Difference between revisions of "Technical Board Meeting Oct 23, 2023"
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Back to [[Main_Page|Main Page]] >> [[Technical_Board | Technical Board]] | Back to [[Main_Page|Main Page]] >> [[Technical_Board | Technical Board]] | ||
− | [[Technical_Board_Meeting_Sept_18,_2023 | Technical Board Meeting September 18, 2023 ]] << >> [[ | + | [[Technical_Board_Meeting_Sept_18,_2023 | Technical Board Meeting September 18, 2023 ]] << >> [[Technical_Board_Meeting_Jan_23,_2024 | Technical Board Meeting January 23, 2024 ]] |
Online: see email | Online: see email | ||
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=Attendance= | =Attendance= | ||
− | + | Present: | |
− | * Kent Paschke, Chair (MOLLER Scientific Coordinator) | + | *Kent Paschke, Chair (MOLLER Scientific Coordinator) |
− | * Krishna Kumar (MOLLER Spokesperson) | + | *Krishna Kumar (MOLLER Spokesperson) |
− | * Mark Pitt (Deputy Spokesperson, MOLLER-NSF Project Coordinator) | + | *Mark Pitt (Deputy Spokesperson, MOLLER-NSF Project Coordinator) |
− | * Ruben Fair (DOE Project Manager) | + | *Ruben Fair (DOE Project Manager) |
− | * Klaus Dehmelt (Deputy DOE Project Manager) | + | *Klaus Dehmelt (Deputy DOE Project Manager) |
− | * Michael Gericke (MOLLER-CFI Project Coordinator) | + | *Michael Gericke (MOLLER-CFI Project Coordinator) |
− | * | + | *Mark Jones (Hall A Leader) |
− | * | + | *David Armstrong (Elected Executive Board Member) |
+ | *Dave Meekins (L2 CAM: Target) | ||
+ | *Carl Zorn (L2 CAM: Detectors) | ||
+ | *Ciprian Gal (L2 CAM: Infrastructure) | ||
+ | *Robert Michaels (L2 CAM: DAQ) | ||
+ | *Vladimir Berdnikov (L2 CAM: Installation) | ||
+ | *Silviu Covrig (Working Group Convener: Target) | ||
+ | *Dustin McNulty (Working Group Convener: Integrating Detectors) | ||
+ | *Paul King (Working Group Convener: DAQ) | ||
+ | *Jim Napolitano (Working Group Convener: Polarimetry) | ||
+ | *Eric Sun (joined for technical assistance) | ||
+ | |||
+ | Not attending: | ||
+ | *Juliette Mammei (Executive Board International Representative) | ||
* Paul A Souder (Elected Executive Board Member) | * Paul A Souder (Elected Executive Board Member) | ||
− | |||
* Robin Wines (Project Engineer) | * Robin Wines (Project Engineer) | ||
− | + | *Mike Dion (L2 CAM: Spectrometer) | |
− | * Mike Dion (L2 CAM: Spectrometer | + | *Caryn Palatchi (Working Group Convener: Polarized Beam) |
− | + | *Nilanga Liyanage (Working Group Convener: Tracking Detectors) | |
− | + | *Rakitha Beminiwattha (Working Group Convener: Simulations) | |
− | + | *Yury Kolomensky (Working Group Convener: Physics Extraction) | |
− | + | ||
− | + | ||
− | * Caryn Palatchi | + | |
− | + | ||
− | + | ||
− | * Nilanga Liyanage | + | |
− | + | ||
− | * Rakitha Beminiwattha (Working Group Convener: Simulations) | + | |
− | * Yury Kolomensky (Working Group Convener: Physics Extraction) | + |
Latest revision as of 20:47, 18 January 2024
Back to Main Page >> Technical Board
Technical Board Meeting September 18, 2023 << >> Technical Board Meeting January 23, 2024
Online: see email
Agenda
- Scattering chamber exit window design and lead time [Dave Meekins] Slides
- Effect of Aluminum Scagttering chamber exit window on MOLLER backgrounds Ciprian docdb:1172
- Physics evaluation of Drift pipe end cap design change [Kent] docdb:1171
Minutes
Drift pipe end:
- Drift pipe end cap was "dish" shaped, about 1" thick, to avoid an excessively thick wall. This added cost and schedule concerns, which can be relieved with a flat, 3" thick flange.
