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Other Backgrounds

As indicated above, the most likely sources of background are those which produce a real slow track in the apparatus which did not come from the target. If this track has the right direction, it could be interpreted as a high rigidity (hence high mass) track from the target. If this track also points to a region of the calorimeter where coincidentally neutral particles have deposited substantial energy in the correct place with the correct time and energy, then the track could simulate a high mass object. Although such multiple overlapping processes are highly unlikely, if we want a sensitivity of order tex2html_wrap_inline1947 such processes must be considered. We have given a detailed analysis of interactions in the upstream detectors above. Here we consider a decay process.

If a centrally-produced tex2html_wrap_inline3743 travels through a significant part of the magnetic field and then decays, the decay proton will have a similar velocity and direction to the parent tex2html_wrap_inline3743 . However the decay proton will not have been bent in the magnetic field by a large enough angle (corresponding to its low momentum) and thus will appear to be a track with higher momentum and hence higher mass. Since the tex2html_wrap_inline3743 and the proton have similar velocities and directions and the tex2html_wrap_inline3743 is centrally produced, the proton track can otherwise appear to be a good late track coming from the target in space and time.

In order to produce a proton that reconstructs as a high mass particle the tex2html_wrap_inline3743 must pass through most of the magnetic field before decaying. In particular, tex2html_wrap_inline3743 's which survive to the end of the first magnet but decay before the second magnet will only give protons that reconstruct to about three times the proton mass. To get masses as high as 10 GeV/c tex2html_wrap_inline2169 , which would be a background for the strangelet search, the tex2html_wrap_inline3743 would have to survive more than 2/3 of the way through the second magnet or more than 7.5m from the target. Figure gif shows the proton kinematics from tex2html_wrap_inline3743 decay. The maximum rapidity of interest is 1.89, corresponding to a 3.02 GeV proton. From Fig. gif one can see that the maximum momentum for a tex2html_wrap_inline3743 which can produce such a proton is less than 4 GeV. For a 4 GeV tex2html_wrap_inline3743 the decay distance is tex2html_wrap_inline3765 =0.294m. The probability to survive 7.5m or 25.5 lifetimes is less than tex2html_wrap_inline1947 . Thus even without requiring any suppression from the calorimeter (the proton energy is wrong for a high mass particle by a large factor) or from the fact that there is no confirming hit in S1, this process is not a background.

  
Figure: tex2html_wrap_inline3743 decay kinematics. Horizontal axis (Theta) is lab. angle of proton with respect to tex2html_wrap_inline3743 direction and vertical axis is proton lab. momentum.

We have also considered possible backgrounds due to neutrons and protons from electromagnetic dissociation and due to nuclear fragments. Neither of these represent a significant background source. Coulomb dissociation products are very peripheral in nature, hence they have the wrong velocity (beam rapidity) and very low P tex2html_wrap_inline3337 so that they do not get into our apparatus. Heavy nuclear fragments have a low production cross section and tend to be produced at beam rapidity so they also pose no problem for this experiment. The details of both of these calculations are available in ``Update to P-864: Production of Rare Composite Objects in Relativistic Heavy Ion Collisions,'' October 1, 1990.


next up previous contents
Next: Summary of Run Plans Up: BackgroundsEfficiencies and Analysis Previous: Accidental Backgrounds: Multiple Interactions

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Tue Jan 21 17:29:21 EST 1997