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Searching for Sterile Neutrinos with an Isotope β-decay Source: The IsoDAR Experiment
Mike Mike Shaevitz Shaevitz - Columbia University
- Columbia University
Aspen Winter Workshop--New Directions in Neutrino Physics February ¡8, ¡2013
Searching for Sterile Neutrinos with an Isotope -decay Source: The - - PowerPoint PPT Presentation
1 Searching for Sterile Neutrinos with an Isotope -decay Source: The IsoDAR Experiment Mike Shaevitz Shaevitz - Columbia University - Columbia University Mike Aspen Winter Workshop--New Directions in Neutrino Physics February 8,
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Searching for Sterile Neutrinos with an Isotope β-decay Source: The IsoDAR Experiment
Mike Mike Shaevitz Shaevitz - Columbia University
Aspen Winter Workshop--New Directions in Neutrino Physics February ¡8, ¡2013
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Where Are We With Sterile Neutrinos?
Δm2 ≈ 1 eV2
– LSND / MiniBooNE νe /νe appearance – Reactorνe disappearance (“Reactor Anomaly”) – Radioactive source νe disappearance – But still no indication of νµ disappearance
particle physics but …..
– Significance at the > 5σ level – Observation of oscillatory behavior within detector
– Multi-detector accelerator neutrino beam experiments – Very short baseline (VSBL) experiments with compact neutrino sources
Some difficulty for fits with one or two sterile neutrino models
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Hasν νe Disappearance Been Observed? ⇒ Reactor Antineutrino Anomaly
Red: 3ν sin2(2θ13) = 0.15 Blue: 4ν ∆m2
new = 2 eV2
and sin2(2θnew)=0.12, with sin2(2θ13) = 0.085 arXiv: 1204.5379 Current Reactor Experiments Older Reactor Exps at Close Distances R = 0.927 ± 0.023 (3.0 σ ) Region to Explore for Sterile Neutrinos
3 ν 4 ν
νe →νs ?
RENO Daya Bay
near detectors
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Very-short Baseline Oscillation Experiments
neutrino source has small extent .
– Look for a change in event rate as a function of position and energy within the detector – Bin observed events in L/E (corrected for the 1/L2) to search for oscillations
ν - Detector
1/ L2 flux rate modulated by Probosc = sin2 2! "sin2 #m2L / E
( )
ν - Source
Radioactive Source
Isotope Source
Reactor Source
Proton into Dump Source
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Possible Sources for VSBL Experiments
– Eν ~ 3 MeV ⇒ optimum distance around 3 to 20 m – Reactor core size can also be an issue
– Eν ~ few MeV ⇒ see oscillations with wavelengths ~ 1m – Compact source can be placed directly into detector or just outside
– Eν ~ 8 MeV (typical of short lived isotopes, i.e. 8Li) – Distance to source can be longer 10m to 20m – Compact source that can be set up near an existing large detector – Beam can be turned off periodically to measure background – Higher energy neutrinos with less background
Need experiments with L/E ~ 1 m/MeV
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IsoDAR Experiment Isotope Decay-at-Rest Neutrino Source (ν νe Disappearance )
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DAEδDALUS 800 MeV Cyclotron System (Under Development)
H2
+ Ion
Source Injector Cyclotron (Resistive Isochronous) Ring Cyclotron (Superconducting) “Isochronous cyclotron” where
but RF does not change with time. This can accelerate many bunches at once.
DAR Target-Dump (about 6x6x9 m3)
IsoDAR Cyclotron
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Submitted to NIM Columbia, Huddersfield, IBA, Maryland, MIT, PSI, INFN-Catania, INFN –Legnaro, RIKEN, Wisconsin
Academics: Neutrino Physicists, Accelerator Physicists And also Scientists at a Corporation
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Ion source Injector Superconducting Ring Cyclotron Target/ Dump
Phase I: The Ion Source
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source solenoid lens slits & diagnostics
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Beam to be characterized at Best Cyclotrons, Inc, Vancouver This spring (NSF funded) Results to be available by Cyclotrons’13 Conference, Sept 2013, Vancouver
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Ion source Injector Superconducting Ring Cyclotron Target/ Dump
We have a workable ion source for a Phase II
A sterile neutrino experiment On its own!
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⇒ being developed as prototype injector for DAEδALUS cyclotron system
scintillator/water detectors such as KAMLAND, SNO+, Borexino, Super-K….
– νe disappearance measurement in the region of the LSND and reactor- neutrino anomalies. – Measure oscillatory behavior within the detector as a function of L and E.
Overview IsoDARν νe Disappearance Exp
Detector Blanket/ Shield
Target cyclotron protons
Phys Rev Lett 109 141802 (2012) arXiv:1205.4419
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IsoDAR Neutrino Source and Events
arXiv:1205.4419
– plus many neutrons since low binding energy
– Meanνe energy = 6.5 MeV – 2.6×1022νe / yr
– Use IBDνe + p → e+ + n process – Detector center 16m from source – ~160,000 IBD events / yr – 60 MeV protons @ 10ma rate – Observe changes in the IBD rate as a function of L/E
5 yrs
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IsoDAR at Kamland
Potential Location of ν Source
Currently working with the Kamland collaboration
cyclotron, beamline, and neutrino source.
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Detectν νe Events using Inverse Beta Decay (IBD)
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IsoDAR ν νe Disappearance Oscillation Sensitivity (3+1)
5 yrs νe →νe
5σ
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IsoDAR Measurement Sensitivity
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IsoDAR’s high statistics and good L/E resolution has potential to distinguish (3+1) and (3+2) oscillation models Oscillation L/E Waves in IsoDAR
5 yrs 5 yrs Observed/Predicted event ratio vs L/E including energy and position smearing νe →νe νe →νe
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Possibility to Probe Lower Δm2 using Super-K
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Beyond Oscillations: IsoDAR sin2θW Measurement
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ν νee Elastic Scattering ⇒ Measure sin2θW
scattering differs from expectation by 3σ
– Is there something special with neutrinos or difficulty in NuTeV analysis?
⇒ Use IsoDAR/Kamland to measure sin2θW with pure lepton process antineutrino-electron elastic scattering:ν
νe + e → ν νe + e
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Kamland Backgrounds toν νee Signal
large since signal is single outgoing electron
low since outgoing νe takes away energy
From L. Winslow electron kinematics Cuts:
⇒ Reduce isotropic bkgnd by x2 Use large sample of IBD events to constrain normalization to 0.2%
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IsoDAR sin2θW Measurement Sensivity
⇒ IsoDAR/Kamland: δsin2θW = 0.0075 (~3%)
– Not as good as NuTeV: sin2θW = 0.2277 ± 0.0016 (0.7%) – But would be bestνee elastic scattering measurement (See 3% band below)
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Final Comments
particle physics
– Some tension with lack of νµ disappearance signals
– New experiments to have better sensitivity (~5σ level) with capabilities to see oscillatory behavior.
– Advantage over reactor and radioactive sources in having neutrinos with x3 higher energy – Source is compact with a very well understood energy spectrum and can be setup near an existing large detector – Combined L and E analysis can isolate the oscillatory behavior and reduce backgrounds – Can turn beam off to measure background – R&D is well underway to produce a high-intensity compact 60 MeV cyclotron to drive the neutrino source (See talk by Matt Toups)