High-pressure gaseous argon
in the DUNE near detector
High-pressure gaseous argon in the DUNE near detector Andy - - PowerPoint PPT Presentation
High-pressure gaseous argon in the DUNE near detector Andy Furmanski, on behalf of the DUNE collaboration CPAD 2019 Madison, Wisconsin DUNE D eep U nderground N eutrino E xperiment: Next-gen long-baseline neutrino oscillation experiment
in the DUNE near detector
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ArgonCube: Liquid argon (LAr) Multi-Purpose Detector (MPD): Gaseous argon (GAr) 3D scintillator tracker (SAND): Hydrocarbon LAr+GAr move off- axis: PRISM A highly capable near detector complex is critical for reducing flux and cross section uncertainties for DUNE’s physics goals!
Neutrinos coming from the right
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– Lower thresholds – Fewer showers
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– Magnet provides good momentum measurement for all particles – Liquid near detector is too small to contain many events
Far detector acceptance LAr near detector acceptance GAr near detector acceptance
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– Reasonable momentum resolution → magnet for curvature – Particle ID – Cross-sectional area matched to LAr
– 1000 kg fiducial mass of argon → high pressure – Measure photons, neutrons → ECAL – Excellent PID – Low thresholds (few-MeV for protons) → spatial resolution
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– New field cage, support structure, etc
– Will be instrumented as a muon
catcher
5m 5m
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– ALICE achieved < 1%
(8.5 atm) ECAL/muID used to ID particles where these lines crossed DUNE baseline design uses the same 90:10 Ar:CH4 mixture as PEP-4
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– High-granularity inner provides photon direction and good energy
resolution
– Maybe neutron TOF too → leads to O(ns) timing resolution requirement
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– Field uniformity – Stray field – Total space needed – Material between liquid and gas
– Solves the mu/pi problem in the ECAL
Superconducting 3-coil Helmholtz with 2 bucking coils Solenoid with partial return yoke (no front face)
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– Using one of the ALICE inner chambers – Small field cage and cathode to form drift region – Pressure vessel rated to 10 atm
– Gas gain for different gas mixtures at various
pressures
– Demonstrate successful drift and readout at 10
atmospheres!
– Test of readout electronics planned for use (as
much overlap with liquid as possible)
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Cosmic, 1atm Fast signal – electron avalanche near anode wires produces lots of positive ions Ions moving away from the pad plane Long positive pulse as ions move in the field cage
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multiple pulses close together
Fe-55, 1atm
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– Results agree with our expectations
1 atm Fe-55 source
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– Gas gain drops as expected – Next stop – 10 atmospheres!
Fe-55, 5atm Cosmic, 5atm
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chamber
– Still in the gas-tight transport box
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– Determination of neutrino mass hierarchy – Observation of CP-violation in the lepton sector (if the
– Supernova detection and measurement – Baryon number violation (nucleon decay) – BSM searches, both accelerator and non-accelerator
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(reconstructed) neutrino energy at far-detector
various oscillation parameters
– Infer best-fit parameters!
sections lead to uncertainties on
– Solution - measure the flux and
cross sections at a near detector!
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In liquid argon, this is all in one voxel
Inner and Outer readout chambers
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– For a t0 tag if entire interaction is contained – Not critical for primary DUNE physics
– Not being pursued for DUNE
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