By Heinz Sorge (auth.), Wolfgang Bauer, Alice Mignerey (eds.)
th The thirteen iciness Workshop on Nuclear Dynamics is the newest installment in a chain of workshops that was once began in 1978. This sequence has grown right into a culture, bringing jointly experimental and theoretical services from all parts of the learn of nuclear dynamics. As continuously, the organizers had positioned emphasis at the very important element of pass fertilization among the various power regimes and wa.ys of viewing a collision of full of life nuclei. This emphasis is mirrored within the vast variety of subject matters lined in those court cases. part transitions in nuclear collisions bought many of the awareness in this workshop, as indicated by means of the variety of contributions in this topic. a number of the questions in reference to those issues stay now not settled and should have a big impact at the physics that may be extracted from experiments on the destiny Relativistic Heavy Ion Collider. whereas the experimental software on the AGS is winding down, the NSCL improve and RHIC promise a vibrant destiny for our box within the united states. In Europe and Asia, significant new amenities are below development to boot. the buzz and anticipation in reference to those new possibilities are mirrored in those court cases besides. Wolfgang Bauer Michigan country college Alice Mignerey collage of Maryland v prior WORKSHOPS the next desk incorporates a checklist of the dates and destinations of the former wintry weather Workshops on Nuclear Dynamics in addition to the individuals of the organizing committees. The chairpersons of the meetings are underlined.
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T.. 6 10' .. ured l I ' ... ''9 o 1 -I o m,-m" Ie-V) Figure 8. Transverse energy spectra in various rapidity intervals, the slope parameters derived from them, and the rapidity distribution, all for negative pions produced in 6 A GeV Au+Au reactions. 22 Table 2. TPC Data Summary for Experiment E895 Energy 8 A GeV 6 A GeV 4 A GeV 2 A GeV Target Au [3%] Au [3%] Trigger Central Min. 0 Tesla Events 364 K 59 K Ag [3%] Ag [3%] Central Min. 0 Tesla 12 K 41 K Au [3%] Au [1%] Au [3%] Central Central Min.
Of course, in order to make a sensitive search one needs to do two things: (1) to credibly model what size the "expected" fluctuations would take, and (2) to predict the size (and frequency) of fluctuations that would result from a DCC being formed. In the WA9S preliminary DCC analysis these were carried out as follows. The VENUS simulation was used to model the basic Pb+ Pb central collisions; parameters were tuned until the predicted spectra for individual Ncharged and Nphoton per event agreed very well with the measured spectra, after which the joint distribution was presumed to model collisions in which no DCC is formed.
Accordingly, much effort has gone into looking for azimuthal asymmetries using detectors with wide coverage , and then looking for correlations between the axes of asymmetries measured with different kinds of particles or in different rapidity ranges. As a first step in such a program, a technique has been investigated in WAgS to identify a reaction plane direction using secondaries near target rapidity observed with the PBall. Each of the PBall's elements can identify the relatively low-energy (in the lab) secondaries by measuring their total kinetic energy in a thick scintillator and their velocity through ionization in a thin scintillator - the well-known E vs dE I dx match.