The MINERvA Experiment: precision -A cross sections Eric Christy, Hampton University Elba, 2010 (for the MINER A Collaboration) MINERVA.

Slides:



Advertisements
Similar presentations
A status report on the MINER A neutrino Experiment Steven Manly, University of Rochester Representing the MINER A collaboration HEP 2012, Valparaiso, Chile.
Advertisements

MiniBooNE: (Anti)Neutrino Appearance and Disappeareance Results SUSY11 01 Sep, 2011 Warren Huelsnitz, LANL 1.
MINERvA Overview MINERvA is studying neutrino interactions in unprecedented detail on a variety of different nuclei Low Energy (LE) Beam Goals: – Study.
How to Build a Neutrino Oscillations Detector - Why MINOS is like it is! Alfons Weber March 2005.
Recent Electroweak Results from the Tevatron Weak Interactions and Neutrinos Workshop Delphi, Greece, 6-11 June, 2005 Dhiman Chakraborty Northern Illinois.
F.Sanchez (UAB/IFAE)ISS Meeting, Detector Parallel Meeting. Jan 2006 Low Energy Neutrino Interactions & Near Detectors F.Sánchez Universitat Autònoma de.
The MINERnA Experiment
The Design of MINER  A Howard Budd University of Rochester August, 2004.
2/21/2008 P5 neutrino session1 Conventional neutrino experiments Heidi Schellman P5 February 21, 2008.
NUFACT06, Irvine, CA August 25, 2006 S. Manly, University of Rochester1 Recent Electron Scattering Results from Jefferson Laboratory S. Manly University.
Bari Osmanov University of Florida MINERvA: neutrino cross-sections for the future EPS HEP July, Krakow, Poland Bari Osmanov, University of.
10/24/2005Zelimir Djurcic-PANIC05-Santa Fe Zelimir Djurcic Physics Department Columbia University Backgrounds in Backgrounds in neutrino appearance signal.
Fancy Rutgers Logo that eats CPU to print was here DNP Oct The MINER A Experiment Ronald Ransome Rutgers, The State University of New Jersey Piscataway,
Physics Topics in MINER A David Boehnlein - Fermilab for the MINERvA Collaboration Overview of MINERvA The high intensity of the NuMI beamline at Fermilab.
July 19, 2003 HEP03, Aachen P. Shanahan MINOS Collaboration 1 STATUS of the MINOS Experiment Argonne Athens Brookhaven Caltech Cambridge Campinas Dubna.
MINERvA Overview MINERvA is studying neutrino interactions in unprecedented detail on a variety of different nuclei Low Energy (LE) Beam Goals: – Study.
1 Overview of the MINER A Experiment Vittorio Paolone(representing the MINER A Collaboration) University of Pittsburgh  Motivation  MINER A Detector.
Measurements of F 2 and R=σ L /σ T on Deuteron and Nuclei in the Nucleon Resonance Region Ya Li January 31, 2009 Jlab E02-109/E (Jan05)
5/1/20110 SciBooNE and MiniBooNE Kendall Mahn TRIUMF For the SciBooNE and MiniBooNE collaborations A search for   disappearance with:
W properties AT CDF J. E. Garcia INFN Pisa. Outline Corfu Summer Institute Corfu Summer Institute September 10 th 2 1.CDF detector 2.W cross section measurements.
The Muon Neutrino Quasi-Elastic Cross Section Measurement on Plastic Scintillator Tammy Walton December 4, 2013 Hampton University Physics Group Meeting.
R. Ransome - PANIC July 26, Charged Current Neutrino Scattering in MINER A Ronald Ransome Rutgers, The State University of New Jersey On behalf.
The fully active scintillator target is surrounded by nuclear targets and calorimeters. Interactions in the scintillator (CH n ) can be compared with interactions.
July 6, INPC 1 The MINER A Experiment R. Ransome Rutgers, The State University of New Jersey for the MINER A collaboration ν Full MINERνA Detector.
Pion Production in MINERνA Brandon Eberly University of Pittsburgh July 27, 2012 On behalf of the MINERνA collaboration MINER ν A 1.
Status of the NO ν A Near Detector Prototype Timothy Kutnink Iowa State University For the NOvA Collaboration.
The Design and Performance of the MINER A Detector Howard Budd, University of Rochester Technology and Instrumentation in Particle Physics 2011.
MINER A (FNAL E938) Gabriel Niculescu, JMU MINERA web site: Miner a Main Injector MINOS Near Detector NuMI Beam Where?  FERMILAB.
FNAL User’s Meeting June The MINER A Experiment Ronald Ransome Rutgers, The State University of New Jersey Piscataway, NJ For the MINER A Collaboration.
Teppei Katori Indiana University Rencontres de Moriond EW 2008 La Thuile, Italia, Mar., 05, 08 Neutrino cross section measurements for long-baseline neutrino.
