A PART-PER-MILLION MEASUREMENT OF THE POSITIVE MUON LIFETIME AND DETERMINATION OF THE FERMI CONSTANT David M Webber University of Illinois at Urbana-Champaign (Now University of Wisconsin-Madison) December 9, 2010 Outline • Motivation • Experiment Hardware • Analysis – Pulse Fitting – Fit Results • Systematic Uncertainties – Gain Stability – Pileup – Spin Rotation • Final Results D. M. Webber 2 Motivation • m gives the Fermi Constant to unprecedented precision (actually Gm) • m needed for “reference” lifetime for precision muon capture experiments – MuCap – MuSun Capture rate from lifetime difference m- and m The predictive power of the Standard Model depends on well-measured input parameters What are the fundamental electroweak parameters (need 3)? a GF MZ sin2qw MW 0.00068 ppm 8.6 ppm 23 ppm 650 ppm 360 ppm * circa 2000 Obtained from muon lifetime Other input parameters include fermion masses, and mixing matrix elements: CKM – quark mixing PMNS – neutrino mixing The Fermi constant is related to the electroweak gauge coupling g by Contains all weak interaction loop corrections In the Fermi theory, muon decay is a contact interaction where Dq includes phase space, QED, hadronic and radiative corrections Dq In 1999, van Ritbergen and Stuart completed full 2-loop QED corrections reducing the uncertainty in GF from theory to < 0.3 ppm (it was the dominant error before) D. M. Webber 5 The push – pull of experiment and theory • Lifetime now largest uncertainty leads to 2 new experiments launched: MuLan & FAST – Both @ PSI, but very different techniques – Both aim at “ppm” level GF determinations – Both published intermediate results on small data samples Meanwhile, more theory updates !! The lifetime difference between m and m- in hydrogen leads to the singlet capture rate LS m- p n m D m - m - 0.16% log(counts) 1.0 ppm MuLan ~10 ppm MuCap MuCap nearly complete μ– μ+ time The singlet capture rate is used to determine gP and compare with theory L S L m - - L m ( m - ) -1 - ( m ) -1 gP Experiment D. M. Webber 10 For 1ppm, need more than 1 trillion (1012) muons ... πE3 Beamline, Paul Scherrer Institut, Villigen, Switzerland The beamline transports ~107 “surface” muons per second to the experimental area. Parallel beam Spatial focus Momentum Selection Dp p 2% Velocity separator removes beam positrons A kicker is used to create the time structure. counts arb. 5 ms Trigger Suppression Accumulation Period 22 ms Extinction ~ 1000 Measuring Period kicker ARNOKROME™ III (AK-3) high-field target used in 2006 - Rapid precession of muon spin - mSR studies show fast damping The target was opened once per day to view the beam profile. Target rotates out of beam D. M. Webber 15 In 2006, The ferromagnetic target dephases the muons during accumulation. •Arnokrome-3 (AK3) Target (~28% chromium, ~8% cobalt, ~64% iron) •0.5 T internal magnetic field •Muons arrive randomly during 5 ms accumulation period •Muons precess by 0 to 350 revolutions D. M. Webber 16 2007 target: crystal quartz, surrounded by an external ~ 135 G magnetic field Installed Halbach Array Quartz • 90% muonium formation – “Test” of lifetime in muonium vs. free – Rapid spin precession not observable by us • 10% “free” muons – Precession noticeable and small longitudinal polarization exists • Creates analysis challenges ! • Magnet ring “shadows” part of detector The experimental concept… Number (log scale) Real dataKicker On 450 MHz WaveForm Digitization (2006/07) Measurement Period time Fill Period MHTDC (2004) 170 Inner/Outer tile pairs The detector is composed of 20 hexagon and 10 pentagon sections, forming a truncated icosahedron. Each section contains either 6 or 5 tile elements a Each element is made from two independent scintillator tiles with light guides and photomultiplier tubes. 