 5.5 GcV protons on uranium. With small silicon dE/dx-E telescopes, we were measuring energy spectra at various angles to the beam of what were then called the fragmentation products produced from high deposition energy reactions. These reactions we would now call cvsntral proton-nucleus collisions. The so-called fragmentation products, helium up through carbon or nitrogen, we would now call intermediate mass fragments. Earl Hyde and I studied these reactions systematically (see Fig. 1), measuring the energy spectra and angular distributions of all the isotopes. 1 There were several anomalies shown which are still not completely understood. These included the apparent low Coulomb barriers, the high "temperatures", and the higher "temperatures" for the neutron deficient isotopes. In addition, the angular distributions were forward peaked in the moving system deduced from the shifts in the energy spectra. In 1974 deuteron and alpha particle beams arrived at 2.1 GeV/nucleon. Although the yields of these -1-fragmentation products were higher, the energy spectra displayed apparent temperatures that were only very slightly higher.
2The small differences produced by the alpha beams compared to proton beams were disappointing. In 1974 the transfer lino was completed connecting the SupcrHILAC to the Bevatron, creating the Bevalac which could produce 2 GeV/nucleon heavy ions an energy more than 100 times higher than previously available. Initially the heaviest beam was oxygen, but the mass increased later to neon. In this new energy regime it was hard to imagine what to expect. Because this field of relativistic heavy io< physics was completely new to all of us, group meetings were very exciting, as everybody contributed on an equal basis. Nobody had any experience and the young people, as you will see, participated equally with the more senior people.
THE GSI-LBL
SHOCK WAVES?While the large area silicon-germanium telescope was being planned and built, Prof. Schopper reported his shock wave peaks in AgCI track detectors irradiated by 0.9 GeV/nucleon oxygen ions.
3In his angular distributions he observed a broad peak with small narrower peaks superimposed. We decided to proceed quickly to verify this. We took a 5 cm thick piece of plastic scintillator, slapped it on a phototube, put a 1 mm thick Li drift silicon detector in front of it, and placed it in my existing scattering chamber (see Fig. 2). This silicon-plastic telescope was designed to look for ^He and 4 He fragments. We used a 1 GeV/nucleon oxygen beam to irradiate a silver target in order to approximate the conditions of the silver chloride track detectors. Our results 4 in 1975 when plotted (see Fig. 3 top) as do7d9 showed a nice broad peak at about 60 degrees in the laboratory, similar to the data of Prof. Schoppcr. However, plotting the data (sec Fig. 3 bottom) as dc...