energy deposition for intense muon sources (chicane + the rest of the front end) pavel snopok...
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![Page 1: Energy deposition for intense muon sources (chicane + the rest of the front end) Pavel Snopok Illinois Institute of Technology and Fermilab December 4,](https://reader035.vdocument.in/reader035/viewer/2022062718/56649e8a5503460f94b8f27a/html5/thumbnails/1.jpg)
Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014)
Energy depositionfor intense muon sources
(chicane + the rest of the front end)
Pavel Snopok
Illinois Institute of Technology
and
Fermilab
December 4, 2014
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Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 2
Outline
• Introduction• History• Current MARS simulations
– new data files for solid target
• Using other codes (ICOOL and G4beamline)• Summary
December 4, 2014
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Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 3
Introduction
• In high-intensity sources muons are produced by firing high energy p onto a target to produce π.
• π decay to μ which are captured and accelerated.• Significant background from p and ē, which may result in
– heat deposition on superconducting materials;– activation of the machine preventing manual handling.
December 4, 2014
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Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 4
Introduction, contd.
• Need a secondary particle handling system for a megawatt class solid C target– solenoidal chicane– followed by a proton absorber.
• Challenges of optimization and integration of the system with the rest of the muon front end.
• Main study tool – MARS, some analysis and validation by using ICOOL and G4beamline.
• Start with the chicane, use the same technique downstream to study the the buncher and phase-rotator sections.
December 4, 2014
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History: MARS simulations
• ROOT-based geometry• 12.5° single bend, Z=0 corresponds to 19 m downstream of the target
– consistent with RDR (IDS-NF).
• W density reduced to 60% to take into account packing fraction for beads.
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Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 6
Reference: no shielding
December 4, 2014
DPD peaks at 15.8
mW/g, that translates
into 42.6 kW/m for Cu
coils or 33.3 kW/m for
SC coils.
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Uniform 35 cm shielding
Empty channel PD total, mW/g
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Non-uniform 30 and 40 cm shielding
Empty channel PD total, mW/g
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Overall DPD per coil/segment
Segmented coil analysis, total DPD, mW/g Average DPD per coil, mW/g
In both cases red line corresponds to 0.1 mW/g SC limit
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Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 10
Current MARS simulations
• New target parameters:– 8 GeV => 6.75 GeV– 4 MW => 1 MW– 3.125e15 protons/sec => 0.925e15 protons/sec– new particle distribution– need to re-run MARS
• The hope is that the new parameters help reduce the amount of shielding required
December 4, 2014
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New results
Muon flux, top view Muon flux, side view
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New results 2
Proton flux, top view Proton flux, side view
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New results 3
Deposited power density, mW/g,top view
Deposited power density, mW/g,side view
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New results 4
Deposited power density, mW/gsegmented coil analysis
Deposited power density, mW/gaveraged
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Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 15
Other codes
• Can G4beamline or ICOOL be used for energy loss/deposition calculations?
• Back in 2010 I did a comparison of the two codes for IDR:
December 4, 2014
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Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 16
Summary
• Simulations of the new 1 MW graphite target are underway, first results presented.– power density > 0.1 mW/g only in a handful of cental
coils, very low everywhere else;– definitely do not need 35 cm of tungsten.
• Action item: implement a more sophisticated geometry (elliptical cross-section following the profile of the beam).– this will allow to significantly reduce the amount of W
used for shielding.
• MARS is the main tool, although G4beamline and ICOOL can also be used for some analyses.
December 4, 2014
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Pavel Snopok | MAP Winter Collaboration Meeting (SLAC, December 3-7, 2014) 17
December 4, 2014
Thank you!