Transcript Document
MINERnA
NuMI
George Tzanakos
University of Athens
Outline
Introduction
Physics Goals
The NuMI Beam
Detector Technology
The MINERvA Detector
Expected Results
Connection to Neutrino Oscillation Expts
Current Status and Outlook
Conclusions
George Tzanakos, University of Athens, Greece
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Main INjector ExpeRiment for v -A
• MINERvA is a newly approved FNAL Experiment
designed to study neutrino-nucleus interactions with
unprecedented detail.
• MINERvA uses a compact, fully active neutrino
detector to make accurate measurements of v – A cross
sections in exclussive channels.
• The MINERvA detector will be placed in the NuMI
beam line upstream of the MINOS Near Detector.
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NuMI Beam
MINOS ND
MINERvA
Main Injector
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MINOS ND
MINERvA
(Animation)
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D. Drakoulakos, P. Stamoulis, G. Tzanakos, M. Zois
University of Athens, Athens, Greece
G. Blazey, M.A.C. Cummings, V. Rykalin
Northern Illinois University, DeKalb, Illinois
D. Casper, J. Dunmore, C. Regis, B. Ziemer
University of California, Irvine, California
W.K. Brooks, A. Bruell, R. Ent, D. Gaskell,,
W. Melnitchouk, S. Wood
Jefferson Lab, Newport News, Virginia
E. Paschos
University of Dortmund, Dortmund, Germany
D. Boehnlein, D. A. Harris, M. Kostin, J.G. Morfin,
A. Pla-Dalmau, P. Rubinov, P. Shanahan, P. Spentzouris
Fermi National Accelerator Laboratory, Batavia, Illinois
M.E. Christy, W. Hinton, C.E .Keppel
Hampton University, Hampton, Virginia
R. Burnstein, O. Kamaev, N. Solomey
Illinois Institute of Technology, Chicago, Illinois
S.Kulagin
Institute for Nuclear Research, Moscow, Russia
I. Niculescu. G. .Niculescu
James Madison University, Harrisonburg, Virginia
Red = HEP, Blue = NP, Black = Theorist
George Tzanakos, University of Athens, Greece
S. Boyd, D. Naples, V. Paolone
University of Pittsburgh, Pittsburgh, Pennsylvania
A. Bodek, R. Bradford, H. Budd, J. Chvojka,
P. de Babaro, S. Manly, K. McFarland, J. Park, W. Sakumoto
University of Rochester, Rochester, New York
R. Gilman, C. Glasshausser, X. Jiang, G. Kumbartzki,
K. McCormick, R. Ransome
Rutgers University, New Brunswick, New Jersey
A. Chakravorty
Saint Xavier University, Chicago, Illinois
H. Gallagher, T. Kafka, W.A. Mann, W. Oliver
Tufts University, Medford, Massachusetts
J. Nelson, F.X.Yumiceva
William and Mary College, Williamsburg, Virginia
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For mass splitting (m2) measurements in νμ disappearance
•
Understanding of relationship between observed energy & incident
neutrino energy (Evis En) ultimate precision in m2
– Measurement of n-initiated nuclear effects
– Improved measurement of exclusive cross sections
For electron appearance (νμ νe)
•
Much improved measurements of n- A exclusive accurate background
predictions signal above background estimation
– Individual final states cross sections (esp. π0 production)
– Intra-nuclear charge exchange
– Nuclear (A) dependence
For Nuclear Physics
•
New precise Jefferson Lab measurements of electron scattering are
inspiring nuclear physicists to consider neutrinos
–
–
Vector versus axial vector form factors
Nuclear effects: are they the same or different for neutrinos?
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• Axial form factor of the nucleon
– Yet to be accurately measured over a wide Q2 range.
• Resonance production in both NC & CC neutrino interactions
– Statistically significant measurements with 1-5 GeV neutrinos *
– Study of “duality” with neutrinos
• Coherent pion production
– Statistically significant measurements of or A-dependence
• Nuclear effects
– Expect some significant differences for n-A vs e/μ-A nuclear effects
• Strange Particle Production
– Important backgrounds for proton decay
• Parton distribution functions
– Measurement of high-x behavior of quarks
• Generalized parton distributions
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Mainly from experiments in the 70’s and 80’s at ANL,
BNL, FNAL, CERN, Serpukov
• World sample statistics is poor!
