1 / 60

Measurements and Experiments in Muon Physics

This program focuses on various experiments and measurements related to muon physics, including muon lifetime, fundamental constants, QCD symmetries, and electro-weak couplings. It covers experiments such as MuLan, MuCap, and MuSun, and explores topics such as calibration of the Sun and muon capture on different targets. The program includes theoretical calculations and experimental results to enhance our understanding of the properties and interactions of muons.

delvecchio
Télécharger la présentation

Measurements and Experiments in Muon Physics

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Muon Lifetime Programme at PSI Fundamental Constants MuLan FAST Peter Kammel Basic QCD Symmetries “Calibrating the Sun” MuSun MuCap

  2. MuLan Muon Lifetime • Fundamental electro-weak couplings • GF • Implicit to all EW precision physics • Uniquely defined by muon decay GFaMZ 9 ppm 0.0004 ppm 23 ppm q QED

  3. MuLan Dramatic Progress in QED Calc. • Extraction of GF from tm not theory limited total MuLan2004 theory 17 ppm 18 ppm 90 ppb 30 ppm 9 ppm 18 ppm <0.3 ppm 0.5 ppm 1 ppm <0.3 ppm van Ritbergen and Stuart: 2-loop QED corrections MuLan Goal ExperimentsRAL, PSI dnm from dm2 Pak & Czarnecki (2008) -0.43 ppm reduction of tmdue to finite me effect

  4. MuLan MuLan Experiment Real data Kicker On PSI DC proton beam590 MeV, 1.7 mA ~ 10 MHz m+ Measurement Period Number (log scale) time Fill Period -12.5 kV 12.5 kV

  5. MuLan MuLan detector has 30 active “houses”, with 170 tile pairs e+ 80 pe/mip

  6. MuLan Statistics & Systematics “Early-to-late” changes • Instrumental shifts Gain or threshold Time response Kicker and accidentals • Effective acceptance Residual polarization or precession • Pileup leads to missed events 2004 symmetric detector stray muons studied different targets

  7. FAST Experiment • Fast imaging target of 4x4x200 mm3 scintillators, PSPMs • Trigger: L1 selects p, L2 selects p → m→ e decay chain • Essentially many small decay detectors in parallel • Proof-of-principle measurement 16 ppm published 2008, 30 kHz L2 • One year run in 2008 to obtain 2 ppm t result (with improved L2)

  8. ±1 ppm  10 New World Situation GF = 1.166367(5) x 10-5 GeV-2(4.1 ppm)

  9. MuCap Muon Capture on the Proton • Historical: V-A and m-e Universality • Today: EW current key probe for Understanding hadrons from fundamental QCD Symmetries of Standard Model Basic astrophysics reactions -+ p  m+ n charged current Lattice CalculationsChiral Effective Theories

  10. MuCap Formfactors and gP - + p  m+ n rateLSat q2= -0.88 mm2 • Muon Capture • Formfactors + second class currentssuppressed by isospin symm. Lorentz, T invariance All form factors precisely known fromSM symmetries and data. CVC, n beta decay apart from gP = 8.3 ± 50%

  11. MuCap Pseudoscalar Form Factor gP gP determined by chiral symmetry of QCD: gP = (8.74  0.23) – (0.48  0.02) = 8.26  0.23 ChPT leading order one loop two-loop <1% • gP basic and experimentally least known nucleon form factor • solid QCD prediction (2-3% level) • basic test of QCD symmetries T. Gorringe, H. Fearing, Rev. Mod. Physics 76 (2004) 31V. Bernard et al., Nucl. Part. Phys. 28 (2002), R1

  12. 1 % LH2 100% LH2 pm ppμ ppmO ppμ pm ppmO ppmP ppmP time (ms) But m- is a heavy electron ! LT= 12 s-1 triplet (F=1) pμ↑↑ Lortho=506s-1 Lpara=200s-1 λop μ ppμ ppμ f λppm ortho (J=1) para (J=0) pμ↑↓ • Interpretation requires knowledge of ppm population • Strong dependence on hydrogen density f singlet (F=0) LS= 710s-1 n+n MuCap

  13. Precise Theory vs. Controversial Experiments gP - + p  m+ n @ Saclay - + p  m+ n + g@TRIUMF ChPT mCapprecisiongoal TRIUMF 2006 exp theory lOP(ms-1) • no overlap theory & OMC & RMC • large uncertainty in lOP gP  50% ? MuCap

  14. MuCap MuCap Experimental Strategy • Lifetime method • 1010m→enn decays • measure - to 10ppm, • S = 1/- - 1/+to 1% • Unambiguous interpretation at low target density • Clean m stop definition in active target (TPC) • Ultra-pure gas system and purity monitoring at 10 ppb level • Isotopically pure “protium” m → enn LSreduces lifetime by 10-3 + log(counts) - μ+ μ – te-tm fulfill all requirements simultaneouslyunique MuCap capabilities