170 scintillator tile pairs readout using 450 MHz waveform digitizers. 2 Analog Pulses Waveform Digitizers x2 1 clock tick = 2.2 ns 1/6 of system Uncertainty on lifetime from gain stability: 0.25 ppm D. M. Webber 20 The clock was provided by an Agilent E4400B Signal Generator, which was stable during the run and found to be accurate to 0.025 ppm. Agilent E4400 Function Generator f = 451.0 450.87649126 +/- 0.2 MHz • Checked for consistency throughout the run. • Compared to Quartzlock A10-R rubidium frequency standard. • Compared to calibrated frequency counter • Different blinded frequencies in 2006 and 2007 Average difference = 0.025 ppm MuLan collected two datasets, each containing 1012 muon decays Ferromagnetic Target, 2006 Quartz Target, 2007 • Two (very different) data sets – – – – Different blinded clock frequencies used Revealed only after all analyses of both data sets completed Most systematic errors are common Datasets agree to sub-ppm Analysis D. M. Webber 23 Raw waveforms are fit with templates to find pulse amplitudes and times >2 x 1012 pulses in 2006 data set >65 TBytes raw data inner A difficult fit Normal Pulse ADT Template outer Two pulses close together D. M. Webber 25 Nearby pulses perturb the time of main pulses. Studied with simulations Fixed reference perturbation Dtavg Dtavg Estimated pull: (0.03 ct ) (0.25% pileup ) 0.075 ppm (1000 ct / m ) D. M. Webber 26 2006: Fit of 30,000 AK-3 pileup-corrected runs. ppm m + Dsecret 22 ms Relative (ppm) R vs fit start time Red band is the set-subset allowed variance 0 9 ms 2007: Quartz data fits well as a simple sum, exploiting the symmetry of the detector. The mSR remnants vanish. Systematics Introduction D. M. Webber 29 Leading systematic considerations: Systematics: Gain Stability D. M. Webber 31 Gain is photomultiplier tube type dependent Artifact from start signal Deviation at t=0 1 ADC = 0.004 V Sag in tube response 0 10 D. M. Webber 20 ms 32 Gain variation vs. time is derived from the stability of the peak (MPV) of the fit to pulse distribution If MPV moves, implies greater or fewer hits will be over threshold δN 3.0 10 - 4 N 0 10 20 ms Carefully studied over the summer. Gain correction is 0.5 ppm shift with 0.25 ppm uncertainty. 33 Systematics: Pileup D. M. Webber 34 Leading order pileup to a ~5x10-4 effect Fill i •Statistically reconstruct pileup time distribution •Fit corrected distribution Fill i+1 Measured vs. Deadtime Normal Time Distribution Pileup Time Distribution Raw Spectrum Pileup Corrected Introducing higher-order pileup A B C D E hit Inner tile Artificial deadtime F G triple pileup Artificial deadtime time Outer tile Artificial deadtime D. M. Webber 36 Pileup to sub-ppm requires higher-order terms • 12 ns deadtime, pileup has a 5 x 10-4 probability at our rates • Proof of procedure validated with detailed Monte Carlo simulation – Left uncorrected, lifetime wrong by 100’s of ppm Pileup terms at different orders … R (ppm) 1 ppm 150 ns deadtime range Artificial Deadtime (ct) The pileup corrections were tested with Monte-Carlo. Monte-Carlo Simulation, 1012 events agrees with truth to < 0.2 ppm 1.19 ppm statistical uncertainty D. M. Webber 38 Lifetime vs. artificially imposed deadtime window is an important diagnostic • A slope exists due to a pileup undercorrection 1 ppm 150 ns deadtime range Extrapolation to 0 deadtime is correct answer D. Correction M. Webber Pileup Uncertainty: 0.2 ppm 39 Explanations of R vs. ADT slope • Gain stability vs. Dt? – No. Included in gain stability systematic uncertainty. • Missed correction? – Possibly – Extrapolation to ADT=0 valid • Beam fluctuations? – Likely – Fluctuations at 4% level in ion source exist – Extrapolation to ADT=0 valid D. M. Webber 40 Systematics Spin Precession D. M. Webber 41 The