μ-e conversion 実験 @J-PARC
- -- COMET ---
Koji Y
- shimura, KEK
- n behalf of COMET collaboration
- e conversion @J - PARC --- COMET --- Koji Y oshimura, KEK on - - PowerPoint PPT Presentation
- e conversion @J - PARC --- COMET --- Koji Y oshimura, KEK on behalf of COMET collaboration Most slides were inherited from Aoki - sans talk
μ-e conversion 実験 @J-PARC
Koji Y
The COMET Collaboration (as of October 16, 2008)
The (quasi) COMET Collaborators
The COMET collaboration is approaching to ....
Muon Task Force, Muon Working Group and the COMET collaboration
COMET collaboration Muon g-2 Japan Group Muon Working Group
(discussing Japanese activities of muon particle physics)
KEK Muon Task Force
Contents
ransport and Muon Stopping Target
nuclei
µ−
Muon Decay in Orbit (MDO) charged Lepton Flavor Violation (c-LFV)μ-e Conversion
Muon Capture(MC)BR[µ− + (A, Z) → e− + (A, Z)] ≡ Γ[µ− + (A, Z) → e− + (A, Z)] Γ[µ− + (A, Z) → νµ + (A, Z − 1)]
µ− + (A, Z) → e− + (A, Z)in foreseeable future.
charged Lepton Flavor Violation
Physics of μ-e Conversion
→ e-N, not for μ→e γ
Physics of μ-e Conversion
→ e-N, not for μ→e γ
c-LFV and SUSY
Physics of slepton mass matrix SUSY
m2
˜ e˜ e
∆m2
˜ e˜ µ
∆m2
˜ e˜ τ
∆m2
˜ µ˜ e
m2
˜ µ˜ µ
∆m2
˜ µ˜ τ
∆m2
˜ τ ˜ e
∆m2
˜ τ ˜ µ
m2
˜ τ ˜ τ
c-LFV slepton mixing
Theoretical Predictions
Process Current Limit SUSY-GUT level Future µ N → e N 10-13 10-16 10-16,10-18 µ → e γ 10-11 10-14 10-13 τ → µ γ 10-6 10-9 10-8
PRSM/PRIME MEG Courtesy Hisano PRISM/PRIME MEG SUSY+Seesaw, MSW Large Angle SUSY-GUT COMET COMET tanβ=3 tanβ=10 tanβ=30 m2
˜ e˜ e
∆m2
˜ e˜ µ
∆m2
˜ e˜ τ
∆m2
˜ µ˜ e
m2
˜ µ˜ µ
∆m2
˜ µ˜ τ
∆m2
˜ τ ˜ e
∆m2
˜ τ ˜ µ
m2
˜ τ ˜ τ
Golden T rio
e ̃ e ̃ B ~ mixing large top Yukawa coupling ̃ ̃g-2 EDM
Real Imaginary
τ-LFV
slepton mass matrix
Principal of Experiment
γ → e+ e-
SINDRUM II
BR < 7 × 10-13COMET @ J-PARC
Physics Capabilities of mu-e
J-PARC PAC report about COMET US P5 Report
Pulsed Proton Beam
Nbg = NP×Rext×Yπ/P×Aπ×Pγ×A NP : total # of protons (~1021) Rext : Extinction Ratio (10-9) Yπ/P : π yield per proton (0.015) Aπ : π acceptance (1.5×10-6) Pγ : Probability of γ from π (3.5×10-5) A : detector acceptance (0.18) BR=10-16, Nbg < 0.12 ⇔ Extinction < 10-9
Arbitrary Unit 1 Prompt Background Stopped Muon Decay Main Proton Pulse 10 p/pulse 8 Timing Window ( μ s ) Time Signal 100 ns 1.1 μsPulsed Proton@ J-PARC
→ Next talk by Tomizawa-san for details.