Measurement of F 2 and R=σ L /σ T in Nuclei at Low Q 2 Phase I Ya Li Hampton University January 18, 2008.
Preliminary Results from the MINER A Experiment Deborah Harris Fermilab on behalf of the MINERvA Collaboration.
Latest Results from the MINOS Experiment Justin Evans, University College London for the MINOS Collaboration NOW th September 2008.
MiniBooNE Cross Section Results H. Ray, University of Florida ICHEP Interactions of the future!
MINERvA Main INjector ExpeRiment for -A is the symbol for the neutrino. The beam that is sent to MINERvA is made out of neutrinos. In chemistry, an A stands.
Detector Monte-Carlo ● Goal: Develop software tools to: – Model detector performance – Study background issues – Calculate event rates – Determine feasibility.
1 Mike Kordosky – NuFact 06 - Aug 27, 2006 Neutrino Interactions in the MINOS Near Detector Mike Kordosky University College London on behalf of the MINOS.
Measurements of neutrino charged current scattering in K2K Fine-Grained Detector Introduction Introduction K2K Near Detector K2K Near Detector CC interactions.
1 Physics Requirements on Reconstruction and Simulation Software Jorge G. Morfín - Fermilab.
Physics - Detector Optimization Studies NuInt05 Highlights Jorge G. Morfín Fermilab.
CP violation in B decays: prospects for LHCb Werner Ruckstuhl, NIKHEF, 3 July 1998.
MINER A Main INjector ExpeRiment for v-A Active segmented scintillator detector: 5.87 tons Nuclear targets of C, Fe and Pb, Water, Helium.
D. Harris Fermilab NuFact09 Neutrino Interactions: results by Neutrino 2012 and beyond Deborah Harris Fermilab Neutrino 2010 Athens June 18, 2010 Special.
MiniBooNE MiniBooNE Motivation LSND Signal Interpreting the LSND Signal MiniBooNE Overview Experimental Setup Neutrino Events in the Detector The Oscillation.
MINER A Main INjector ExpeRiment for v-A Active segmented scintillator detector: 5.87 tons Nuclear targets of C, Fe and Pb.
THE MINERVA EXPERIMENT Heidi Schellman DIS DIS2010.
April 26, McGrew 1 Goals of the Near Detector Complex at T2K Clark McGrew Stony Brook University Road Map The Requirements The Technique.
Susan Burke DØ/University of Arizona DPF 2006 Measurement of the top pair production cross section at DØ using dilepton and lepton + track events Susan.
The MINER A Experiment Sacha Kopp, University of Texas at Austin on behalf of the Minerva Collaboration.
Heavy stable-particle production in NC DIS with the ZEUS detector Takahiro Matsumoto, KEK For the ZEUS collaboration.
NUMI NUMI/MINOS Status J. Musser for the MINOS Collatoration 2002 FNAL Users Meeting.
Results and Implications from MiniBooNE: Neutrino Oscillations and Cross Sections 15 th Lomonosov Conference, 19 Aug 2011 Warren Huelsnitz, LANL
MINER A at the Triple Point: Three Phases at once Deborah Harris AEM August 31, 2009.
 CC QE results from the NOvA prototype detector Jarek Nowak and Minerba Betancourt.
Nuclear Target Cross Section Ratios at MINERvA Brian G. Tice - Argonne National Laboratory With travel support from Rutgers, The State University of New.
INPC 2013 June 4 th ‘13 Alessandro Bravar for the Miner a Collaboration The MINER A Experiment What is Miner a ? beam and  flux Why Miner a ? / CCQE x-sections.
STATUS OF MINERvA Heidi Schellman DPF DPF09.
MINERνA Overview  MINERνA is studying neutrino interactions in unprecedented detail on a variety of different nuclei  Low Energy (LE) Beam Goals: t Study.
MINERνA Overview  MINERνA is studying neutrino interactions in unprecedented detail on a variety of different nuclei  Low Energy (LE) Beam Goals: t Study.
Measuring Nuclear Effects with MINERnA APS April Meeting 2011 G. Arturo Fiorentini Centro Brasileiro de Pesquisas Físicas On behalf of the MINERnA collaboration.
Mike Kordosky, 3 rd Project X Workshop June 5-6, 2008 MINERvA Mike Kordosky William and Mary High Precision Neutrino Scattering at the Main Injector.
5/31/2006Fermilab Users Meeting1 Zelimir Djurcic Physics Department Columbia University MiniBooNE, NO A, MINER A.
The MiniBooNE Little Muon Counter Detector
J. Musser for the MINOS Collatoration 2002 FNAL Users Meeting
Chris Smith California Institute of Technology EPS Conference 2003
F.Sánchez for the K2K collaboration UAB/IFAE
Neutrino interaction measurements in K2K SciBar
Duality in Pion Electroproduction (E00-108) …
Impact of neutrino interaction uncertainties in T2K
Susan Burke, University of Arizona
Presentation transcript:

