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Harold G. Kirk Brookhaven National Laboratory Target Baseline IDS-NF Plenary CERN March 23-24, 2009
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Harold G. Kirk The Neutrino Factory Target Concept
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Harold G. Kirk Iron Plug Proton Beam Nozzle Tube SC-1 SC-2 SC-3SC-4 SC-5 Window Mercury Drains Mercury Pool Water-cooled Tungsten Shield Mercury Jet Resistive Magnets Neutrino Factory Study 2 Target Concept ORNL/VG Mar2009 Splash Mitigator Path toward a Target System Design
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Harold G. Kirk Alternative Collection System Another containment approach includes a shortened Hg container Drain lines exit cryostat between SC-3 and SC-4 This would trap container in the cryostat, preventing future replacement
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Harold G. Kirk The Hg Jet Nozzle Nozzle performance: The Issue
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Harold G. Kirk The Jet/Beam Dump Interaction T. Davonne, RAL
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Harold G. Kirk Fluka Simulation - Energy deposition in mercury pool with 24GeV beam How much of the beam energy is absorbed in the beam dump? T. Davonne, RAL
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Harold G. Kirk Eruption of mercury pool surface due to 24GeV proton beam Autodyne simulation Splash following pulse of 20Terra protons
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Harold G. Kirk Splash Mitigation Study 2 assumed a particle bed of tungsten balls to minimize effects of jet entering pool Many other feasible concepts to accomplish this function Simulation/analytical studies may be useful to limit options Pool circulation and drainage locations also need to be studied Prototypic testing needed for comparison & final determination
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Harold G. Kirk Containment Design Requirements Material compatible with high-field magnets l Must also withstand some number of full-power beam pulses with no Hg in vessel (accident scenario) Desire no replaceable components Provide support for Hg weight l ~220 liters, 3 metric tons Sloped (1°-2°) for gravity drain Overflow drain for 20m/s jet (1.6 liter/s) Vent for gas transfer
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Harold G. Kirk Toward a Target Prototype l Esatablish a coherent, engineered design concept l Design and test an improved nozzle l Design an Hg handling system l Design and test a CW Hg delivery system l Design, fabricate and beam test a target prototype
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Harold G. Kirk Hg Jet Target Geometry Previous results: Radius 5mm, θ beam =67mrad Θ crossing = 33mrad
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Harold G. Kirk The Target/Collection System Count all the pions and muons that cross the transverse plane at z=50m. For this analysis we select all pions and muons with 40 < KE< 180 MeV.
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Harold G. Kirk 50GeV Beam-Mesons at 50m 40MeV<KE<180MeV
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Harold G. Kirk Mesons at 50m Mesons/ProtonMesons/Proton normalized to beam power ISS Results reported April, 2006 Fixed Parameters: R=5mm; Beam Angle=67mrad; Jet/Beam = 33mrad
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Harold G. Kirk Vary the Target Radius
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Harold G. Kirk Optimized Target Radius 2 to 100 GeV
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Harold G. Kirk Beam Angle and Jet/Beam Crossing Angle Beam Angle Crossing Angle
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Harold G. Kirk Mars14 vs Mars15 Comparison
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Harold G. Kirk Normalized to Beam Power
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Harold G. Kirk Normalized to Peak
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Harold G. Kirk Summary l Peak meson production efficiency for a Neutrino Factory Hg Target system occurs in the region of 6 to 8 GeV l At 20 GeV we have a 25% loss in efficiency l At 40 GeV we have a 45% loss in efficiency l At 80 GeV we have a 50% loss in efficiency
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Harold G. Kirk Backup Slides
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Harold G. Kirk Optimized Target Parameters Target RadiusBeam Angle Beam/Jet Crossing angle
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Harold G. Kirk Optimized Target Parameters Target Radius Proton Beam Angle
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Harold G. Kirk Beam/Jet Crossing Angle
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Harold G. Kirk Meson Production Normalized to Beam Power
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Harold G. Kirk Process mesons through Cooling Consider mesons within acceptance of ε ┴ = 30π mm and ε L = 150π mm after cooling 180 MeV
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Harold G. Kirk Compare 50m to Post-Cooling
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Harold G. Kirk Step 1: Vary the Target Radius Rmax=0.48cm
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Harold G. Kirk Proton Driver Parameters Proton driver power: 4 MW Proton driver repetition rate: 50 Hz Proton energy: around 10 GeV 3 proton bunches in train l 1.7×10 13 protons per bunch at 10 GeV Bunch length 1 – 3 ns Train length at least 200 μs
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Harold G. Kirk Optimizing Soft-pion Production
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Harold G. Kirk Step 2: Vary the Beam Angle beam =89mrad
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Harold G. Kirk Step 3: Vary the Beam/Jet Crossing Angle crossing =25mrad
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Harold G. Kirk Post-cooling 30π Acceptance
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