latest results on ρand δfrom muon decay · robert tribble – int, october, 2008 fitting the data...

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Robert Tribble – INT, October, 2008 Latest Results on ρ and δ from Muon Decay Robert E. Tribble Texas A&M University for the TWIST Collaboration

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Page 1: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Latest Results on ρ and δ from Muon Decay

Robert E. TribbleTexas A&M University

for the TWIST Collaboration

Page 2: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Muon decay spectrum

The energy and angle distributions of positrons following polarized muon decay obey the spectrum:

)1(3)34(32)33(

)(cos0

2

2

xxxxx

dxdxd

−+−+−∝Γ ηρ

θ

⎥⎦⎤

⎢⎣⎡ −+−+ )34(

32)1(cos xxP δθξμ

max,e

e

EEx =where

)1(3)34(32)33(

)(cos0

2

2

xxxxx

dxdxd

−+−+−∝Γ ηρ

θ

⎥⎦⎤

⎢⎣⎡ −+−+ )34(

32)1(cos xxP δθξμ

max,e

e

EEx =

)1(3)34(32)33(

)(cos0

2

2

xxxxx

dxdxd

−+−+−∝Γ ηρ

θ

⎥⎦⎤

⎢⎣⎡ −+−+ )34(

32)1(cos xxP δθξμ

[Radiative corrections not included]

Page 3: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Muon decay matrix element

• Most general local, derivative-free, lepton-number conserving muon decay matrix element:

• In the Standard Model, gVLL = 1, all others are zero

• Pre-TWIST global fit results (all 90% c.l.):

∑=

=

ΓΓ=

LRTVS

mneF egGM

,,,,

||)()(||2

4

μεγ

μγμγ

εγεμ μνν

Page 4: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Muon decay parameters and coupling constants

SM ρ = 0.7518 ± 0.0026 3/4 η = -0.007 ± 0.013 0Pμξ = 1.0027 ± 0.0079 ± 0.0030 1δ = 0.7486 ± 0.0026 ± 0.0028 3/4Pμ(ξδ/ρ) > 0.99682 (90% c.l.) 1

Prior to TWIST

Page 5: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Goal of TWIST• Search for new physics that can be revealed by order-

of-magnitude improvements in our knowledge of ρ, δ, and Pμξ

• Model-independent limit on muon handedness

• Left-right symmetric models

• …..

⎥⎦⎤

⎢⎣⎡ −+= ξδξμ

916

311

21

RQ

2

23

43 ζρ =−

⎟⎟

⎜⎜

⎛⎟⎟⎠

⎞⎜⎜⎝

⎛+⎟⎟

⎞⎜⎜⎝

⎛+=−

42241

R

L

R

L

MM

MMP ζζξμ

Two examples

Page 6: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

What is required?

Must:• Determine spectrum shape

-- All three parameters• Understand sources of muon depolarization

-- Pμ and ξ come as a product• Measure forward-backward asymmetry

-- For Pμξ and δto within a few parts in 104

[Radiative corrections to O(α2)]

Page 7: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Surface muon beam

TRIUMFM13 beam line

Page 8: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

TWIST spectrometer

Page 9: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Detector array• 56 low-mass high-precision planar chambers symmetrically placed around thin target foil (DME,CF4/Isobutane)

• Measurement initiated by single thin scintillation counter at entrance to detector

• Beam stop position controlled by variable He/CO2 gas degrader

Yu.Davydov et al. NIM A461(2001)68R.Henderson et al. NIM A548(2005)306

Page 10: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Typical events

• Use pattern recognition (in position and time) to sort hits into tracks, then fit to helix

• Must also recognize beam positrons, delta tracks, backscattering tracks

Page 11: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Physics data sets• Fall 2002

– Test data-taking procedures and develop analysis techniques– First physics results – ρ and δ– Graphite-coated Mylar target not suitable for Pμξ

• Fall 2004– Al target (70 μm) and Time Expansion Chamber enabled first Pμξ

measurement– Improved determinations of ρ and δ recently published

• 2006-07– Ag and Al target data– Larger data sets and better beam characterization– Achieve ultimate TWIST precision for ρ, δ, and Pμξ

Page 12: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Analysis method

• Extract energy and angle distributions for data:– Apply (unbiased) cuts on muon variables.– Reject fast decays and backgrounds.– Calibrate e+ energy to kinematic end point at 52.83 MeV.