The MINERvA Experiment: precision -A cross sections Eric Christy, Hampton University Elba, 2010 (for the MINER A Collaboration) MINERVA

Elba 2010June 22, MINER A Main Injector ExpeRiment ν-A ~70 Particle, Nuclear, and Theoretical physicists from 21 Institutions  MINERvA is studying A dependence of neutrino interactions in unprecedented detail, from He to Pb  Uses high intensity NuMI Beamline at Fermilab and MINOS near detector as muon spectrometer  Nuclear physics goals  High precision measurement of the axial form factor to high Q 2 and search for A dependence of form factor.  Studies of quark-hadron duality in neutrino interactions, complementing JLab.  Search for x-dependent nuclear effects in neutrino interactions. (For instance DIS structure functions)  Precision cross section measurements and studies of final states LHe

Elba 2010June 22, Institutions of MINER A MINOS T2K NOVA Nuclear Theory MINERVA Irvine Tufts William & Mary FNAL Duluth Texas Athens Pitt Rochester Hampton Valparaiso (Chile) James Madison Rutgers Jefferson Lab Dortmund INR, Moscow MCLA (Mass.) ‏ Otterbein UNI (Peru) ‏ PUCP (Peru) ‏ CBPF (Brazil) ‏ Guanajuato (Mex) ‏ Northwestern Florida MiniBooNE

Elba 2010June 22, A scattering is complementary to e-A form factorsstructure functions  Can study nucleon form factors and structure functions and their medium modifications  Same structure as determined by QCD, but with a different probe than the photon.  Different sensitivity to parton flavor, strange and weak axial FFs, and medium effects.  Charged current scatting is flavor sensitive.  Combination of and anti- scattering allows for separation of form factors and valence/sea quark distributions.

Elba 2010June 22, Nuclear Modifications in -A neutrino+iron anti-neutrino+iron l- l- d u W+W+ W-W- l+ l+ d u CTEQ nuclear PDF fit, Schienbein et al., PRD77(2008)  Essentially NO data on A dependence of structure functions in -A.  Reasons to believe that these might be different that e-A (eg. Different shadowing due to presence of axial vector current – S. Kulagin).  MINER A will map out the nuclear dependence.

Elba 2010June 22, Neutrino – Nucleon Scattering Total cross section/E Quasi-elastic Resonance production  Current World data has large uncertainties  MINER A plans to significantly improve this  Wide range of nuclear targets Exchange W or Z couples to weak charge.

Elba 2010June 22, Some Experimental differences between e-A and -A experiments (from an electron scattering perspective). 1. Low Rates => Need very large mass target => large detectors Also means,  don't need a fast trigger...  In fact MINERvA doesn't have one! 2. Can not directly monitor beam (indirect monitoring is possible) 3. Typically wide band beam (in energy) => often don't know the neutrino energy event by event without complete calorimetry of final states.

