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Search for Proton Decay in Super-Kamiokande
Yusuke SudaMini-Workshop for High Energy Gamma Ray Astrophysics
Max-Planck-Institute for Physics, Nov. 24, 2017
Who am I• I am Yusuke Suda from Univ. of Tokyo, Japan
• Master of Science (Mar. 2014)
• “Research and Development of Large-Aperture Hybrid Photo-Detectors for Hyper-Kamiokande”
• Doctor of Philosophy (Sep. 2017)
• “Search for Proton Decay Using an Improved Event Reconstruction Algorithm in Super-Kamiokande”
• Postdoc at Center for High Energy gEophysics Research (CHEER), Earthquake Research Institute (ERI), UTokyo
• Muon radiography (Muography) for geoscience
2
First
What is Proton Decay• Phenomena predicted by Grand Unified Theories (GUTs) of
elementary particles
• Unification of three fundamental forces (EM, Weak, Strong)
• Very high energy scale ( ≧1015 GeV)
• Solve electromagnetic charge quantization, etc.
• Mixture between quarks and leptons → Proton decay
• Proton decay is the best tool to test GUTs!
3
Accelerators
Prot
on
⇡0
↵↵
Predicted Proton lifetime:1032 - 1039 years
⌧ ⇠ M4X
↵2m5p
Year1940 1960 1980 2000 2020 2040
Life
time
Lim
it (y
ears
)
2110
2510
2910
3310
3710 0π+ e→Minimal SU(5), p0π+ e→Minimal SO(10), p
Goldhaberet alFlerov
Evans & SteinbergFiremanBennett
(1954)et alReines (1958)et alReines
et alBackenstoss Giamati & ReinesKropp & Reines
et alGurr Bergamasco & PicchiReines & Crouch
et alLearned (NUSEX)et alBattistoni
(KGF)et alKrishnaswamy (Soudan)et alBartelt (Frejus)et alBerger (Homestake)et alCherry
(Kamiokande)et alHirata (IMB)et alMcGrew
(Super-K I)et alShiozawa (Super-K I-II)et alNishino
(Super-K I-IV)et alAbe
Proton Decay So Far
4
SO(10) GUT
SU(5) GUT
Water Cherenkov
Iron Calorimeter
Liquid Scintillator
Geochemical Radiochemical
(1954)
• Long history of over 60 years. No significant candidate
• Super-Kamiokande (SK) is the top and still in predictions
• Proton decay may happen at any time
• Let’s search proton decay in SK!
Baryon number conservation
5
Super-KamiokaNDE• 50kton water Cherenkov detector
• 1000m underground, Kamioka, JPN
• Record Č light (Q・T) by 20-inch PMTs
• PID by Č ring pattern
SK1 SK2 SK3 SK4
Period 1996-2001 2002-2005 2006-2008 2008-
Live time 1489.2 798.6 518.1 2650.4(~Sep. 2016)
Photocoverage(# of PMTs)
40%(11,146)
19%(5,182)
40%(11,129)
40%(11,129)
Outer Detector
(veto)
InnerDetector
50kton Tank
ucleonecay
xperiment
39.3 m
41.4
m
Half of the all data
e, γ
Fuzzy
μ
Sharp
6
7
1033 protons in inner detector
10 years null observation of proton decay→ Proton lifetime > 1034 years
8
My target decay mode: p→e+π0 ・Most dominant in non-SUSY GUTs ・Most sensitive for SK
Decay time of π0: 8×10-17 s Gamma conversion length: ~40cm
9
Back-to-back topology→ Easily distinguish from
atmospheric neutrinos
e+
γ
γ
Proton Decay Simulation
Elec.
Cable hole μ
Invisible μ
Stopping μ
Through-going μ
Radioactive BG
FC neutrino
VETO
Rock
PC neutrino
UPMU neutrino
Flasher
Proton decay
Michel e
Michel e
Data Flow
10
106 events/day
8 events/day
Reconstruction
Proton decay search
Fully contained reduction(no OD activity, no flasher
PMT etc.)
Mostly atmospheric neutrino events
(BG for proton decay)
Vertex, #rings, PID, momentum etc.
Cut-based analysis
I was an expert of fully contained reduction(trouble shooting, preparation for data set etc.)
