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Klaus P. Jungmann, Kernfysisch Versneller Instituut, Groningen, NL Arbeitstreffen „Hadronen und Kerne“, Pommersfelden, 26 September 2001 Standard Model Precision Experiment Fundamental Constants Related Experiments Interpretation Future Possibilities
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QED - Contributions: Weak Interaction Corrections: a (QED) = 116 584 705.6(2.9) * 10 -11 (Kinoshita 2000) a (weak) = 151(4) * 10 -11 (Kutho 1992, Degrassi 1998)
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QED - Contributions: Weak Interaction Corrections: a (QED) = 116 584 705.6(2.9) * 10 -11 (Kinoshita 2000) a (weak) = 151(4) * 10 -11 (Kutho 1992, Degrassi 1998)
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minor error in calculations
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The new measurement of the muon magnetic anomaly at the Brookhaven National Laboratory aims for 0.35 ppm relative accuracy. Why? We have in the listing of fundamental physical constants: electron magnetic anomaly 1.159 652 186 9(41) 10 -3 (0.0035 ppm) muon magnetic anomaly 1.165 916 02(64) x 10 -3 (0.55 ppm) Sensitivity to heavier objects larger by (m /m e ) 2 40 000
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Hadronic Corrections for g -2 a hadr.,1 st order) = 6951(75) 10 -11 (Davier, 1998) a hadr., higher order) = -101(6) 10 -11 (Krause, 1996) a hadr., light on light) = -79(15) 10 -11 (Hayakawa, 1998) !! Situation Spring 2001
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Early “Shopping List”
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The fixed probes 4 ppm Proton NMR
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Electronics inside the trolley The NMR-Trolley 17 probes - Proton NMR in water
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Electrostatic Quadrupole Electrodes NMR Trolley Rails Fixed NMR Probes Trolley NMR Probes Vacuum Vessel
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900 000 000 positrons with E > 2GeV in 1999
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Systematic Uncertainties, Results Magnetic Field p,0 spherical probe 0.05 ppm p (R,t i ) 17 trolley probes 0.22 ppm p (R,t) 150 fixed probes 0.15 ppm p (R) aging - p (R I ) inflector fringe field 0.20 ppm < p muon distribution 0.12 ppm total systematic uncertainty p =0.4 ppm Spin Precession Pileup 0.13 ppm AGS background 0.10 ppm Lost muons 0.10 ppm Timing Shifts 0.10 ppm E field and vertical CBO 0.08 ppm Binning and Fitting procedure 0.07 ppm Coherent Betatron Oscillations 0.05 ppm beam debunching 0.04 ppm Gain Instability 0.02 ppm total systematic uncertainty a,sy = 0.25 ppm total statistical uncertainty a,st = 1.25 ppm p /2 = 61 791 256 (25) Hz a /2 = 229 072.8 (0.3) Hz
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QED mm g-2 hadronic contribution weak contribution New Physics + e - HFS, n=1 QED corrections weak contribution + e - 1S-2S m QED corrections QED mm , , g h
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a = a m ca m c e B = aa pp aa pp pp - Experiment: Theory: * need for muon ! * hadronic and weak corrections * various experimental sources of better 100ppb> need constants at very moderate * no concern for (g-2) accuracy * a and B ( p ) measured in (g-2) experiment * c is a defined quantity * m ( ) is measured in muonium spectroscopy (hfs) NEW 1999 * e is measured in muonium spectroscopy (1s -2s) NEW 1999 * p in water known >> probe shape dependence * 3He to p in water >> gas has no shape effect being improved
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Muonium Hyperfine Structure Solenoid e in SS Detector MW-Resonator Yale - Heidelberg - Los Alamos exp = 4 463 302 765(53) Hz ( 12 ppb) theo = 4 463 302 649(520)(34)(<100) Hz(<120 ppb) p = 3.183 345 13(39) (120 ppb) m m e = 206.768 273(24) (120 ppb) = 137.036 010 8(5 2) ( 39 ppb) W. Liu et al. Phys. Rev. Lett. 82, 711 (1999)