Elba 2010June 22, Downstream Calorimeters: 20 modules,, sheets of lead (Electromagnetic Calorimetry) or steel (Hadronic calorimetry) between scintillator planes Side Calorimeters: 2 thin lead “rings” for side electromagnetic Calorimetry, 4 layers of instrumented steel frames. Experiment Configuration MINOS Near Detector (momentum reconstruction for escaping muons) VetoWall LHe

Elba 2010June 22, Nuclear Targets Target: water VetoWall LHe Target Material Estimated Charged Current Statistics Helium 0.6 M Scintillator 9 M Carbon 1.4 M Iron 2.9 M Lead 2.9 M Water 0.7 M

Elba 2010June 22, NuMI Beam MINERvA MINOS ND MINOS ND Hall

Elba 2010June 22, Components of the MINERvA Detector

Elba 2010June 22, MINERvA Detector Module Outer Detector (OD) Layers of iron/scintillator for hadron calorimetry: 6 Towers Inner Detector Hexagon – X, U, V planes for stereo view 1 tower2 tower 6 tower 5 tower4 tower 3 tower  ~32k channels 80% in inner hexagon 20% in Outer detector  ~500 M-64 PMTs (64 channels)  1 wave length shifting fiber per scintillator, which transitions to a clear fiber and then to the PMT  127 pieces of scintillator per Inner Detector plane  8 pieces of scintillator per Outer Detector tower, 6 OD detector towers per module. Lead Sheets for EM calorimetry

Scintillator strips glued into 'planks' (Covered in polycarbonate 'Skin') WLS fibers glued Into strips and Routed to optical Connector location 5 Planks assembled into plane, glued and covered with 'outer skin' optical Connector Connector glued and then flycut Fiber 'Baggie' sealed and plane light tightened Inner Detector Fabrication (W&M, Hampton U., Fermilab)

Elba 2010June 22, Module Assembly Module Assembly (Wideband) OD Frame Fabrication FNAL (Wideband) Assembled Module On Strongback Optical Cable Prepping Wideband Gluing side Ecal Pb Installing components Into frames. Optical Connectors

Elba 2010June 22, Fully Assembled MINER A (Sans Cryotarget and Veto Wall) MINOS ND PMT Racks Readout Electronics

Elba 2010June 22, From scintillation to hit position and energy (Inner detector scintillator and optics shown, Outer Detector has similar optics but rectangular scintillator) 1.7 × 3.3 cm 2 strips Wave Length Shifting (WLS) fiber readout in center hole Exploit charge sharing to provide 2-3 mm position resolution within plane. Optical Connectors Scintillator (pink) & embedded Wave Length Shifting (WLS) Fiber Clear fiber M-64 PMT PMT Box Particle Scintillator

Elba 2010June 22, Stages of MINER A Frozen Detector (55% of full detector) : November 2009 – March 2010 Nov – March 2010: Low E anti-ν (~4 GeV average) March 2010 – March 2012: Low E (~ 4 GeV average) Spring 2013 – 2016: Medium E  (~8 GeV average) Full Detector:

Elba 2010June 22, Tracking region ECAL HCAL Over 99.9% of channels live! MINERνA detector occupancy plot during beam on Initial Detector Performance (1) 18 ADC counts

Elba 2010June 22, Detector availability and Livetime Initial Detector Performance (2) LT > 97% Per plane resolution From track residuals ~3 mm

Elba 2010June 22, What do real MINERvA event topologies look like?  +n→  - +p e +n→ e - +p  +n→  - +   +X p     p e real events Sample of real events below from tracking prototype in neutrino mode. (Candidate process noted below each display)

Elba 2010June 22, MINERvA Run Plan Summary Low Energy Anti-neutrino beam: November 2009– March Low Energy Neutrino Beam: March 2010 – March 2012, plan for 4x10 20 protons on target. Analyze data during long Fermilab accelerator shutdown in Medium Energy Neutrino beam with NOvA after 2012 shutdown: plan for 3 year run, plan for 12x10 20 protons on target.

