meg 最初の一年、その展望

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Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama 1 MEG MEG 最最最 最最 最最最最 一、 最最最 最最 最最最最 一、 最最最最最最最最最最最最最最最最最 最最最最最最最最最最最最最最最最最 最最 最 最最 最

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MEG 最初の一年、その展望. 東京大学素粒子物理国際研究センター 三原 智. Contents. Introduction MEG Detector Sensitivity and background Our schedule Summary. Introduction. n e. n m. e. μ. μ. e. W. Br( m e g ) ∝ (sin q m e (m m 2 -m e 2 )/m 2 SUSY ) 2. ~. ~. ~. ~. g. g. μ → e γ. - PowerPoint PPT Presentation

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Page 1: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama1

MEGMEG最初の一年、その展望最初の一年、その展望

東京大学素粒子物理国際研究センター東京大学素粒子物理国際研究センター

三原 智三原 智

Page 2: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama2

ContentsContents

• IntroductionIntroduction

• MEG DetectorMEG Detector

• Sensitivity and backgroundSensitivity and background

• Our scheduleOur schedule

• SummarySummary

Page 3: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama3

IntroductionIntroduction

Page 4: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama4

• Lepton Flavor Violation (LFV) is strictly forLepton Flavor Violation (LFV) is strictly forbidden in SMbidden in SM

• Neutrino oscillationNeutrino oscillation– LF is not conservedLF is not conserved

– Contribute (m∝Contribute (m∝ /m/mWW))44

• SupersymmetrySupersymmetry– Off-diagonal terms in the slepton mass matrixOff-diagonal terms in the slepton mass matrix

μ e

W

e

μμ→→eeγγ

233

232

231

223

222

221

213

212

211

2~

mmm

mmm

mmm

ml

μ e

0~x

e~~

Just below the current limit

Br(μ→eγ) = 1.2 x 10-11

(MEGA, PRL 83(1999)83)

Br(e) (sin∝ e(m2-me

2)/m2SUSY)2~~ ~ ~

Page 5: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama5

Other LFV search experimentsOther LFV search experiments

• , e, e– KEK, BELLEKEK, BELLE– SLAC, BABARSLAC, BABAR

• -e conversion-e conversion– J-PARC, PRISM project, PRIMEJ-PARC, PRISM project, PRIME

Page 6: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama6

MEGMEG

ee decay search experiment at Paul Sche decay search experiment at Paul Scherrer Institutrrer Institut

Japan, Italy, Switzerland, Russia, USAJapan, Italy, Switzerland, Russia, USA

Page 7: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama7

Signal and BackgroundSignal and Background

• SignalSignal

• EE = m = m/2 = /2 = 52.8MeV52.8MeV

• EEee = m = m/2 = /2 = 52.8MeV52.8MeV

• = 180= 180oo

• Time coincidenceTime coincidence

• BackgroundBackground– Radiative Radiative decay decay

– Accidental overlapAccidental overlap

ee

ee

ee????

Page 8: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama8

EssentialsEssentials

• Intense muon beamIntense muon beam– DC beam is better to reduce accidental pile-up eventsDC beam is better to reduce accidental pile-up events

• Gamma DetectorGamma Detector– Good resolutionsGood resolutions– Capability of identifying pile-up eventsCapability of identifying pile-up events

• Positron DetectorPositron Detector– Good resolutionsGood resolutions– Low amount of materialLow amount of material– Blind to low energy positronsBlind to low energy positrons

Liquid Xenon DetectorLiquid Xenon Detector

COBRA spectrometerCOBRA spectrometer

Page 9: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama9

PSI Proton CyclotronPSI Proton Cyclotron

Proton energy: 590MeVNominal operation current: 1.8mA.Max > 2.0mA possible.

Target unit Target flask

MEG

Page 10: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama10

MEG DetectorMEG Detector

• Liquid xenon photon detectorLiquid xenon photon detector• COBRA spectrometer – Magnet, DC, TCCOBRA spectrometer – Magnet, DC, TC• All detector waveforms are recorded.All detector waveforms are recorded.