Additional Extinction Means
Pion Production & Capture
Detector Section Pion-Decay and Muon-Transport Section Pion Capture Section A section to capture pions with a large solid angle under a high solenoidal magnetic field by superconducting maget A detector to search for muon-to-electron conver- sion processes. A section to collect muons from decay of pions under a solenoi- dal magnetic field. Stopping Target Production TargetPion Production
ater cooling or Radiation cooling
Pion Capture
< 100 W on SC coil
0.05 (π+μ)/8-GeV-proton
μ-yield vs. Bmax 10MARS simulation
π-Capture Solenoid
(20cm-Cu SC coil : 1 kW)
30 mm × 5 mm NbTi 1.28 mm diameter 32 strands NbTi: Cu: Al = 19%: 34%: 46% density: 4.0 g/cm3
Al-SC: one of world leading expertise of KEK
Muon Beamline and Muon Stopping Target
Detector Section Pion-Decay and Muon-Transport Section Pion Capture Section A section to capture pions with a large solid angle under a high solenoidal magnetic field by superconducting maget A detector to search for muon-to-electron conver- sion processes. A section to collect muons from decay of pions under a solenoi- dal magnetic field. Stopping Target Production TargetMuon Beamline
Guide π’s until decay to μ’s Suppress high-P particles
High-P Suppression
D[m] = 1 0.3 × B[T] × s R × p2
l + 1 2p2 tpl
V ertical Drift in Torus
See “Classical Electrodynamics”, J.D.Jackson Ch.12-Sec.4 Momentum (MeV) 20 40 60 80 100 120 140 160 180 200 y (cm)δP/δx = 1 MeV/c/cm
Muon Stopping Target
Curved Solenoid Spectrometer
Detector Section Pion-Decay and Muon-Transport Section Pion Capture Section A section to capture pions with a large solid angle under a high solenoidal magnetic field by superconducting maget A detector to search for muon-to-electron conver- sion processes. A section to collect muons from decay of pions under a solenoi- dal magnetic field. Stopping Target Production TargetCurved Solenoid Spectrometer
60-MeV/c DIO electrons
D[m] = 1 0.3 × B[T] × s R × p2 l + 1 2p2 t pl105-MeV/c μ-e electron
Electron Total Energy (MeV) 20 40 60 80 100 Transmission Efficiency 0.05 0.1 0.15 0.2 0.25 0.3 0.35 0.4 Transmission EfficiencyElectron Detectors
rigger calorimeter
Detector Acceptance & Signal Sensitivity
Acceptance Geometrical Acc. 0.74 Electron T ransport 0.32 pt > 52 MeV/c 0.66 χ2 Cut (χ2 < 9) 0.89 Energy Selection 0.52 Timing cut 0.38 Total 0.028 Cycle Time 1.5 sec 0.9 sec Proton Intensity 4 × 1013 Hz 7 × 1013 Hz Running Time 2 × 107 sec 2 × 107 sec μ’s yields per proton 0.004 0.004 μ-stopping efficiency 0.3 0.3 Total 1.1 × 1018 stopped μ’s 1.8 × 1018 stopped μ’sB(µ− + Al → e− + Al) = 1 Nµ · fcap · Ae
< 5 × 10-17 (90% C.L.)
Backgrounds
Background estimates for COMET *: assuming the extinction 10-9
Background Events Comments Muon decay in orbit 0.05 230 keV (sigma) assumed Pattern recognition errors <0.001 Radiative muon capture <0.001 Muon capture with neutron emission <0.001 Muon capture with charged particle emission <0.001 Radiative pion capture* 0.12 prompt pions Radiative pion capture 0.002 due to late arriving pions Muon decay in flight* <0.02 Pion decay in flight* <0.001 Beam electrons* 0.08 Neutron induced* 0.024 for high energy neutrons Antiproton induced 0.007 for 8 GeV protons Cosmic rays induced 0.1 with 10-4 veto inefficiency Total 0.4COMET to PRISM
COMET:BR<10-16
5 m PRISM Phase Rotated Intense Slow Moun source PRIME PRISM Muon to Electron conversion experiment Pion Decay Muon Transport FFAG Phase-Rotator Muon-Stopping Target Proton Beam PRIME Detector Pion CapturePRISM:BR<10-18
Why Staging, why 10-18
real-world step by step; we may see something new in every step
space
COMET and mu2e
COMET @ J-PARC mu2e @ Fermilab
Detector Section Pion-Decay and Muon-Transport Section Pion Capture Section A section to capture pions with a large solid angle under a high solenoidal magnetic field by superconducting maget A detector to search for muon-to-electron conver- sion processes. A section to collect muons from decay of pions under a solenoi- dal magnetic field. Stopping Target Production TargetJ-PARC -- FNAL/Booster U-curve -- S-curve U-curve -- Straight
MELC → MECO →
mu2e and COMET
MECO mu2e COMET Machine BNL/AGS FNAL Booster+Debuncher J-PARC/MR Energy 7.5 GeV/c 8 GeV/c 8 GeV/c Pulse 1.4 μs 1.7 μs 1.2 μs Beam Power 56 kW 20 kW 50-100 kW Extraction Bunched Slow ← ← Extinction 10-9 ← ← Target Heavy Metal ← Heavy Metal Muon Beamline S-Curved Solenoid S-Curved Solenoid U-Curved Solenoid + V ertical Field μ stop 1011 muons/s ← 1011 muons/s Detector Straight Straight Curved Rate 500 kHz/wire 100 kHz/wire 10-100 kHz/detector Sensitivity 10-16 ← ← Upgradability NO Project-X PRISM(10-18)Summary
TeV-scale physics.
and to world-leads muon particle physics.
down to a level of 10-16 at J-PARC. A proposal of COMET was already submitted to J-PARC/PAC.
location issue of COMET.
a good chance to join the COMET collaboration.
