PREX/CREX May 2, 2018 10:00am

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  1. Tritium simulations: Adam haplog
    • AZ: indeed the shadow was due to the septum kryptonite detector.
    • AZ: we plan to measure the does at different locations (in particular close to the HRS platform or close the entrance of the dump)
  2. TOSCA update: Adam haplog
    • AZ: the script sent over by Jay works great, but I am still trying to understand the output
    • AZ: the dipole component seems to be consistent with what we had before and we can see a good reduction from the tritium Q1 shielding
    • AZ: the quadruple component seems to be wrong. JB: when you estimate the total quad component you need to divide by the distance between the points. KP: the plots show the cos0, cos1 components but we may be interpreting them badly. JB: the circles I use in the script are at 3cm so you need to divide by 3^n.
  3. SAM redesign - Cameron, Tao
    • CC: we are analyzing the output from a couple of designs. by next week will have tables with results.
    • KP: would vary the length of the can, thickness of the can (look at post in the elog for thickness)
    • TY: working on determining the signal level
    • KP: you should look at the dump elastomer (the plastic ring). AZ: detector 3201
  4. Other:
    • KP: a draft of the acc schedule should be released soon.


Eric K, Caryn P, Bob M, Jay B, Ciprian G, Adam Z, Kent P, Amali P, Dave G, Victoria O, Tao Y, Jinlong Z, Ryan R, Paul S, Dustin M, Silviu D, Seamus R, Devi A, Chandan G, Guido U, Cameron C,


Sanghwa P, David A, KK