Cosmic ray events with high multiplicity
For my Cosmic rays study, version 2 I was combining all possible pairs of tracks in events with 2 or more global tracks. I made some plots to understand where the tracks were going though the TPC and was surprised by some structures in the plots of z positions.
In these plots, zouter is the z of the outermost (or last) hit on the track, and zinner is the z of the innermost (or first) hit. The "matching" requirement is that tracks are back-to-back in both azimuth φ and polar angle θ.
Here are plots of:
Top-left: zouter,1 vs. zouter,2 {matching}
Top-right: zinner,1 vs. zinner,2 {matching}
Bottom-left: zouter,1 vs. zouter,2
Bottom-right: zinner,1 vs. zinner,2
Here we see structure in these distributions using the TOF group of data:
The structures seem particular to events with high multiplicity (some events have thousands of tracks). Here we see the structures for track pairs from events with 5 or more tracks:
I believe these are due to Au+X events at low energy, generated when C-AD was trying to see if it could deliver AuAu beams at 5 GeV.
After removing these events with 5 or more tracks, the distributions look much better. I include here both the TOF group of triggers (left) and MTD group (right). Such high multiplicity events are thus to be excluded from the cosmic ray study.
-Gene
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