• Fit to identically derived distributions from simulation:– GEANT3 geometry contains virtually all detector components.– Simulate chamber response in detail.– Realistic, measured beam profile and divergence.– Extra muon and beam positron contamination included.– Output in digitized format, identical to real data.

Page 13: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

2-d momentum-angle spectrum

Acceptance of the TWIST spectrometer

In angular fiducial

In momentum fiducial

Page 14: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Fitting the data distributions

• Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so a fit to first order expansion is exact.

• Fit data to simulated (MC) base distribution with hidden assumed parameters, λMC = (ρ,η,Pμξ|Pμξδ

,Pμξδ)plus MC-generated distributions from analytic derivatives, times fitting parameters (Δλ) representing deviations from base MC. (η is now fixed to global analysis value) (graphic thanks to Blair Jamieson)

λMC hiddenblind analysis

Page 15: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Validating the Monte Carlo with “upstream stops”

(DS-Fit)-(US-Fit)

μ stops

target

Page 16: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Normalized residuals[(Data-Fit)/sigma] of the 2-d momentum-angle fit

Fit describes the data well, even when extrapolated far outside the fiducial region

Angle-integrated results

Fitting the 2002 data to determine ρ and δ

Page 17: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

First TWIST results for ρ and δ

• From Fall, 2002 run:

– ρ = 0.75080 ± 0.00032 (stat) ± 0.00097 (syst) ± 0.00023 (η)J. Musser et al., PRL 94, 101805

– δ = 0.74964 ± 0.00066 (stat) ± 0.00112 (syst)A. Gaponenko et al., PRD 71, 071101

Page 18: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Systematics in the first measurements

The same effects tend to dominate the systematic uncertainties for both ρ and δ

Systematic uncertainties typically determined from data sets with a possible problem exaggerated or by MC done with an exaggerated ‘defect’ put into detector

Page 19: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Global Analysis

• Follow Fetscher, Gerber, Johnson formulation (Phys. Lett. 173B, 102 (1986))

∑=

=

ΓΓ=

LRTVS

mneF egGM

,,,,

||)()(||2

4

μεγ

μγμγ

εγεμ μνν

Use general form of interaction:

Page 20: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Global Analysis

Constraints:

Normalization:

Note that ≈ 1

(from Phys. Lett. 173B)

Page 21: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Global Analysis

Relation to muon decay observables:

e+L{

e+T {

rad. decay {

Page 22: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Global Analysis2005 Input:

2005 Output:

PRD 72, 073002

Page 23: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Reducing the leading systematics• Issues that were unique to 2002 data

– Stopping target thickness uncertainty– Chamber orientation uncertainty with respect to magnetic field

• Improvements in 2004 data– Chamber response

• Improved gas system regulation and monitoring• Improved determination of foil geometry• Improved treatment of drift chamber behavior

– Positron interactions better understood– Detector fully instrumented– Improved alignment techniques and understanding of uncertainties– New momentum calibration techniques (uncertainty is statistical)– Radiative corrections uncertainty evaluated

Page 24: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Systematic uncertainties for 2004 data: ρ and δ

6.711.34.69.2Total in quadrature

0.41.11.11.2Other

δ (×104)ρ (×104)Systematic uncertainties

1.0

2.9

6.1

5.5

3.7

5.6

2002

Theoretical radiative correction

Momentum calibration (ave)