  15. MuCap MuCap Detector

  16. MuCap m- Muons stop in active TPC target 10 bar ultra-pure hydrogen, 1.16% LH2 2.0 kV/cm drift field ~5.4 kV on 3.5 mm anode half gap bakeable glass/ceramic materials Observed muon stopping distribution E p e- 3D tracking w/o material in fiducial volume

  17. Results cN, cO < 5 ppb, cH2O~ 8-30 ppb correction based on observed capture yield x t z Imp. Capture MuCap Unique Capabilities: Impurities rare impurity capture mZ(Z-1)+n+n LZ (C, N, O) ~ (40-100) x LS ~10 ppb purity required Hardware Circulating Hydrogen Ultrahigh Purification System(CHUPS) Gas chromatographyCRDF 2002, 2005 CHUPS Diagnostic in TPC

  18. MuCap gP Landscape after MuCap 07 SMuCap = 725.0  13.7stat 10.7sys s-1 Czarnecki, Marciano,Sirlin , PRL 99 (2007) MuCap, PRL 99, 032001 (2007) - + p  m + n + g gP = 7.3 ± 1.1

  19. Muon Capture on the DeuteronThe MuSun Experiment

  20. Motivation • m- + d  n + n + nRateLd from md() atom • MeasureLdto < 1.5 % • Simplest weak interaction process in a nucleusallowing for precise theory & experiment • Close relation to neutrino/astrophysics • Broader Impact on modern nuclear physics • EFT relates m+d to strong processes like p+d  g + n +n, ann

  21. m + d  n + n + nTheory • Axial current reaction • Gamow-Teller 3S1 1S0 • one-body currents well defined • two-body currents not well constrained by theory (short distance physics) • Methods • Potential model + MEC • hybrid EFT • Effective field theories model independent D p MEC EFT  L1A, dR Low Energy Constants

  22. Connection to Neutrino/Astrophysics • Basic solar fusion reaction • p + p  d + e+ +  • Key reactions for Sudbury Neutrino Observatory • e + d  p + p + e- (CC) • x + d  p + n + x (NC) • Intense theoretical studies, scarce direct data • EFT connection to m+d capture via LEC L1A, • Muon capture soft enough to relate to solar reactions with L1A ~ 6 fm3

  23. Precise Experiment Needed consistent ChPT pionless, needs L1A hybrid EFT Potential Model + MEC

  24. Muon Kinetics Collisional processes density f dependent, e.g. hfs transition rate from q to d state = flqd densityf normalized to LH2 density Muon-catalyzed Fusion lq lqd ld md() md md() m3He complicated, can one extract fundamental weak parameters ?

  25. Cryo-TPC Design

  26. Observables • Observables in MuSun experiment • decay electrons main observable • fusion and capture essential as kinetics and background monitors Experience from MCF experiments mN capture 1.8 1010 109 5 105

  27. Statistics + Systematics 1.81010 events Experiment approved PAC 2008

  28. Summary and Outlook • MuLan: • First GF update in 23 years – 2.5x improvement, no surprise in result • Factor 10 additional improvement on the way • MuCap: • First precise gP with clear interpretation • Consistent with ChPT expectation, clarifies long-standing puzzle • Factor 3 additional improvement on the way • MuSun • Muon-deuteron capture with 10x higher precision • Calibrates basic astrophysics reactions and provides new benchmark in axial 2N reactions

  29. Part of MuLan http://www.npl.uiuc.edu/exp/mucapture/ http://www.npl.uiuc.edu/exp/mulan/ http://www.npl.uiuc.edu/exp/musun/ Part of MuCap http://fast.home.cern.ch/fast/

  30. Quest for L1A, dR “Calibrate the Sun” • Precision m+d experiment • by far the best determination • of L1A in the theoretically clean • 2-N system

  31. Bahcall & Pena-Garay 2004 • v fluxes from experiments + Luminosity constraint • Relevance of 7Be exp. • Relevance of pp experiment • SSM correct at 1%, n/g Luminosity(steady state, other energy generation?) • MSW-vacuum transition • Improvement q12

  32. Impact for Solarand n Physics • SNO assumes 1.1% uncertainty in s(n+d)but Truhlik, Vogel et al. estimate 2-3% model dependence • SSM assumes 0.4% uncertainty in pp S-factor • Impact for both solar and n physics should be updatede.g. SNO III: Df(CC) from 6.3% to 4.0% • m+d capture: calibration of fundamental reactions based on first principles completely rests on hybrid EFT & 3-N A. B. Balantekin and H. Yuksel

  33. Experimental Strategy • Two main conditions • Unambiguous physics interpretation • Muon kinetics  optimization of D2 conditions • Very high precision Ld to 1.2% (5 s-1) • Statistics: several 1010 events • Systematics !

