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HIJET/GEANT Simulations

As indicated above, we used HIJET to simulate Au-Au interactions. The parameter CENTRA was set to 5 for most of our studies. This selects the central few percent of the cross section, which is expected to correspond to events selected by our multiplicity trigger. In addition, HIJET includes secondary interactions, the nucleon Fermi momentum distribution, and uses a Wood-Saxon nucleon potential. The rescattering parameter was set to 3.25, which reproduces existing AGS multiplicity data.

For single particle production we used the following model:

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where:

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with cutoffs:

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GEANT is used to track particles produced by either generator through the apparatus. All physics processes were turned on in GEANT; these include Gaussian multiple scattering, decays, hadronic interactions, Compton scattering, pair production, and positron annihilation. Energy loss with Landau fluctuations including tex2html_wrap_inline3297 -ray production is used to compute the energy deposited in the tracking detectors. The arrival time for each energy deposition is also calculated. All interactions in the collimators, magnet pole tips, vacuum chamber walls, etc. were simulated for the shielding hits library. Finally, standard GEANT momentum cutoffs were used. Studies showed that the results did not change if the momentum cutoffs were lowered.

The output from GEANT was stored in the form of ``hits banks'' for each detector for each event. The hits files have x, y, z, TOF, tex2html_wrap_inline3299 E for each particle which deposits energy in a detector.

To give a feeling for the nature of the events from the simulation we show a typical event. Figure gif shows the spectrometer magnets, collimator, part of the vacuum chamber, and the detectors as described in GEANT. In Fig. gif a typical central Au-Au interaction is shown overlaid on the detector. One can see

  
Figure: E864 Apparatus as entered into GEANT.

  
Figure: Typical central Au-Au interaction tracked by GEANT through the E864 Apparatus. Dashed or dotted lines are neutral particles.

  
Figure: Central Au-Au interaction with tracks from shielding included. Dashed or dotted lines are neutral particles

that interactions in the detectors and air are included. In Fig. gif tracks from the collimators and other non-detector material are included. One should note that these figures are highly anamorphic - hence the appearance of very wide angle tracks from the shielding is somewhat deceiving. Dotted or dashed lines represent neutral particles and particle trajectories are not drawn inside the magnet iron or shielding. Figure gif shows the longitudinal origin of all proton and neutron tracks which produced hits in any detector from GEANT tracing a sample of HIJET central Au-Au collisions. (Tracks from shielding interactions are not included in this plot.) There are a total of

  
Figure: Longitudinal origin of all proton and neutron tracks which produced hits in any detector from GEANT tracing a sample of HIJET central Au-Au collisions. (Horizontal scale is meters from target.)

3.88 x 10 tex2html_wrap_inline3301 tracks in the histogram. Almost 2/3 of these tracks come from the interaction target. The remaining 1/3 come from decays and interactions in the detectors, vacuum window and air downstream of the vacuum window. All these processes are included in our simulations.

Table gif gives the average number of hits in the detectors for various types of events. As noted in the section on ``Magnets, Collimators and Vacuum Chamber'' there is a significant increase in the number of particles entering the calorimeter (about a factor of 2) due to the interactions in the collimators and shielding, but almost all of the increase is from very low energy photons which should have little effect on the performance of the calorimeter.

   table595
Table: Average hit multiplicities for central events in the E864 detectors with and without extra track from showers in the shielding.(Parentheses show RMS spreads.)


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Next: Time of Flight Simulation Up: Monte Carlo Simulations Previous: Monte Carlo Simulations

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Tue Jan 21 17:29:21 EST 1997