Reconstruction Algorithm• Conventional: APfit
• Determine reconstruction params. step-by-step (vertex → #rings → PID → momentum)
• Use charge&time information of “hit” PMT only
• Momentum determination by using observed charge inside Č-cone w/ a half angle of 70° → Bias
• Developed 20 years ago and written by Fortran (hard to maintain)
• New: fiTQun
• Determine all params simultaneously by a maximum likelihood method
• Use not only hit PMT information but also “unhit” PMT information
• Initial development by the T2K experiment, written by C++ 11
12
fiTQun
Charge PDF Time PDFUnhit PDF
Distance btw. true/recon. vertex (cm)0 10 20 30 40 50 60 70 80 90 100
Num
ber o
f Eve
nts
0
500
1000
1500
2000
2500
3000
3500
4000
): σResolution (1: 19.6 cm (Dwall>1.5m)fiTQun: 19.5 cm (Dwall>2.0m)fiTQun
: 29.6 cm (Dwall>2.0m)APfit
True Momentum (MeV/c)0 200 400 600 800 1000 1200 1400
Mom
entu
m R
esol
utio
n (%
)
0123456789
10
(Dwall>1.5m)fiTQun (Dwall>2.0m)fiTQun
(Dwall>2.0m)APfit
Hit PDF
Vertex Resolution Momentum ResolutionEx) Atm.-νe CCQE MC
(Poisson w/ correction)
• Fit params. x = {x, y, z, t, θ, φ, p} × (# of rings)• Construct likelihood function for given ring(s) hypotheses• Maximize likelihood for each event
(Poisson) (Gaussian)
Observed Q&T
)µLe/Lln(-3000 -2000 -1000 0 1000 2000 3000
Num
ber o
f Eve
nts
0
100
200
300
400
500
600
700
800 SK-IV DataπCC w/o eν
oth.0πCC w/ 0eν 0πCC w/ eνπCC w/o µν
oth.0πCC w/ 0µν0πCC w/ µν
NC
Validation of fiTQun• Performance in MC was well examined, but treatment of real
data was not enough to physics analysis
• I did
• Check in data/MC likelihood distributions
• Correction of time dependent detector params.
• Estimation of energy scale uncertainty
• Uncertainty 2.1%, same as APfit
• Tuning of ring counting parameter
• Finally, fiTQun has been verified for SK-IV data/MC
• Then, T2K experiment employed fiTQun for their analysis and announced a new hint for leptonic CP violation in summer 2017
13
PID μ←→e
Elapsed Years0 1 2 3 4 5 6 7 8
PMT
Gai
n (a
.u.)
0.95
1
1.05
1.1
1.15
1.2
Calibration of fiTQun
14
Date1996 1998 2000 2002 2004 2006 2008 2010 2012 2014 2016 2018
Wat
er A
ttenu
atio
n Le
ngth
(m)
50
60
70
80
90
100
110
120
130
PMT gain corr. Water Atten. corr.w/o corr.
Mom
entu
m/R
ange
(M
eV/c
/cm
)
Ex) SK1
RMS/Mean=2.2% RMS/Mean=1.0% RMS/Mean=0.6%
SK1SK2SK3SK4
Year
+2%/year
• PMT gain and water attenuation length vary with time
PMT Gain Water Attenuation Length
Search for Proton Decay• First application of fiTQun to proton decay
• First time of changing SK proton decay analysis framework
• Target decay mode: p→e+π0
• Hybrid search: APfit (SK1-3, null observation) + fiTQun (SK4)
• Selection criteria
15
1. Fiducial volume
2. Number of rings (2 or 3)
3. PID (all shower ring, no Micheal-e)
4. π0 mass (for 3-ring events)
5. No gamma-ray from neutron capture
6. Total invariant mass and momentum cut
Distance from the wall to the true vertex (cm)0 200 400 600 800 1000 1200 1400 1600 1800
Effic
ienc
y in
eac
h bi
n
0
0.2
0.4
0.6
0.8
1
1.2
16
• By changing selection criteria for fiTQun, I did
• Expand fiducial volume by 10%
• Reduce # of BG events by arrpox. 30%
• Tighter total invariant mass cut is applied
• While keeping similar level of signal efficiency as APfit
fiTQun free-pAPfit free-p
fiTQun all-pAPfit all-p
APfitfiTQun
Chance of discovery!(22.5 kton → 24.7kton)
17
fiTQun APfitLower box Upper box Lower box Upper box
Eff. (all) (%) 20.0±0.3 18.1±0.3 19.0±0.3 19.0±0.3BG (/Mt/yr) 0.028±0.019 0.778±0.102 0.030±0.021 1.116±0.132
*stat. error only
Bound-pFree-p
Signal MC Atm-ν MC (500 years)
• To enhance sensitivity, signal region is divided by two
• Lower box: less BGs & systematics error (Fermi motion)
• #total BG in SK4: ~0.14 (0.19) events for fiTQun (APfit)
Upper boxLower box
Result
18
)2Total Invariant Mass (MeV/c0 200 400 600 800 1000 1200
Tota
l Mom
entu
m (M
eV/c
)
0
100
200
300
400
500
600
700
800
900
1000
)2Total Invariant Mass (MeV/c0 200 400 600 800 1000 1200
Tota
l Mom
entu
m (M
eV/c
)
0
100
200
300
400
500
600
700
800
900
1000
APfit (163.0 kton*years)fiTQun (179.5 kton*years)
SK-IV SK-IV
• No candidate was found in SK-IV data for both fitters
• Combine with the other SK data (APfit, no candidates) and calculate lower lifetime limit by Bayes’ theorem
• Lifetime limit: τ/B(p→e+π0) > 1.88×1034 years @ 90% C.L.
