the majorana project: a next- generation neutrino mass probe craig aalseth for the majorana...
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![Page 1: The Majorana Project: A Next- Generation Neutrino Mass Probe Craig Aalseth for The Majorana Collaboration NDM03, Nara, Japan June 9, 2003](https://reader035.vdocuments.site/reader035/viewer/2022081419/56649ef15503460f94c01a2e/html5/thumbnails/1.jpg)
The Majorana Project: A Next-Generation Neutrino
Mass ProbeCraig Aalseth
for
The Majorana Collaboration
NDM03, Nara, JapanJune 9, 2003
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The Majorana CollaborationBrown University, Providence, RI Rick Gaitskell
Duke University, Durham, NC Werner Tornow
Institute for Theoretical and Experimental Physics, Moscow, RussiaA. Barabash, S. Konovalov, V. Stekhanov, V. Umatov
Joint Institute for Nuclear Research, Dubna, RussiaV. Brudanin, S. Egorov, O. Kochetov, V. Sandukovsky
Lawrence Berkley National Laboratory, Berkley, CAPaul Fallon, I. Y. Lee
Lawrence Livermore National Laboratory, Livermore, CAKai Vetter
Los Alamos National Laboratory, Los Alamos, NMSteve Elliott, Andrew Hime
New Mexico State University, Carlsbad, NMJoel Webb
North Carolina State University, Raleigh, NCEric Adles, Rakesh Kumar Jain, Jeremy Kephart, Ryan Rohm, Albert Young
Osaka University, Osaka, JapanHiro Ejiri, Ryuta Hazama, Masaharu Nomachi
Pacific Northwest National Laboratory, Richland, WAHarry Miley, Co-spokespersonCraig Aalseth, Dale Anderson, Ronald Brodzinski, Shelece Easterday, Todd Hossbach, David Jordan, Richard Kouzes, William Pitts, Ray Warner
University of Chicago, Chicago, ILJuan Collar,
University of South Carolina, Columbia, SCFrank Avignone, Co-spokesperson Horacio Farach, George King, John M. Palms,
University of Washington, Seattle, WAPeter Doe, Victor Gehman, Kareem Kazkaz, Hamish Robertson, John Wilkerson
http://majorana.pnl.govhttp://majorana.pnl.gov
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Outline
Introduction and OverviewReference Concept Backgrounds and Mitigation– Pulse-Shape Discrimination– Detector Segmentation
Experiment SensitivityProgress and StatusConclusions
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Germanium Basics
“Internal Source Method” from Fiorini76Ge: Endpoint = 2039 keV– Energy above many contaminants– Except: 208Tl, 60Co, 68Ge…
FWHM = 3-4 keV around 2 MeV (~0.2%)Long experience with Ge decay– Previous efforts found 2 at T1/2 ~1021 y
– Expect 0 at T1/2 ~ 4 x 1027 y
Ready to go!– Essentially no R&D needed
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Majorana OverviewGOAL: Sensitive to effective Majorana mass as low as 0.02-0.07 eV0-decay of 76Ge potentially measured at 2039 keVBased on well known 76Ge detector technology plus:– Pulse-shape analysis– Detector segmentation– Ready to begin now
Requires:– Deep underground location– 500 kg enriched 85% 76Ge– Many crystals, each segmented– Advanced signal processing
• Pulse shape discrimination– Special low background
materials
n
n
p+ p+
e-
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e
Reference ConfigurationReference Configuration
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Majorana Reference Concept
Optimization underway of performance and risk– Several low-risk designs possible– Many segmentation schemes possible
Alternative packaging, cooling, shielding under consideration– Nature of Ge crystals allows repackaging
3-D model of reference configurationSegmentation (6x2) results in2500 individual 200g segments210 2.35 kg crystals
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Starting Background Estimate
International Germanium Experiment (IGEX) achieved between 0.1-0.3 counts/keV/kg/yDocumented experiences with cosmic secondary neutron production of isotopes
Spallation Isotope
T1/2 (d) Rate from [Bro95]
After Construction
Rate During Experiment
Total in ROI
After PSD Rejection
After Seg Rejection
68Ge 270.82 0.1562 0.03702 3.93E-03 70.15 18.59 2.57 56Co 77.27 0.0238 0.00212 6.43E-05 1.15 0.30 0.04 60Co 1925.2 0.0177 0.01294 7.15E-03 127.55 33.80 4.66 58Co 70.82 0.0024 0.000202 5.60E-06 0.10 0.03 0.00
cts/keV/kg/y cts/keV/kg/y cts/keV/kg/y Counts Counts Counts
Total 0.2 0.0523 0.0112 198.95 52.72 7.28
Calculated
Experimental
[Bro95] R. L. Brodzinski, et al, Journal of Radioanalytical and Nuclear Chemistry, Articles, Vol. 193, No. 1 (1995) 61-70.