Page 11: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama11

Beam LineBeam Line• Length 10.4 mLength 10.4 m• Solid angle 150 msrSolid angle 150 msr• Momentum acceptance (FWHM) 10 %Momentum acceptance (FWHM) 10 %• Momentum resolution (FWHM) 2 %Momentum resolution (FWHM) 2 %

SepSepSepSep

Trip ITrip ITrip ITrip I Trip IITrip IITrip IITrip II

ASCASCASCASC

BTSBTSBTSBTS

COBRACOBRACOBRACOBRA

XXXX

YYYY

森田裕一 “MEG実験におけるビームチューニング”  29日午後森田裕一 “MEG実験におけるビームチューニング”  29日午後

separatorBeam Transport Solenoid Target

Page 12: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama12

Beam Line Commissioning• 2005 mid July – end August2005 mid July – end August

– Beam Transport Solenoid (BTS) Beam Transport Solenoid (BTS) CommissioningCommissioning

– Bfield mappingBfield mapping– Phase space measurements up to end BTSPhase space measurements up to end BTS

• 2005 beg November – end December2005 beg November – end December– Commissioning BTS with Cryo-plant and Commissioning BTS with Cryo-plant and

Control systemControl system• BTS automated operationBTS automated operation

– Phase Space measurements inside COBRAPhase Space measurements inside COBRA• Pill scinti + APD on 3-D measuring machinePill scinti + APD on 3-D measuring machine

USUSUSUS DSDSDSDS

•End-caps and insertion systemEnd-caps and insertion system•Complex design He/Vacuum/N2/Air interfaceComplex design He/Vacuum/N2/Air interface• Materials minimized Al & CH2/EVAL (background)Materials minimized Al & CH2/EVAL (background)

Calibration target installation

Page 13: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama13

Target System

• Various solutions under study– Target material

• Rohacell form/CH2 combination• Complete Rohacell• CH2 or polystyrene Target + wire frame

DCDCStructureStructure

InsertionInsertionBellowsBellows

Page 14: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama14

COBRA Magnet

• 360A, 1.27T• 0.197X0 around the center

Compensation coil (NC)

Inner/Outer end coil (SC)

Gradient coil (SC)

Central coil (SC)

Page 15: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama15

COBRA Magnet

• Cooling by using two GM-type refrigerators– No need of helium for operation

• Compensation coil to reduce field strength around the xenon detector

• Field measurement has been completed recently

Design fieldDesign field

Measured field around the xenon detectorMeasured field around the xenon detector

Page 16: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama16

Liquid Xenon Detector

• 800~900 liquid xenon• 846 PMTs immersed in the liquid• No segmentation

• Why Liquid Xe ?– Good resolutions

• Large light output yield• Wph(1MeV e) = 22.4eV

– Pile-up event rejection• Fast response and short decay time• s = 4.2nsec, =45nsec (for electron, no E)

•西村康宏 “MEG実験用光電子増倍管の液体キセノン中における LEDを用いた利得解析と現状”  27日午後•西村康宏 “MEG実験用光電子増倍管の液体キセノン中における LEDを用いた利得解析と現状”  27日午後

Page 17: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama17

Depth Reconstruction

• Broadness of light distribution at the entrance side

waveform

shallow deep

Page 18: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama18

PMT test in LXe

• All PMTs were tested in LXe before installing to the detector– Pisa LXe PMT test facility

– Xenon Detector Large Prototype

• QE, Gain, response linearity• All information is stored in a database for future u

se.

No zenerNo zener

with zenerwith zenerBad

Page 19: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama19

Construction Status

•Cryostat Construction in progress in Italy

•Delivery in June

•PMT installation and setup after that

•Ready in September

•Cryostat Construction in progress in Italy

•Delivery in June

•PMT installation and setup after that

•Ready in September

Page 20: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama20

DCDC

• Position resolutions (~300Position resolutions (~300m) for m) for both r and z.both r and z.

