The MINER A Experiment Sacha Kopp, University of Texas at Austin on behalf of the Minerva Collaboration.

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Presentation transcript:

The MINER A Experiment Sacha Kopp, University of Texas at Austin on behalf of the Minerva Collaboration

NuFact2010, Mumbai, India 2 Outline Previous  Results NuMI Beam & measuring the flux MINER A Detector MINER A Event Displays Kinematic Distributions Summary

NuFact2010, Mumbai, India interaction physics Past measurements –bubble chambers –wide band neutrino beams at low energy –NBB for >20 GeV Limitations on measurement accuracies –low statistics samples –significant uncertainty on flux in wide band neutrino beams In many cases the nuclear physics effects not well- understood 3 note: plot does not include MiniBooNE or SciBooNE data

NuFact2010, Mumbai, India interaction physics Renewed interest for En reconstruction in oscillation experiments –calorimetric exp’ts –Water Cherenkov QEL 4 note: plot does not include MiniBooNE or SciBooNE data

NuFact2010, Mumbai, India 5 New Data, Still Inconsistent New Data Clear inconsistency between MiniBooNE/SciBooNE and NOMAD results

NuFact2010, Mumbai, India 6 MINER A Precision measurement of cross sections in the 1-10 Gev region –Understand the various components of cross section both CC and NC CC & NC quasi-elastic Resonance production,  Resonance↔deep inelastic scatter, (quark-hadron duality) Deep Inelastic Scattering Study A dependence of interactions in a wide range of nuclei

NuFact2010, Mumbai, India Main Injector Accelerator Plan View Extraction magnets target Evacuated Decay Volume focusing horns Access Tunnel Hadron Absorber Muon Alcoves Minerva Detector Hall Target Hall beam p p,K,     NuMI Beamline Fast-extracted 120 GeV p beam → C target (3-4)x10 20 protons/year → π ± /K ± 2 horns focus π + /K + → μ + ν μ or π - /K - → μ - ν μ Absorber stops hadrons not   absorbed by rock,  → detector Extensive instrumentation to monitor p, hadron, muon beams

NuFact2010, Mumbai, India 8 NuMI Variable Energy Beam NuMI target mounted on a rail drive for remote positioning Provides in situ method to measure flux Vary (p z,p T ) of   contributing to flux. –Horn current (p T kick supplied to  ’s) –Target Position (p z of focused particles) Target Moved 2.5m back from horns Target Moved 1m back from horns pTpT pZpZ Normal Running p ++ ++ p

NuFact2010, Mumbai, India 9 In Situ Flux Measurement Past experiments in wide band beams limited to ~30% uncertainty in flux External hadron production data sometimes inconsistent, or leaves no opportunity for in situ check of the flux. Variable beam configurations offer in situ flux method Can check cross sections at single E using several beam configurations Measure event spectrum with QEL’s Normalize to NBB (CCFR) at high energy Goal is 7% error flux shape, 10% norm cross-check cross sections with several spectra

NuFact2010, Mumbai, India 10 Absolute Flux with  Monitors Alcove 2 E  >11GeV  >6GeV Alcove 3 E  >21GeV  >11GeV  Sampling  flux = Sampling hadrons off target = Sampling  flux.  Sample different energy regions of the flux.  Several beam settings → differential flux  Goal of  monitors is to understand flux shape and normalization to 10%  ’s  ’s ’s Alcove 1 Alcove 3 Alcove 2 Alcove 1 E  >4GeV  >2GeV

NuFact2010, Mumbai, India 11 b Muon Monitor Signal (arb) b b Horn Current (kA) b Early Data from  Monitors Target 100cm upstream of hornTarget 250cm upstream of horn

NuFact2010, Mumbai, India VetoWall LHe ¼ ton 12 MINER A Detector Made of 120 planar “modules”. –Total Mass: 200 tons –Total channels: ~32K Nuclear Targets with Pb, Fe, C, H 2 O,CH In same experiment reduces systematic errors between nuclei Fully Active Fine Segmented Scintillator Target 8.3 tons, 3 tons fiducial Side HCAL Side ECAL

