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Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute for Physics, Nov. 24, 2017

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Page 1: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

Search for Proton Decay in Super-Kamiokande

Yusuke SudaMini-Workshop for High Energy Gamma Ray Astrophysics

Max-Planck-Institute for Physics, Nov. 24, 2017

Page 2: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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

Page 3: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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

Page 4: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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

Page 5: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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

Page 6: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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Page 7: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

7

1033 protons in inner detector

10 years null observation of proton decay→ Proton lifetime > 1034 years

Page 8: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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

Page 9: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

9

Back-to-back topology→ Easily distinguish from

atmospheric neutrinos

e+

γ

γ

Proton Decay Simulation

Page 10: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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.)

Page 11: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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

Page 12: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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

Page 13: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

)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

Page 14: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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

Page 15: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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

Page 16: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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)

Page 17: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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

Page 18: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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

Page 19: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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

Page 20: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

20Let’s go as much as we can!

Page 21: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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)

Page 22: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

/ 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

Page 23: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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

Page 24: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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

Page 25: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

Transition of My Research

25

Past

Now

Future?

Page 26: Search for Proton Decay in Super-Kamiokande...2017/11/24  · Search for Proton Decay in Super-Kamiokande Yusuke Suda Mini-Workshop for High Energy Gamma Ray Astrophysics Max-Planck-Institute

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