Proton Calorimetry/Meetings/2017/06/21: Difference between revisions
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'''ABF''': | '''ABF''': | ||
* Assembling photodiode circuit with Hamamatsu preamp. | |||
* Waiting on resistor value for preamp from Hamamatsu. | |||
'''Suggestions needed for our Water Equivalent range telescope plastic scintillator detector.''' | |||
; SciRT : '''Sci'''ntillating '''R'''ange '''T'''elescope |
Latest revision as of 15:09, 21 June 2017
Minutes for UCL Proton Calorimetry Meeting, 21st June 2017 (D17, Physics & Astronomy, UCL)
Present
Simon Jolly, Laurent Kelleter, Anastasia Basharina-Freshville, Ruben Saakyan, Phil Allport
LK:
- Looking further into nuclear build-up for energy variation:
- Relative reduction becomes constant at beam energies above 200 MeV: "saturation".
- RS suggests that nuclear interactions become important above 200 MeV: suggests to count numbers of all secondaries by species in the entrance region.
- PA suggests using a liquid Hydrogen target to simplify the nuclear interactions.
ABF:
- Assembling photodiode circuit with Hamamatsu preamp.
- Waiting on resistor value for preamp from Hamamatsu.
Suggestions needed for our Water Equivalent range telescope plastic scintillator detector.
- SciRT
- Scintillating Range Telescope