decay positron energy and angular distributions are not uniform, resulting in position dependant measurement rates. Highest Energy Energy Positrons Positrons Lowest Ee = Emax = 52.83 MeV Positron energy distribution •• Lowest Highest energy energy positron positronwhen when neutrinos neutrinosare are antiparallel. Ee = 13.2 MeV Ee = 26.4 MeV x Detection threshold Ee Emax parallel. • Neutrino helicities cancel angular momentum. • Neutrino helicities add so that they have angular • Positron spin must be in the same direction as muon momentum of 2. spin. q • Positron spin must compensate to bring total to 1. • Chiral limit dictates right handed positrons. • Chiral suppression (not well justified at this energy) •makes Most probable positron direction is same as muon positron most likely right handed. e+ spin • Most probable positron direction is opposite muon spin mSR rotation results in an oscillation of the measurement probability for a given detector. eB gm 2 m c m g 2 B m m B = 34 G This oscillation is easily detected counts arb. counts arb. N (t ) N 0exp - t / 1 a Pcos t B=1G This oscillation is not easily detected and systematic errors may arise counts arb. The sum cancels muSR effects; the difference accentuates the effect. B counts arb. counts arb. Sum m Difference/Sum 2006 target: AK3 ferromagnetic alloy with high internal magnetic field •Arnokrome-3 (AK3) Target (~28% chromium, ~8% cobalt, ~64% iron) •0.4 T transverse field rotates muons with 18 ns period •Muons arrive randomly during 5 ms accumulation period Ensemble Averge Polarization •Muons precess by 0 to 350 revolutions DEPHASED small ensemble avg. polarization A small asymmetry exists front / back owing to residual longitudinal polarization 85 Opposite Pairs All 170 Detectors pairs summed OppositeLifetime m When front / back opposite tile pairs are added first, there is no distortion Front “front-back folded”Back 2007 target: crystal quartz, surrounded by an external ~ 135 G magnetic field Installed Halbach Array Quartz • 90% muonium formation – “Test” of lifetime in muonium vs. free – Rapid spin precession not observable by us • 10% “free” muons – Precession noticeable and small longitudinal polarization exists • Creates analysis challenges ! • Magnet ring “shadows” part of detector We directly confront the mSR. Fit each detector for an “effective lifetime.” Would be correct, except for remnant longitudinal polarization relaxation. Difference between Top of Ball and Bottom of Ball to Sum, vs time-in-fill Illustration of free muon precession in top/bottom detector differences Longitudinal polarization distorts result in predictable manner depending on location. The ensemble of lifetimes is fit to obtain the actual lifetime. (Method robust in MC studies) Relative effective lifetime (ppm) (+ blind offset) Magnet-right data 2007: Consistency against MANY special runs, where we varied target, magnet, ball position, etc. Start-time scan Consistency Checks D. M. Webber 53 2006: Fit of 30,000 AK-3 pileup-corrected runs ppm m + Dsecret 22 ms Relative (ppm) R vs fit start time Red band is the set-subset allowed variance 0 9 ms 2006: AK-3 target consistent fits of individual detectors, but opposite pairs – summed – is better Difference of Individual lifetimes to average All 170 Detectors 85 Opposite Pairs 2007: Quartz data fits well as a simple sum, exploiting the symmetry of the detector. The mSR remnants vanish Variations in m vs. fit start time are within allowed statisical deviations D. M. Webber 57 Conclusions D. M. Webber 58 Final Errors and Numbers ppm units Effect Kicker extinction stability Residual polarization Upstream muon stops Overall gain stability: Short time; after a pulse Long time; during full fill Electronic ped fluctuation Unseen small pulses Timing