• Systematics large due to flux uncertainties
• See examples:
•
•
•
•
Quasi elastic scattering
Single pion production (CC)
Total Cross Section
Coherent pion production
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S. Zeller - NuInt04
K2K and MiniBooNe
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nμp–p+
nμn–n+
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nμn–p0
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(tot/En) vs En
NuMI flux (1-20 GeV)
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En
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• Need an Intense Neutrino Beam (NuMI Beam)
•
Improved Systematics in Neutrino Flux (NuMI
Target in MIPP Experiment)
• We need a detector with
– Good tracking resolution
– Good momentum resolution
– A low momentum threshold
– Timing (for strange particle ID)
– Particle ID to identify exclusive final states
– Variety of targets to study nuclear dependencies
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Protons
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• 120 GeV primary Main
Injector beam
• 675 meter decay pipe
for p decay
• Target readily movable
in beam direction
• 2-horn beam adjusts for
variable energy range
Move Target only
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Move Target
and Horn #2
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•
•
•
•
Extremely intense beam: means near detectors see huge event rates.
Example: NuMI low energy beam, get ~million events per ton-year in near hall
MIPP measurements of NuMI target mean that n flux will be better predicted than ever before
Perfect opportunity for precision n interaction studies.
Examples of Real MINOS ND Events in
two spills:
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Assume:
• 16×1020 POT in 4 years (mixture of LE, ME, & HE tunes)
• Fiducial Volumes 3 ton (CH), 0.6 ton C, 1 ton Fe & 1 ton Pb
• 16 M total CC events (8.8 M in CH, 7.2 M in C,Fe, Pb)
Expected event yields:
– Quasi-elastic
0.8 M events
– Resonance Production
1.6 M
– Transition: Resonance to DIS
2.0 M
– DIS and Structure Functions
4.1 M
– Coherent Pion Production
85 K (CC) & 37 K (NC)
– Strange & Charm Particle Production
>230 K fully reco’d
– Generalized Parton Distributions
~10 K
– Nuclear Effects
C: 1.4M; Fe: 2.9M; Pb: 2.9M
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• 1.7 x 3.3 cm triangular Sci strips
• 1.2 mm WLS Fiber readout
Form Planes
PMT Box
Clear fiber
Scintillator and
embedded WLS
DDK
Connectors
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Cookie
M-64 PMT
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PMT Box Assembly
Fiber Bundle
Fiber Cookie
M64 MAPMT
• 64 pixels, 8 X 8 array
• pixel: 2 x 2 mm2
• QE (520 nm): >12.5%
• Cross-talk: ~ 10%
• Anode Pulse Rise
Time: ~0.83 nsec
• TTS: 0.3 nsec
• Uniformity: 1:3
Hamamatsu
M64 MAPMT
George Tzanakos, University of Athens, Greece
64 signals
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n
n
•
•
•
Active Target: Segmented scintillator
detector 5.87 tons
1 ton of US nuclear target (C, Fe, Pb)
planes (absorber + Scintillator)
Side ECAL: Pb X0/3 sampling
George Tzanakos, University of Athens, Greece
•
Downstream (DS) Calorimeters:
–
–
•
ECAL: Pb X0/3 between each sampling plane
HCAL: 1 inch steel (l0/6) between each
sampling plane.
Outer Detector (OD): (HCAL) frames
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Side view
Steel Frame
Mounting ears
3.80 m
Lead Collar
Scintillator planes or
calorimeter targets
Scintillator for
calorimeters
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OD
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ECAL
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• Quasi-elastic nn–p
p
n
–
• Proton and muon tracks are clearly resolved
• Observed energy deposit is shown as size of hit; can clearly
see larger proton dE/dx
• Precise determination of vertex and measurement of Q2
from tracking
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0 Production
g
nuclear targets
active detector
ECAL
HCAL
n
g
• two photons clearly resolved (tracked).
• can find vertex.
• some photons shower in ID, some inside ECAL (Pb absorber) region
• photon energy resolution is ~6%/sqrt(E) (average)
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• QE Scattering Cross Sections
• Axial Form Factors
• Nuclear Effects
• Coherent Pion Production
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MINERnA
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• Vector form factors measured with electrons.
• GE/GM ratio varies with Q2 - a surprise from JLab
• Axial form factor poorly known
FA from previous
D2 experiments
Minerna (4 year run}
Efficiencies and
Purity included.