Spectrometer alignment

Positron interactions

Stopping target thickness

Chamber response (ave)

2.0

2.0

2.2

4.6

4.9

5.1

2002

<0.1<0.1

4.12.9

0.30.3

0.91.6

<0.1<0.1

5.22.9

20042004

Page 25: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

set number31 32 33 34 35 36 37 38 39

0.004

0.005

0.006

0.007

0.008

0.009

0.01

/ ndf 2χ 9.025 / 6

Prob 0.1722

> δΔ< 0.0003036± 0.008715

/ ndf 2χ 9.025 / 6

Prob 0.1722

> δΔ< 0.0003036± 0.008715

vs setδΔ

set number31 32 33 34 35 36 37 38 39

-0.009

-0.0085

-0.008

-0.0075

-0.007 / ndf 2χ 3.143 / 6

Prob 0.7907> ρΔ< 0.0001714± -0.008284

/ ndf 2χ 3.143 / 6

Prob 0.7907> ρΔ< 0.0001714± -0.008284

vs setρΔ

Consistency Checks: ρ and δ

• Data sets for 2004 analysis• Δ’s from fits to MC• No corrections applied• Decay parameters in BB still hidden

Page 26: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Results to date• From Fall, 2002 run:

– ρ = 0.75080 ± 0.00032 (stat) ± 0.00097 (syst) ± 0.00023 (η)– δ = 0.74964 ± 0.00066 (stat) ± 0.00112 (syst)

• From Fall, 2004 run:– ρ = 0.75014 ± 0.00017 (stat) ± 0.00044 (syst) ± 0.00011 (η)

– δ = 0.74964 ± 0.00030 (stat) ± 0.00067 (syst)R. McDonald et al., PRD 78, 032010

Page 27: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Global Analysis Results

<0.0024<0.0031<0.0051

2004 Data2002 DataPre-TWIST

<0.025<0.036<0.066|gVLR|

<0.021

<0.074

|gTLR|

|gSLR|

<0.036

<0.125

<0.025

<0.088

90% confidence limits

μRQ

Page 28: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

Final Uncertainty Goals

Final (est.)Published

2.3

1.3Statistics

δ

ρ

3.0

1.7Statistics

3.26.7

2.44.4SystematicsSystematics

Final Publications in 2009

all values in units of 10-4

Page 29: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

TWIST Collaboration

Page 30: Latest Results on ρand δfrom Muon Decay · Robert Tribble – INT, October, 2008 Fitting the data distributions • Decay distribution is linear in ρ, η, Pμξ, and Pμξδ, so

Robert Tribble – INT, October, 2008

TWIST ParticipantsTRIUMF

Ryan Bayes *†Yuri DavydovJaap DoornbosWayne FaszerMakoto FujiwaraDavid GillAlex GrossheimPeter GumplingerAnthony Hillairet *†Robert HendersonJingliang HuJohn A. Macdonald ‡Glen MarshallDick MischkeMina NozarKonstantin OlchanskiArt Olin yRobert OpenshawTracy Porcelli §Jean-Michel PoutissouRenée PoutissouGrant ShefferBill Shin §§

AlbertaAndrei Gaponenko **Peter KitchingRobert MacDonald **Maher QuraanyNate Rodning ‡John SchaapmanGlen Stinson

British ColumbiaJames Bueno *Mike HasinoffBlair Jamieson **

MontréalPierre Depommier

ReginaTed MathieRoman Tacik

Kurchatov InstituteVladimir SelivanovVladimir Torokhov

Texas A&MCarl GagliardiJim Musser **Bob Tribble Maxim Vasiliev

ValparaisoDon KoetkePaul NordShirvel Stanislaus

* Graduate student** Graduated† also U Vic§ also Manitoba§§ also Saskatchewan‡ deceased

Supported under grants from NSERC (Canada) and DOE (USA).Computing facilities of WestGrid are gratefully acknowledged.