• Vernier pad readout for z measureVernier pad readout for z measurementment

• Low amount of materialLow amount of material

• Need very precise pressure controNeed very precise pressure control ~1Pal ~1Pa

Page 21: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama21

TC

TC Final Design

PM-Scintillator Coupling

Scintillator Housing

BC404-Scintillator slab

Main Support

ladder Board& cabling

PM

APD

APD F.E. Board

Scintillating Fibers (Phi Counter)

APD Cooled Support

• A PLASTIC SUPPORT STRUCTURE ARRANGES THE SCINTILLATOR BARS AS REQUESTED

• THE BARS ARE GLUED ONTO THE SUPPORT

• INTERFACE ELEMENTS ARE GLUED ONTO THE BARS AND SUPPORT THE FIBRES

• FIBRES ARE GLUED AS WELL

• TEMPORARY ALUMINIUM BEAMS ARE USED TO HANDLE THE DETECTOR DURING INSTALLATION

• PTFE SLIDERS WILL ENSURE A SMOOTH MOTION ALONG THE RAILS

Page 22: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama22

TC Assembly

• PMT test completed• Assembly test started

Page 23: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama23

Electronics

Page 24: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama24

Trigger Tree

. . . 14 boards

14 x 48Type1Type1

Type116

4

LXe front face

(216 PMTs)

2 boards

. . . 5+5+2 boards

9 x 48

Type1Type1

Type116

4

LXe lateral facesback (216 PMTs) 4 in 1

lat. (144x2 PMTs) 4 in 1 up/down

(54x2 PMTs) 4 in 1

1 board

Timing counterscurved (640 APDs) 8 in 1u/d stream (30x2 PMTs)

1 board

1 board

2 x48

Type2

Type2

Type2

Type2

Type2

. . . 9 boards

9 x 48Type1Type1

Type116

4

2 boards

2 x 48Type1Type1

16

4

16Drift chambers

16+16 channels

2 x48

1 x48

Type11 x48

16

4

Auxiliary devices16 channels

Page 25: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama25

Trigger Electronics

• PCB production finished• Currently board mounting in progress• Ready to install in June

Type 1

Type 2

Page 26: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama26

DAQ/Waveform Digitizer

DRS

R. Paoletti, N. Turini, R. PegnaMAGIC collaboration

USB

PSI GVME Board

FPGA with4 Power-PC

Page 27: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama27

DRS – Domino Ring Sampler0.2-1 ns Inverter (“Domino”) chain Rotating

signal

Input 1

Output 1

40 MHz

Input 2

Channels3 to 10

Output 2

Domino Ring

Sampler

Domino Ring

Sampler

Page 28: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama28

Waveform Analysis• Q,T evaluation from waveforms• Pile-up rejection• Waveform fitting is very CPU time

consuming

•Constant fraction

•Fraction:0.3, delay 10nsec

T=50ns. T=15ns

11MeV + 42MeV

Peak search method

Differential method

simulationsimulation

simulation simulation

•内山雄祐 “MEG実験用液体キセノン検出器の波形解析による性能評価”  27日午後•内山雄祐 “MEG実験用液体キセノン検出器の波形解析による性能評価”  27日午後

Page 29: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama29

Background and Sensitivity

PILE UP EVENTS RD+RD dominant

Energy deposit/ 52.8MeV

δθeγ= 14mrad100psec 1

4E7sec

# of

Bac

kgro

und

even

ts,

2 ye

ars

RU

N

Muon stopping rate [/sec]

Page 30: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama30

How Far Can We Go?

• Expected sensitivity at 90% C.L.

BEAMTIME=4E7 sec 2 year YEAR 20061 MONTH BEAMTIME

muon beam intensity (/sec) muon beam intensity (/sec)

Page 31: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama31

Schedule

• MEG beam time; Apr-Jun, Aug-Dec

• DC/TC run with beam; Sep-

• LXe– Setup; -Sep~Oct, Calibration run; ~Nov –– Ready in Nov

• DAQ/Trigger; Ready in Jun

• Ready to start DAQ; ~mid Nov

Page 32: MEG 最初の一年、その展望

Satoshi MIHARA, ICEPP Univ. of Tokyo, JSPS meeting in Matsuyama32

Summary

• MEG starts in 2006• Detectors are getting

ready• Analysis/online softwa

res also• For further informatio

n, visit http://meg.icepp.s.u-tokyo.ac.jp

•澤田龍 “汎用データ解析ソフトウェア生成ツール ROME&ARGUS”  30日午後•澤田龍 “汎用データ解析ソフトウェア生成ツール ROME&ARGUS”  30日午後