NuFact2010, Mumbai, India 13 MINER A  Spectrometer The MINOS Near Detector is MINER A  Spectrometer Minos (previously installed)

NuFact2010, Mumbai, India 14 Tracking Scintillator Planes Strips WLS fiber glued into scintillator Fibers mirrored on far end. Near end terminated in optical connector, polished, and light- tightened. Position determined by charge sharing Particle 3 different strip orientations

NuFact2010, Mumbai, India 15 Broad Range of Nuclear Targets 5 nuclear targets + water target Helium target upstream of detector Near million-event samples (4  POT LE beam + 12  POT ME beam 15 TargetMass in tonsCC Events (Million) Scintillator39 He C (graphite) Fe Pb Water Nuclear Targets: Fe Pb C

NuFact2010, Mumbai, India Current run plan 4 × POT LE beam (10 20 POT accum. so far) 12 × POT ME beam 0.9 × POT special runs Yield: ~14M CC events 9M in scintillator NuMI Low Energy Beam (neutrinos) Quasi-elastic Resonance production Resonance to DIS transition region DIS Low Q 2 region and structure functions Coherent Pion Production charm / strange production 0.8 M 1.7 M 2.1 M 4.3 M CC 89k, NC 44k 230 k Charged Current Sample

NuFact2010, Mumbai, India MINERvA Run Plan: History and Summary Low Energy Anti-neutrino beam: 11/2009 – 3/2010 –55% of detector commissioned by 11/09 –Installation of remaining 45% –Accumulated ~0.8x10 20 protons on target Low Energy Neutrino Beam: 3/2010 – 3/2012 –4x10 20 protons on target in “standard”  beam –0.9x10 20 in special runs to understand flux Fermilab accelerator shutdown, switch to Medium Energy Beam configuration: 3/2012—2/2013 Medium Energy Neutrino beam with NOvA after 2/2013 –12x10 20 protons on target in neutrino mode –Would be interested in antineutrinos too, of course 17

NuFact2010, Mumbai, India 18 MINER A Events in Beam CCQE anti-event –Information buffered in the spill and read out at end of spill – Timing for different slices ( events) –4 th slice –3 view, x (top), & V –Outer calorimeter X view of other events Event with  0

NuFact2010, Mumbai, India MINER A Events in Beam 19 From to

NuFact2010, Mumbai, India Candidate Nuclear Target Events Upstream region of detector has 5 different planes of nuclear targets and gap for water target, separated by 4 modules 20

NuFact2010, Mumbai, India 21  eam Data 4.04 × POT in anti- mode MC generator GENIE v –GEANT4 detector simulation –2 × POT MC, LE Beam MC anti-  flux, untuned –Area normalized Require reconstructed muon in MINOS

NuFact2010, Mumbai, India 22  Data in  Beam  Distributions same conditions as before Very good agreement between Data and MC

NuFact2010, Mumbai, India 23 Summary The high statistics MINER A is on the air ! –Have ~25% of the needed Low Energy beam so far Using various techniques to understand the flux –Have first glance at 2 of 6 special neutrino beam runs Precision Measurement of various cross section and support current and future  experiments –QE, Resonance, DIS, Detector working very well Analysis of data is proceeding Expect preliminary results in the near future. My gratitude to colleagues H.Budd, E.Christy, G.Perdue, R.Ransome, from whose slides I’ve drawn.

NuFact2010, Mumbai, India 24 Nuclear Effects, FGM & FSI Rescattering/Absorb in nuclear media – Resonance →QE,  is lost –Kinematics of event are modified Paschos et al, hep-ph/ Before Interactions After Interactions Resonance production in Oxygen Fermi gas model, nucleons obey Pauli exclusion principle –Nucleons fill up states to some Fermi momentum –Maximum momentum k F ~ 235 MeV/c Nuclear binding, additional binding energy which in simple models is treated as a constant. Pauli blocking for nucleons not escaping nucleus, as states are already filled with identical nucleons