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Single-site interaction example
Monte-Carlo 2038-keV deposition from 0-decay of 76Ge
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Multiple-site interaction example
Monte-Carlo 2038-keV deposition from multi-Compton of 2615-keV 208Tl
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Multi-Parametric Pulse-Shape Discriminator
Extracts key parameters from each preamplifier output pulse Sensitive to radial location of interactions and interaction multiplicity Self-calibrating – allows optimal discrimination for each detector Discriminator can be recalibrated for changing bias voltage or other variables Method is computationally cheap, requiring no computed libraries-of-pulses
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PSD can reject multiple-site backgrounds
(like 68Ge and 60Co)
228Ac1587.9 keV
DEP of 208Tl
1592.5 keV
212Bi1620.6 keV
Keeps 80% of the single-site DEP (double escape peak)Rejects 74% of the multi-site backgrounds (use 212Bi peak as conservative indicator)
Improves T1/2 limit by 56%
Experimental Data
Original spectrum
Scaled PSD
result
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Detector Segmentation
Sensitive to axial and azimuthal separation of depositionsreference design with six azimuthal and two axial contacts is low riskThis level of segmentation gives good background rejectionThis segmentation gives us ~2500 segments of 200 g or 40 cc
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0 efficiency = 91% internal 60Co efficiency =
14%Improves T1/2 limit by
140%
Monte-Carlo Example(single crystal)
Sensitive to z and phi separation of depositions
Segment multiplicity at 2039 keV
Next Steps:•T ½ improvement
increases to 260% - 620% when including array self-shielding, depending on position of crystal – not included in earlier background estimate
•Time-series analysis of background very promising
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Sensitivity vs. TimeSlow Production: Gradual ramp to 100 kg/y - total 500 kg 85% 76Ge Fast Production: 200 kg/y (No ramp) Present 76Ge T1/2 limit rapidly surpassed (T1/2 > 1.9 1025
y)
0
H
alf
-Lif
e
Based on early IGEX background levels with reasonable background reduction and cutting methods appliedBased on early IGEX background levels with reasonable background reduction and cutting methods applied
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Collaboration Progress:Optimizations for Full Experiment
Segmented Enriched Germanium Array (SEGA):Segmented Ge
Multi Element Germanium Assay (MEGA):16+2 natural Ge
High density
Materials qualification
Cryogenic design test
Geometry & signal routing test
Powerful screening tool
g
Full Experiment
MAJORANA:500 kg Ge detectorsAll enriched/segmentedMulti-crystal modules
1 to 5 Crystals
First enriched, segmented detector in testing!
Additional tests being planned for other segmented systems
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Progress and StatusSEGA: Segmentation Optimization
First (enriched) 6x2 SEGA operating– Current: Testing (TUNL)– Shallow UG testing at U Chicago LASR facility– Operation in WIPP
Second and third SEGA planning– Funds in hand (LANL, USC)– Alternate segmentation testing in planning (USC/PNNL)– 40-fold-segmented LLNL detector now available
Figure-Of-Merit vs. Axial & Azimuthal Segmentation
for internal 60Co background
SEGA crystal initial test cryostat
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Progress and StatusMEGA: Cryogenic testing
Materials in hand– Detectors (20 - 70% HPGe),
electronics Assembly and cryogenic testing of two-packs underway (PNNL, UW, NC State)UG facility (WIPP) in prep (LANL, NMSU)Summer installation anticipatedSensitive to ~1e4 short-lived atoms
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Recent Crystal Packaging Test(MEGA)
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Progress and StatusUltra-Low Level Screening
Screening facility – Operating in Soudan (Brown U)
• Some contamination issues… 207Bi
– Two HPGE detectors (1.05 kg, 0.7 kg)
Planned use for screening– Minor materials used in manufacturing– Improved Cu testing– Small parts qualification
• FET, cable, interconnects, etc
Dual counter shield: 1.05 and 0.7 kg detectors
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Progress and StatusLow-Background Electroformed
Copper
Can be easily formed into thin, low-mass partsRecent designs reduce MCu/MGe x5UG Electroforming can reduce cosmogenicsPre-processing can reduce U-ThRecent results suggest cleaner than thought
Electroformed cups shown have wall thickness of only 250 m!
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ConclusionsUnprecedented confluence:– Enrichment availability/Neutrino mass interest/
Underground facility development
High Density: – Modest apparatus footprint, no special lab
required
Low Risk:– Proven technology/ Modular instrument /
Relocatable
Experienced and Growing Collaboration– long track record, many technical resources
Neutrino mass sensitivity:– potential for discovery
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Thank YouNDM03, Nara