Join COMET
End of Slides
LFV 探索の現状
Reaction 90% CL Upper Limit B( µ + → eγ ) 1.2 ×10 −11 B( µ + → e +e −e +) 1.0 ×10 −12 B( µ −Ti → e − Ti) 6.1 ×10 −13 B( µ −Pb → e − Pb) 4.6 ×10 −11 B( µ −Ti → e + Ca) 1.7 ×10 −12 P( µ +e − → µ −e +) 8.3 ×10 −11 B(τ →eγ ) 2.7 ×10 − 6 B(τ → µγ ) 1.1 ×10 − 6 B(τ → µµµ) 1.9 ×10 − 6 B(τ → eee) 2.9 ×10 − 6 B( KL → µe) 4.7 ×10 −12 B( K + → π +µ +e −) 2.1 ×10 −10 B( KL → π 0µ ±e ) 6.2 ×10 − 9 B( D 0 → µe) 8.1×10 − 6 B( D 0 → τe) 5.3 ×10 − 4 B( D 0 → φµe) 3.4 ×10 − 5 B( B → µe) 3.5 ×10 − 6 B( B → Kµe) 1.8×10 − 5 B( Z → µe) 1.7×10 − 6 B( Z → τe) 9.8 ×10 − 6 B( Z → τµ ) 1.2 ×10 − 5 Based on a table written by Y. Kuno Updated in August, 2000ミュオンが大 変健闘してい る
µ-LFV 探索の歴史
1 0= µ-LFV探索の歴史 = フレーバー物理の歴史
==> 世代(フレーバー)概念
Slepton Mixing Mechanism
GUT Yukawa interaction Neutrino Yukawa interaction Quark mixing matrix Neutrino mixing matrix @ Plank mass scaleSUSY-GUT SUSY Seesaw Model
(m2 ˜ l )ij = m2 0δij (∆m2 ˜ l )ij = 0 (m2 ˜ L)21 ∼ 3m2 0 + A2 8π2 h2 tV ∗ tdVts ln MGUT MRS (m2 ˜ L)21 ∼ 3m2 0 + A2 8π2 h2 i U ∗ i1Ui2 ln MGUT MRS PRISM/Phase-1 LoI (2006)LHC and c-LFV
strengthened.
structure (SUSY-GUT, SUSY-Seesaw) will become more important.
SUSY particle
comes forefront.
μ-LFV
μ→eγ μ→eee μN→eN
μ→eγ, μ→eee, μN→eN
L = mµ Λ2 µRσµνeLFµν + 1 Λ2
F
(µLγµeL)(eLγµeL) + 1 Λ2
F
(µLγµeL)(qLγµqL)
c-LFVの一般的なラグランジアン
(A. de Gouvea, talk at Nufact’06)
μ→eγ μ→eee μN→eN
tree ×α ×α 1-loop tree
photonic non-photonic
Principal of Experiment
γ → e+ e-
SINDRUM II
PSI/πE5
SINDRUM II
BR < 7 × 10-13
μ-e Conversion vs. μ → e γ
μ→e γ
Physics is complemental
Different Background Mechanism Different Technologies Experiments are also complemental
μ-N → e-N
MECO, mu2e, PRISM and COMET
MECO BNL/AGS
Straw Tracker Crystal Calorimeter Muon Stopping Target Muon Beam Stop Superconducting Production Solenoid (5.0 T – 2.5 T) Superconducting Detector Solenoid (2.0 T – 1.0 T) Superconducting Transport Solenoid (2.5 T – 2.1 T) CollimatorsMECO BNL/AGS
Straw Tracker Crystal Calorimeter Muon Stopping Target Muon Beam Stop Superconducting Production Solenoid (5.0 T – 2.5 T) Superconducting Detector Solenoid (2.0 T – 1.0 T) Superconducting Transport Solenoid (2.5 T – 2.1 T) CollimatorsCancelled
Staging Strategy
On the evening before the MECO cancellation
5 m PRISM Phase Rotated Intense Slow Moun source PRIME PRISM Muon to Electron conversion experiment Pion Decay Muon Transport FFAG Phase-Rotator Muon-Stopping Target Proton Beam PRIME Detector Pion Capture !""# !""$ !""% !""& !"'" !"'' !"'! !"'( !"') !"'* !"'# !"'$ !"'% +,-.MECO:BR<10-16 PRISM:BR<10-18
Staging Strategy
On the evening before the MECO cancellation
5 m PRISM Phase Rotated Intense Slow Moun source PRIME PRISM Muon to Electron conversion experiment Pion Decay Muon Transport FFAG Phase-Rotator Muon-Stopping Target Proton Beam PRIME Detector Pion Capture !""# !""$ !""% !""& !"'" !"'' !"'! !"'( !"') !"'* !"'# !"'$ !"'% +,-.MECO:BR<10-16 PRISM:BR<10-18