stability Pileup correction Clock stability Total Systematic Total Statistical 2006 0.20 0.10 2007 0.07 0.20 0.10 0.25 0.12 0.20 0.03 0.42 1.14 0.42 1.68 (R06) = 2 196 979.9 ± 2.5 ± 0.9 ps (R07) = 2 196 981.2 ± 3.7 ± 0.9 ps (Combined) = 2 196 980.3 ± 2.2 ps (1.0 ppm) D(R07 – R06) = 1.3 ps Comment Voltage measurements of plates Long relax; quartz spin cancelation Upper limit from measurements MPV vs time in fill; includes: MPVs in next fill & laser studies Different by PMT type Bench-test supported Uncorrected pileup effect gain Laser with external reference ctr. Extrapolation to zero ADT Calibration and measurement Highly correlated for 2006/2007 GF & m precision has improved by ~4 orders of magnitude over 60 years. Achieved! Lifetime “history” FAST The most precise particle or nuclear or (we believe) atomic lifetime ever measured New GF GF(MuLan) = 1.166 378 8(7) x 10-5 GeV-2 (0.6 ppm) The lifetime difference between m and m- in hydrogen leads to the singlet capture rate LS m- p n m D m - m - 0.16% log(counts) 1.0 ppm MuLan ~10 ppm MuCap MuCap nearly complete μ– μ+ time The singlet capture rate is used to determine gP and compare with theory L S L m - - L m ( m - ) -1 - ( m ) -1 gP In hydrogen: 1/m-)-(1/m+) = LS gP now in even better agreement with ChPT* Using previous m world average Using new MuLan m average Shifts the MuCap result *Chiral Perturbation Theory 64 Conclusions • MuLan has finished – PRL accepted and in press. (see also arxiv:1010.0991) – 1.0 ppm final error achieved, as proposed • Most precise lifetime – Most precise Fermi constant – “Modest” check of muonium versus free muon • Influence on muon capture – Shift moves gP to better agreement with theory – “Eliminates” the error from the positive muon lifetime, needed in future MuCap and MuSun capture determinations (R06) = 2 196 979.9 ± 2.5 ± 0.9 ps (R07) = 2 196 981.2 ± 3.7 ± 0.9 ps (Combined) = 2 196 980.3 ± 2.2 ps (1.0 ppm) D(R07 – R06) = 1.3 ps MuLan Collaborators 2004 Institutions: University of Illinois at Urbana-Champaign University of California, Berkeley TRIUMF University of Kentucky Boston University James Madison University Groningen University Kentucky Wesleyan College 2006 2007 D. M. Webber 66 D. M. Webber 67 Backup Slides What is gP? gP is the pseudoscalar form factor of the proton D. M. Webber 69 Muon capture At a fundamental level, the leptonic and quark currents possess the simple V−A structure characteristic of the weak interaction. GFVud L 2 ν d μ u a (1- 5 )m d a (1- 5 )u D. M. Webber 70 Muon capture In reality, the QCD substructure of the nucleon complicates the weak interaction physics. These effects are encapsulated in the nucleonic charged current’s four “induced form factors”: ν n μ p n ( a ) gV (i a q ) g M ( a 5 ) g A (qa 5 ) g P p Return D. M. Webber 71 Miscellaneous D. M. Webber 72 The decay positron energy and angular distributions are not uniform, resulting in position dependant measurement rates. Highest Energy Energy Positrons Positrons Lowest Ee = Emax = 52.83 MeV Positron energy distribution •• Lowest Highest energy energy positron positron when when neutrinos neutrinos are are Ee = 13.2 MeV Ee = 26.4 MeV x Detection threshold Ee Emax anti-parallel. parallel. •• Neutrino so angular that theymomentum. have Neutrino helicities helicities add cancel angular momentum of 2. q • Positron spin must be in the same direction as •muon Positron spin.spin must compensate to bring total to 1. • Chiral limit dictates right handed positrons. e+ • Chiral suppression (not well justified at this •energy) Most probable positronmost direction same as makes positron likelyisright muon spin handed. Effect of h on GF • In the Standard Model, h=0, • General form of h • Drop second-order nonstandard couplings • Effect on GF return D. M. Webber 74