Elba 2010June 22, Kinematic Reconstruction Tools Scattering / production angles: Momentum/energy: Tracking/vertexing utilizing MINERvA segmented scintillator planes  High energy leptons tracks exiting minerva use momentum reconstructed from MINOS.  Contained single tracks use fit of dE/dx profile (specifically protons and pions which range out before the HCAL).  Larger energy hadrons use total energy from HCAL corrected for non-visible energy.  e/  /  0 use ECAL corrected for non-visible energy.

Elba 2010June 22, Momentum from dE/dx Calculated dE/dx for Protons with P (GeV/c): all We wish to use all the information on energy deposition available to us and not just range or average dE/dx. => Fit the entire (visible) energy deposition profile in z to that expected for various momenta and particle mass. Calculated profiles based on 1. vertex, 2. angle of track 3. material dbase Best fit profile from  2 Visible energy in scintillator planes

Elba 2010June 22, Candidate  /  track Method allows good determination of the momentumAND Most probable mass Monte Carlo indicates effective PID method

Elba 2010June 22, Candidate proton track

Elba 2010June 22, Expected physics capability of MINER A

Elba 2010June 22, MINER A Event Rates 14.5 Million total CC events in the current run-plan 7 Million NC events Run-plan assumes 4.0x10 20 in LE  and 12.0x10 20 ME NuMI beam configurations Main CC Physics Topics (Statistics in CH)  Quasi-elastic 0.8 M events  Resonance Production 1.7 M total  Transition: Resonance to DIS2.1 M events  DIS, Structure Funcs. and high-x PDFs 4.3 M DIS events  Coherent Pion Production89 K CC / 44 K NC  Strange and Charm Particle Production > 240 K fully reconstructed events  Generalized Parton Distributions order 10 K events  Nuclear Effects He: 0.6 M, C: 0.4 M, Fe: 2.0 M and Pb: 2.5 M

Elba 2010June 22, Expected MINER A Quasi-Elastic s Statistical Error Only: includes purity and efficiency

Elba 2010June 22, MINER A Measurement of Nuclear Effects The Axial-vector Current and Shadowing in DIS Sergey Kulagin Estimate of MINER A Error Bars Current run plan MINER A data Could allow first Observation of differences due to probe.

30 Coherent Pion Production MINER A Region where NEUGEN overestimates the cross sections Rein-Seghal Paschos- Kartavtsev MINER A’s nuclear targets allow the first measurement of the A-dependence of  coh across a wide range of nuclei.

Elba 2010June 22, Summary  MINERvA will measure -A cross sections to unprecedented precision  This will allow studies complementary to e-A scattering such as: DIS structure functions, Elastic form factors, resonance production, duality studies, and more.  Data taking in progress.... Stayed tuned!

Elba 2010June 22, Backup Slides

Elba 2010June 22, Empty Taret Background 33 l - d u W+W+ W-W- l + d u neutrino beam: Al/H=6.7 anti-neutrino beam: Al/H=3.5

Elba 2010June 22,  Data show no simple scaling with average nuclear density for light nuclei  9 Be and 3 He have similar average densities but very different EMC ratios. New Jlab results on EMC effect in light Nuclei => Correcting from nucleus to nucleon using nuclear density questionable

Elba 2010June 22, Neutral Current Quasi-elastic Current World data set from BNL E734 but... 80% of events were from bound protons in Carbon. Requires neutron target (Deuterium)‏ Systematic uncertainty is dominated by flux The follow ratios can be used to isolate form factors with reduced systematics.

Elba 2010June 22, Combined analysis of E734 + Jlab HAPPEX & G0 PV data S. Pate, arXiv: hep-ex  p elastic sensitive to strangeness  Combining e-p parity violating elastic measurements with  p elastic measurements allows extraction of strange axial form factors.  Uncertainties are dominated by E734 systematics.

Elba 2010June 22, Overview of MINERvA MINERvA and Cross Section Measurements (examples) Quasi-elastic Cross Section –First precise measurements at high Q 2 of proton axial form factor –First study in nuclear modification of form factors conjectured at low Q 2 Coherent  production Cross Section –Overwhelming statistics (> 100 increase) –Wide energy range –Range of nuclear targets (C, Fe, Pb, H 2 O, He) –MINERvA is in a position to measure this important background for ν e appearance and to check recent surprising K2K null result 4-year MINERVA run MiniBooNe & K2K MiniBooNE & K2K measurements Quasi-Elastic Cross Section