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Muonium 1S-2S Experiment Laser Diagnostics Detection -.25 R 1S 2S 244 nm Energy -R 0 e kin in ee Target Mirror Heidelberg - Oxford - Rutherford - Sussex - Siberia - Yale 1s-2s = 2455 528 941.0(9.1)(3.7) MHz 1s-2s = 2455 528 935.4(1.4) MHz m = 206.768 38 (17) m e q = [ -1 -1.1 (2.1) 10 -9 ] q e- exp theo V.Meyer et al., Phys.Rev.Lett. 84, 1136 (2000)
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2.6 deviation
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Possible Explanations for a a (exp) and a (latest theory) differ by 42(16) *10 -10 The probability for agreement is < 1% Statistical Fluctuation Undiscovered Error in Experiment (not recognized systematics) Not yet complete standard theory calculation (hadronic contribution) New Physics 4 times more data on tape & data for - being taken
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Courtesy of W. Kluge, Karlsruhe (Summer 2001) About 1 year’s data needed
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Hadronic Corrections for g -2 a hadr.,1 st order) = 6951(75) 10 -11 (Davier, 1998) a hadr., higher order) = -101(6) 10 -11 (Krause, 1996) a hadr., light on light) = -79(15) 10 -11 (Hayakawa, 1998) !! ??SIGN ??
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Muon Magnetic Anomaly in Super Symmetric Models approximate rule : a SUSY 1.4 [ (100 GeV/c 2 ) /m g ] 2 tan goal BNL 821: a to 0.4 after: U. Chattopadyay and P. Nath, 1995 A t, m 0 vary over parameter space m 0 < 1TeV/c 2 no constraints from dark matter constraint through dark matter w w k ~ k k ~
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Note: Even if there will be a difference between muon g-2 and theory established and unquestioned, it does not carry a tag about the nature of the difference! We will need further experiments then to learn more! Such as: - searches for rare muon decays - search for a muon edm -..............................
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e appears in composite models if a as suggested
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Concept works also for (certain) nuclei; GSI could start right now Exploit huge motional electric fields for relativistic particles in high magnetic fields; observe spin rotation EDM closely related to non standard anomaly in many models!
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CERN Neutrino Factory baseline scenario (target muon budget) 4 MW 2.2ms/13.3ms 3.3 s (144b of 3ns) 10 16 p/s 1.210 14 s =1.2 10 21 yr 0.9 10 21 yr 3 10 20 e yr 3 10 20 yr 3 10 20 e yr 3 10 20 yr 10 20 e yr 10 20 yr (© A. Blondel) Similar Bright Possibilities at almost any High Power Proton Facility, e.g. - ESS - GSI (?) - JHF Don’t Mi(e)ss It! Future Possibilities
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SPARES
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Neutrino Factory @ CERN Possibly Interesting experiments High Intensity Low Energy Muon Experiments (targets!) rare decays e + e e + e e + > Lepton number muonium - antimuonium conversion > Lepton number “normal” muon decay > G F muon magnetic anomaly > g-2, a muon edm > d muon parameters > m , , muonic atoms > r p, g p CF Next Generation ISOLDE Experiments radioactive muonic atoms > r n, r p nuclear structure of short lived nucleids > r n, r p nuclear structure far off valley of stability > r n, r p muon capture Neutrino Experiments long baseline short baseline charm Production NC/CC > m w (10-20 MeV) and sin 2 q w eff (2.10 -4) Kaon Experiments ( >> 15 GeV postaccelerator ) K Jungmann 18-Apr-2001
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Muon Experiments Possible at a CERN Neutrino Factory - Expected Improvements K Jungmann 18-Apr-2001
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< < < < Muon Experiments possible at a CERN Neutrino Factory - Required Beam Parameters K Jungmann 18-Apr-2001
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