counting electrons to measure the neutrino mass hierarchy j. brunner 17/04/2013 apc
TRANSCRIPT
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Counting Electrons to Measure the Neutrino Mass Hierarchy
J. Brunner17/04/2013
APC
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Outline
• Oscillation Probabilities• Neutrino Cross Sections• The Proton Accelerator • The Neutrino Beam• Detector Performance• Event Rates / Result
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Oscillation Probabilities
• GLOBES for Baseline of 2600km (neutrinos)• CP phase in steps of 30 degree• 0,180 : magenta• 90,270 : orange• Width of CP-band– About 30%
• NH/IH 5
P(µe)
NH
IH
Thanks to A. Meregaglia for help with GLOBES
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Oscillation Probabilities
• All relevant oscillation probabilities taken into account
• Full 3-flavour treatment• CP-phase variations included
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Oscillation parameters
• Taken from Global Fit (Fogli et al.) for both hierarchy options
• CP phase left free
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Neutrino Cross sections
Simple parton scaling assumed (QE, Res. ignored)Flavour universality
m threshold
NC approximation
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Neutrino Cross sections
Simple parton scaling assumed (QE, Res. ignored)Flavour universality
m threshold
NC approximation
NC, CC: e µ Solid : neutrino , dashed : antineutrino
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Cross Section Weighted Posc
• Allows to find optimal energy range for MH determination• No flavour tagging or CC/NC separation used• Kinematical suppression of exploited
NH / IH Ratio of Integrals IH/NH (2.5 GeV - Emax)
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Cross Section Weighted Posc
• Optimal energy range for “event counting” 2-6 GeV• 11-14% suppression of IH w.r.t. NH
Ratio of Integrals IH/NH (2.5 GeV - Emax)
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Proton Accelerator Complex Protvino
Presentation S. Ivanov (IHEP) on 22/11/2012 @ CERN
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Proton Accelerator Complex Protvino
Presentation S. Ivanov (IHEP) on 22/11/2012 @ CERN
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Where is Protvino ?• Baseline 2588km ; beam inclination : 11.7˚ (cos = 0.2)• Similar distance to Frejus : 2400km• Deepest point 134km : 3.3 g/cm3
• With upgrade 1021 p.o.t. in 3 years might be feasible
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SKAT bubble chamber
Courtesy: R. Nahnhauer
p target
focus
Decay pipe55m
Shielding SKAT
140m270m
245m
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Beam parametrisation (1988)
• Neutrino Focus • Anti-Neutrino FocusScaling to ANTARES site
(0.245/2600)2
Z. Phys. C 40 (1988) 487
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Beam parametrisation (1988) • Very clean µ beam• Less than 1% contaminations from other flavours• Most neutrinos between 1-8 GeV
1988 publication140m decay tube
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Effective Mass• From study of A. Trovato for “default” ORCA detector• Vertex in instrumented volume• Reco Quality cut (track)• Conservative here – beam direction known, no background from atmospherics
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Effective Mass
• Same function used for all CC interaction– Same light output for µ and e ok
– Conservative for due to escaping neutrinos
• NC evaluated at E/2
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Flavour identification
• Need to separate “tracks” from “cascades”• 2004 @ Villars : C2GT project (F. Dydak)– CERN to Gulf of Taranto
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Flavour identification• 2004 @ Villars : C2GT project (F. Dydak)• Clean separation of µ CC and e CC at 0.8 GeV• OM spacing 3m
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Flavour identification
• Misidentification probability : – assume same for both directions
• 50% at 2 GeV random ; 20% at 5 GeV ; 10% at GeV
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Event rates
• Here : no flavour misidentification• CC Rates
• NC Rates
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Event rates• Event numbers for 1.5 1021 pots – NH : 1621 +/- 255 (CP-phase variations)– IH : 497 +/- 100 (CP-phase variations)
• 20 sigma statistical separation of both Mass Hierarchy hypotheses from signal
• 10000 muon events for beam normalisation
µ CC e CC NH
IH
No oscil
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Event rates
• Include Background and Flavour tagging• Total Background :
• Total Event Rate :
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Event rates• Event numbers for 1.5 1021 pots• 9-18% difference for NH/IH• 7 sigma statistical separation of MH hypotheses• With 3-4% syst uncertainty still 3 sigma for MH test• No assumption on energy reconstruction ! • Background largely independent from MH (& CP)
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Event rates• Event numbers for 1.5 1021 pots • 9-18% difference for NH/IH
• 7 sigma statistical separation of MH hypotheses• With 3-4% syst uncertainty still 3 sigma for MH test• No assumption on energy reconstruction !
Tracks Cascades
Total EvtTotal Bg NC
Total EvtTotal Bg NC
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Systematic Uncertainties
• Detector Response• Water parameters– Extensively studied in ANTARES
• Neutrino flux– Can be monitored with muon events
• Neutrino Cross Section– Ongoing and planned short baseline Experiments
• Oscillation parameters– ORCA with atmospheric neutrinos
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Conclusion
• Powerful proton accelerator at Protvino well suited for LBL towards Mediterranean Sea
• Preliminary Performance Figures of ORCA encouraging
• Complementary to measurement with atmospheric neutrinos
• High Significance determination of Mass Hierarchy after few years of data taking