• 5% improvement from APfit-based analysis
Not official yetNot official yet
Signal box
Summary• Proton decay is a smoking gun for GUTs
• Developed and validated the new event reconstruction algorithm, fiTQun
• Improved search for p→e+π0 with fiTQun was conducted
• Same efficiency but fiducial volume +10%, #BGs -30%
• No candidate was found
• World leading proton lifetime limit: 1.88×1034 years @ 90% C.L.
• Most stringent constraint for non-SUSY GUT
19
Detail information can be found in Suda’s thesis http://www-sk.icrr.u-tokyo.ac.jp/sk/publications/index-e.html#doctor
20Let’s go as much as we can!
74 m
60 m
Think Bigger
• Hyper-Kamiokande project (~10 times bigger than SK)
• Search region of proton decay will reach 1035 years
• Many rich physics: CP violation, ν mass hierarchy, SN relic etc.
• FiTQun is compatible with HK
• Photosensor is a key to success21
Hyper-K
Super-K
KAMIOKANDE 1983
1996
2026 (expected)
/ ndf 2χ 473.8 / 161Prob 1.465e-32p0 6.4± 375.9 p1 0.057± 9.577 p2 0.064± 2.133 p3 7.0± 587.1 p4 0.1± 18.8 p5 0.122± 3.304 p6 14.7± 652.2 p7 0.1± 27.8 p8 0.149± 3.082 p9 39.8± 510.5 p10 0.20± 36.37 p11 0.285± 3.413 p12 8.2± 389.9 p13 0.45± 46.07 p14 0.634± 5.003
Charge [pC]0 20 40 60 80 1000
100
200
300
400
500
600
700 / ndf 2χ 473.8 / 161
Prob 1.465e-32p0 6.4± 375.9 p1 0.057± 9.577 p2 0.064± 2.133 p3 7.0± 587.1 p4 0.1± 18.8 p5 0.122± 3.304 p6 14.7± 652.2 p7 0.1± 27.8 p8 0.149± 3.082 p9 39.8± 510.5 p10 0.20± 36.37 p11 0.285± 3.413 p12 8.2± 389.9 p13 0.45± 46.07 p14 0.634± 5.003
Multi-photoelectron distribution
Avalanche Diode
8-inch
200ton tank
Cosmic-ray μInstall
R&D of Hybrid Photo-Detector• One of candidates. Better performance than SK PMT
• Hope to use in HK (20-inch HPD is testing in water tank)
22
SudaHPD
Photon counting!
1PE
Photon counting!
2PE 3PE4PE
5PE
Current Research
23
↑ Satsuma-Iwojima Volcano, Japan
H. Tanaka, 2009
2m
3m2mScintillation detector →
μ
Magma
• Muon radiography (Muography) @ Earthquake research institute, Japan
• Explore inner structure of volcanos and active fault by measuring cosmic-ray muon flux through target
• Commit to geophysics and disaster prevention
• One of the few applications of high energy physics
Active Fault
24
• Muography of Atotsugawa fault (near Super-K)
• Estimation of 3D density profile of the fault by measuring muon flux (θ, φ) at each depth (Data taking is ongoing)
• I will evaluate expected muon flux at detector by GEANT4
• Working hard to publish the world’s first result
Borehole
Fractured zone(low density)
Rock
Detector
μTerrain @ GEANT4
Scintillation muon detector
Transition of My Research
25
Past
Now
Future?
Expected Future Work
26
• Gamma-ray burst search @ CTA LST
• GRB is the brightest explosion in the universe
• Explore mechanisms of jet formation and particle acceleration especially for long GRBs with LST’s high statistics data
• I would like to contribute to
• Low energy threshold (20GeV or less) in order to detect GRBs
• PMT calibration and analysis tool development utilizing my experience (fiTQun, HPD, etc.)
• Pointing calibration in order to not miss GRBs
• Eager to accomplish the first measurement of a GRB by the ground based telescope