  34. Comments on Systematic Errors

  35. QCD • High q2 (q > some GeV) short distance <0.1 fm • Weakly interacting quarks and gluons asymptotic freedom • Low q2 (q << 1GeV) long distance > 1 fm • QCD has chiral symmetry spontaneously brokenp is Nambu-Goldstone boson, weakly interacting chiral effective theory ↔ Nuclear Physics • Lattice QCD: ab initio calculations • issues: continuum transition, etc. • physical quark masses not reached Edwards et al. LHPC Coll (2006) MuCap

  36. Constraining Short Distance Nuclear Physics • ga axial current coupling to single-nucleon system • axial current coupling to two-nucleon system • Connection to N-p physics analogous to Goldberger-Treiman relation 1N sector • Applications • contribution to chiral 3N force from term • determination reduces ann uncertainty from theory • p + d → n + n + g ann= 18.90 ± 0.27(exp) ± 0.30(th) fm • future <0.05

  37. Experiment Overview e eSC ePC2 ePC1 mPC Cryo-TPC m mSC

  38. m + d Experiment m   d • Experimental Challenges • Dalitz Plot • Intensity at low Enn • ChPT covers most of DP • pEFT only pn< 90 MeV/c m → enn lm= 455162 s-1 mdq,d → n+n+nLq ~ 10 s-1, Ld = 400 s-1md() + d→ md() + dddm→ 3He + n + mrates ~ lm

  39. Cryo-TPC Design Criteria

  40. Technical Design Cryo-System Vibration free cooling Continuous cleaning

  41. Gas Purity (Z-1)* + n • CirculatingHydrogenUltrahighPurificationSystem(CHUPS) • US CRDF 2002, 2005 • New: • cryo-TPC • cryo filter before TPC • continuous getter in gas flow for gas chromatography • Particle detection in TPC • much harder – fusionfor MuSun – m signal 1 MeV • excellent TPC resolution • full analog readout • tags – p after capture • – X-ray • protium measurement Rare impurity capture:md + Z d + mZ  (Z-1)* + n MuCap achieved: ~ 10 ppb purity and 0.1 ppb purity monitoring MuSun needs: ~ 1 ppb purity or 0.5 ppb purity monitoring

  42. Impurity detection • Capture recoil 300-500 keV • f (MuSun) = 5 f (MuCap) • Separate mN signal with • Excellent energy resolution(30keV) • Additional tag • TPC signal topology • Coincident X-ray, neutron mN capture, cN = 41 ppb p

  43. Muon Capture, Big Picture { gP, gA, ChPT } m + p m + d m + 3He { gP, gA, ChPT, L1A, ann } { gP, gA, hybrid EFT, L1A, 3N} Final MuCap 2-3x improvement Combinedanalysis

  44. Solar • Sun Facts • Solar radius = 695,990 km = 109 Earth radii • Solar mass = 1.989 1030 kg = 333,000 Earth masses • Solar luminosity (energy output of the Sun) = 3.846 1033 erg/s • Surface temperature = 5770 K = 9,930º F • Surface density = 2.07 10-7 g/cm3 = 1.6 10-4 Air density • Surface composition = 70% H, 28% He, 2% (C, N, O, ...) by mass • Central temperature = 15,600,000 K = 28,000,000º F • Central density = 150 g/cm3 = 8 × Gold density • Central composition = 35% H, 63% He, 2% (C, N, O, ...) by mass • Solar age = 4.57 109 yr  

  45. pp cycle

  46. Solar n updates • Borexino 2008 • Kamland 2008

  47. CHUPS cN, cO < 5 ppb, cH2O~ 8-30 ppb correction based on observed capture yield

  48. MuCap Results + from PDG and MuLan SMuCap = 725.0  13.7stat 10.7sys s-1 further sub percent theory required Average of HBChPT calculations of S: Apply new rad. correction (2.8%): gP = 7.3 ± 1.1 (MuCap 2007)

  49. MuSun Solar Fusion and Neutrinos • Basic solar fusion reaction • p + p  d + e+ +  1.4x1010 yrs • d + p  3He + g 6 s • 3He + 3He  4He + 2p 106 yrs • Key reactions for Sudbury Neutrino Observatory • e + d  p + p + e- (CC) •  + d  p + n +  (NC) Solar neutrino problem solved by neutrino oscillation Intense theoretical studies, Very limited direct experimental info

More Related