Dipole Form:
GD q 2
GD q 2
George Tzanakos, University of Athens, Greece
Gp G
1
1
q2
1 2
MV
2
, M V2 0.
p 2
2
p
2n
G
G
q
,
G
0,
G
,
M
0.71
GeV
E
D
E
M
V
2
q2
1 2
Sept 23, 2005
V
MERICE05,
q 2 , G n 0, G p G
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q2 , Gn G
Deviation from Dipole behavior. Plot FA/Dipole form vs Q2
FA from the D2
experiments.
Cross Section/Dipole
Polarization/Dipole
MINERvA can determine:
• Whether FA deviates from a dipole
• Which Q2 form is correct: “cross-section” or “polarization”
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• Tests understanding of the weak
interaction
–The cross section can be calculated
in various models
• Neutral pion production is a significant
background for neutrino oscillations
– Asymmetric π0 showers can be
confused with an electron shower
Precision measurement of (E) for NC
and CC channels
Measurement of A-dependence
Comparison with theoretical models
George Tzanakos, University of Athens, Greece
n/±
n
0 /
±
Z/W
P
N
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N
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4-year MINERVA run
Expected MiniBooNe
& K2K measurements
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Plotted: σcoh vs. A
A-range of current
measurements
Rein-Seghal model
MINERvA errors
Paschos- Kartavtsev model
A
MINERvA’s nuclear targets allow
the first measurement of the
A-dependence of σcoh
across a wide A range
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Nuclear Effects & Δm2 Measurements
μ
n
π
Evis ≠ En
– Understand the relationship
Evis En
– π absorption & rescattering
– Final state rest masses
– v-nuclear corrections
predicted to be different from
those in charged lepton
scattering (studied from
Deuterium to Pb at high energies)
George Tzanakos, University of Athens, Greece
Sergey Kulagin model
F2, Pb/C (MINERnA stat. errors)
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Plotted: Evis/En versus En
-3
Fe: Effect of pion absorption
Nominal abs
+3
C
• Nuclear targets: C, Fe, Pb
•No Pion Absorption
•Effect of pion rescattering
Fe
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Pb
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(δΔ/Δ) versus Δ
(Δ Δm2)
Before MINERvA (AM)
Post MINERvA (PM)
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• NOvA’s near detector will see
different mix of events than the
far detector
Total fractional error in the predictions as a
function of reach (NOvA)
Before
Process
QE
RES
COH
DIS
d/ NOW (CC,NC) (%)
20
40
100
20
d/ after MINERnA (CC,NC) (%)
5/na
5/10
5/20
5/10
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After
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T2K’s ND will see different mix of events than the FD
•
•
To make an accurate prediction one needs
– 1 - 4 GeV neutrino cross sections (with energy dependence )
MINERvA can provide these with low energy NuMI configuration
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• April 2004 – Stage I approval from FNAL PAC
• October 2004 – Complete first Vertical Slice Test with MINERνA
extrusions, WLS fiber and Front-End electronics
• January 2005 – First Project Director’s (‘Temple’) Review
• Summer 2005 – Second Vertical Slice Test
• December 2005 – Projected Date for MINERvA Project Baseline Review
• October 2006 – Start of Construction
• Summer 2008 – MINERvA Installation and Commissioning in NuMI Near
Hall
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•
Presently Low Energy n- Nucleus interactions are poorly measured.
MINERnA, a recently approved experiment, brings together the
expertise of the HEP and NP communities to use the NuMI beam and a
high granularity detector to break new ground on precision low-energy
n-A interaction measurements.
•
MINERvA will provide a high statistics and improved systematics study
of important exclusive channels across a wider En range than currently
available. With excellent knowledge of the beam (NuMI + MIPP),
exclusive cross sections will be measured with unprecedented
precision.
•
MINERvA will make a systematic study of nuclear effects in n-A
interactions (different than well-studied e-A channels) using C, Fe and
Pb targets.
•
MINERvA will help improve the systematic errors of current and future
neutrino oscillation experiments (MINOS, NOvA, T2K, and others).
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ERICE05, Sept 23, 2005
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The MINERvA Collaboration
Especially:
S. Boyd, H. Budd, D. Harris, K.
McFarland, J. Morfin, J. Nelson,
R. Ransome
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