Staging of PRISM
COMET:BR<10-16
5 m PRISM Phase Rotated Intense Slow Moun source PRIME PRISM Muon to Electron conversion experiment Pion Decay Muon Transport FFAG Phase-Rotator Muon-Stopping Target Proton Beam PRIME Detector Pion CapturePRISM:BR<10-18
Detector Section Pion-Decay and Muon-Transport Section Pion Capture Section A section to capture pions with a large solid angle under a high solenoidal magnetic field by superconducting maget A detector to search for muon-to-electron conver- sion processes. A section to collect muons from decay of pions under a solenoi- dal magnetic field. Stopping Target Production TargetAfter the MECO Cancellation
beam bunching
22 batches = 1. 467s MI cycle Booster Batches Accumulator Recycler Debuncher 4.6×1012 p/batch 4×4.6×1012 p/1467ms = 12.5 ×1012 p/sec 56 ×1012 p/sec 0.1s 1.367s NEUTRINO PROGRAM MUONS (NuMI +Muons) (NuMI) (Muons) (Alternative: 24 batches=1.6s MI cycle→ 11.5 ×1012 p/s) AP4 Line AP5 Line A-D LineCOMET
PRISM/Phase-1 Overview
Pulsed Proton Beam
J-PARC
144π mm.mrad
@ 30 GeV
adiabatic dumping
空バケツの作り方
RFチョッパーダンプのビームによる熱負荷 Empty Bucket へのRFチョッパーによる漏れ込みEmittance Control
ertical: Reduce RCS painting area
Tomizawa Scheme
Detector
Cosmic Ray V eto
Detector Acceptance & Signal Sensitivity
Acceptance Geometrical Acc. 0.73 Electron T ransport 0.44 pt > 52 MeV/c 0.67 χ2 Cut (χ2 < 9) 0.86 Energy Selection 0.56 Timing cut 0.38 Total 0.04 100 ns 700 ns 1.17 µs Timing Window of Detection Proton Intensity 4 × 1013 Hz ← Running Time 4 × 107 sec 2 × 107 sec μ’s yields per proton 0.0024 0.007* μ-stopping efficiency 0.29 0.26 Total 1.1 × 1018 stopped μ’s 1.5 × 1018B(µ− + Al → e− + Al) = 1 Nµ · fcap · Ae
< 10-16 (90% C.L.)
*Tungsten Target + Beamline UpdateBackground
Background estimates for 10-16 *: assuming the extinction 10-9
Curved Solenoid Spectrometer
Straw-man’s Layouts
J-PARC NP-Hall
Full PRISM at NP-Hall
Fast Extraction (to NP-Hall) Scheme exist
まとめ
やμ→eeeと共に注目されている。
最後に
End of Slides
Straw-man’s Cost Estimate
Muon Yield
0.002 0.004 0.006 100 125 150 175 200 225 250 275 300 325 0.02 0.04 0.06 0.08 0.1 x 100.002 μ’s/proton
Curved Solenoid Spectrometer
Muon momentum dist.
μ-e Conv. Next Generation
Curved Solenoid Spectrometer
T ransmission efficiency
60-MeV/c DIO electrons
D[m] = 1 0.3 × B[T] × s R × p2 l + 1 2p2 t pl105-MeV/c μ-e electron
V ertical Drift
もっと見栄えの良い絵がほしいところ。 前ページとコンバインもしたい。
Flavor Mixing
s W − u Vus VKM = Vud Vus Vub Vcd Vcs Vcb Vtd Vts Vtb = 0.97383+0.00024 −0.00023 0.2272+0.0010 −0.0010 (3.96+0.09 −0.09) × 10−3 0.2271+0.0010 −0.0010 0.97296+0.00024 −0.00024 (42.21+0.10 −0.80) × 10−3 (8.14+0.32 −0.64) × 10−3 (41.61+0.12 −0.78) × 10−3 0.999100+0.000034 −0.000004 sin2(2θ23) > 0.90 tan2(θ12) = 0.45+0.09
−0.07