- There is a 5" thick wall just upstream of this, at the end of the downstream torus vacuum enclosure.
- Simulations confirm this understanding: the additional thickness at the upstream end of the drift pipe do not add significantly to backgrounds.
- There might even be a very small benefit, but at this level the statistical significance of the simulation is not fully sufficient.
Scattering Chamber Exit Window:
Cip: Physics simulation
- added Al window at the scattering chamber exit
- found that 400micron roughly doubles the total Al contributions from the target windows. The additional contribution is consistent with linear scaling with thickness of the scattering chamber windown
- "deconvolution" results don't degrade, but this is based on assumptions of Al fractions and asymmetries being perfectly known
- In fact, Al corrections will be uncertain at the 10% level due to uncertainty in the Al asymmetry
- Qweak measured APV to 10% (Note in chat: SM coupling known better than this, so this would be a worst-case limit for knowledge of asymmetry.)
- DA: what about uncertainty in rate?
- rates with gas-filled target are hard to get, since knowing the gas density was difficulty
- KK: simulation is required, other studies will be possible
- KK : Be window would be very valuable to have, even if installed later. So we should keep this development alive, even if we got with the Al window to start Run1.
Meekins:
- delivery is not going to be available from previous vendor.
- Materian (now purchased and absorbed into another company) will no longer provide flanges.
- Al is easy, but Be is difficult
- Be brazing is possible, (in conversation with WessDel) but this is also challenging to move forward due to inconsistent vendor response.
- This would require the experiment is accept brazing alloy of zinc/Al
- Be: better thermal conduction, better cyclic loading, low Z for backgrounds
- Aim to prepare to handle 20psi load if H2 cell failure. 15pse for atmosphere
- Dishing is required, allows for relief of mechanical stress under thermal load
- This design has 10 mils in vacuum window, 25 mils in 3" diameter for accepted scattered particles
- Old window, was about 1 calendar year replacement cycle at 10trips/hr
- new design is probably much better, but not so clear yet. Now looking at 70k cycles compared to 45k in flat design.
- status: "Its done", this can be built in machine shop.
- May need to make several to meet thickness goals, with reasonably small variation. There are measurement tools to know what we have well.
- KK: Summary from the experiment side: we would prefer Be window to improve physics, but we are ok with this Al design even for full experiment.
Attendance
Present:
- Kent Paschke, Chair (MOLLER Scientific Coordinator)
- Krishna Kumar (MOLLER Spokesperson)
- Mark Pitt (Deputy Spokesperson, MOLLER-NSF Project Coordinator)
- Ruben Fair (DOE Project Manager)
- Klaus Dehmelt (Deputy DOE Project Manager)
- Michael Gericke (MOLLER-CFI Project Coordinator)
- Mark Jones (Hall A Leader)
- David Armstrong (Elected Executive Board Member)
- Dave Meekins (L2 CAM: Target)
- Carl Zorn (L2 CAM: Detectors)
- Ciprian Gal (L2 CAM: Infrastructure)
- Robert Michaels (L2 CAM: DAQ)
- Vladimir Berdnikov (L2 CAM: Installation)
- Silviu Covrig (Working Group Convener: Target)
- Dustin McNulty (Working Group Convener: Integrating Detectors)
- Paul King (Working Group Convener: DAQ)
- Jim Napolitano (Working Group Convener: Polarimetry)
- Eric Sun (joined for technical assistance)
Not attending:
- Juliette Mammei (Executive Board International Representative)
- Paul A Souder (Elected Executive Board Member)
- Robin Wines (Project Engineer)
- Mike Dion (L2 CAM: Spectrometer)
- Caryn Palatchi (Working Group Convener: Polarized Beam)
- Nilanga Liyanage (Working Group Convener: Tracking Detectors)
- Rakitha Beminiwattha (Working Group Convener: Simulations)
- Yury Kolomensky (Working Group Convener: Physics Extraction)