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Klaus P. Jungmann, Kernfysisch Versneller Instituut, Groningen, NL on behalf of the muon g-2 collaboration 3 rd Joint NIPNET ION-CATCHER HITRAP Collaboration Meeting: 2-6 June, 2004, Krakow, Poland Fundamental Laws Quantities Magnetic Moments Standard Model Precision Experiment Fundamental Constants Related Experiments Interpretation
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Vernon Hughes 1921-2003
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fundamental What means >> fundamental << ? Physicists in general: have always a tendency to put their own activities as fundamental renormalization of meaning Albert Einstein : God >> I would like to know how God has made the world. I am notphenomenon not interested in one or another phenomenon, notspectrum not in the spectrum of one or another element. His Thoughts I would like to know His Thoughts, everything else are just details. << recalls literal meaning, i.e. basic, not deducible law
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Fundamental Interactions – Standard Model Physics outside Standard Model Searches for New Physics Physics within the Standard Model
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TRI P Possibilities to Test New Models Low Energies & Precision Measurement High Energies & direct observations
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Magnetic Moment * Dirac: g = 2 forspin ½ particles * Baryon Octet: g 2 inner structure proton :g p > 2 neutron: g n 0 * Leptons: g 2 interaction with virtual fields, e.g. QED... electron muon tauon mc e g 2 2 7922 cm e. N p 2 91.12 n cm e N... 2 1 2 2 2 3 2 2 aa g a r e =a 0 e-e- v e = c L=1 magnetic moment M = area * current = area * current = a 0 2 * e*v e /(2 a 0 ) = a 0 2 * e*v e /(2 a 0 ) = e / (2 e m c) = e / (2 e m c) = “magneton” = “magneton” Bohr Magneton for electrons
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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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Slides taken from T. Beier, GSI The bound state introduces : the m e /M nucleus mass ratio the expansion parameter Z
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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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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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Fourier Spectra for different Run Conditions @BNL
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Systematic Uncertainties, Results Magnetic Field p,0 spherical probe 0.05 ppm p (R,t i ) 17 trolley probes 0.09 ppm p (R,t) 150 fixed probes 0.07 ppm p (R) trolley measurement 0.05 ppm < p muon distribution 0.03 ppm p (R I ) others 0.10 ppm total systematic uncertainty p =0.17ppm Spin Precession Pileup 0.08 ppm Lost muons 0.09 ppm Coherent Betatron Oscillations 0.07 ppm Gain Instability 0.12 ppm others 0.11 ppm total systematic uncertainty a,sy = 0.21 ppm total statistical uncertainty a,st = 0.6 ppm p /2 = 61 791 400 (11) Hz a /2 = 229 073.59(15)(5) Hz
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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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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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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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Final results from Experiment E821 @BNL
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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) !!
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Final results from Experiment E821 @BNL Newest Theory Offer: 2.4 SD from Experiment
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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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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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? 18 10 m mm r 0 00 K KK || K 12 102 avg a | e a e a| 3 101.2 avg g | e g e g| e r CPTbreakb,a μμ Invariance LorentzbreakH,d,c,b,a μν μμ ? Lepton Magnetic Anomalies in CPT and Lorentz Non-Invariant Models CPT tests Are they comparable- Which one is appropriate Use common ground, e.g. energies Leptons in External Magnetic Field Bluhm, Kostelecky, Russell, Phys.Rev. D 57,3932 (1998) For g-2 Experiments : Dehmelt, Mittleman,Van Dyck, Schwinberg, hep-ph/9906262 μμ qAiiD 0D μ γ 5 γ μν id ν D μ γ μν ic μν σ H 2 1 μ γ 5 γ μ b μ γ μ am μ D μ (iγ equation DIRAC violating Lorentz and CPT generic ψ ) 2 c l m a Δω l upspin E | l downspin E l upspin E| l r l 3 4b l a ω l a ω a Δω avg ll 2 l c l a |aa| cm ω r 24 103.5 μ r 21 101.2 e r :: muonelectron CPT CPT – Violation Lorentz Invariance Violation What is best CPT test ? New Ansatz (Kostelecky) K 0 10 -18 GeV/c 2 n 10 -30 GeV/c 2 p 10 -24 GeV/c 2 e 10 -27 GeV/c 2 10 -23 GeV/c 2 Future: Anti hydrogen 10 -18 GeV/c 2 often quoted: K 0 - K 0 mass difference (10 - 18 ) e - - e + g- factors (2* 10 -12 ) We need an interaction with a finite strength !
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CPT and Lorentz Invariance from Muon Experiments Muonium: new interaction below 2 * 10 -23 GeV Muon g-2: new interaction below 4 * 10 -22 GeV (CERN) 15 times better expected from BNL V.W. Hughes et al., Phys.Rev. Lett. 87, 111804 (2001)
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Concept works also for (certain) nuclei; Deuteron particularly interesting 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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Klaus P. Jungmann, Kernfysisch Versneller Instituut, Groningen, NL on behalf of the muon g-2 collaboration International Conference on Linear Colliders 04 : 19-23 April 2004 - "Le Carré des Sciences", Paris, France Standard Model Precision Experiment Fundamental Constants Related Experiments Interpretation How reliable is Theory ? What mean Speculations built on whishfull definition of Theory Value? What next in Experiment? - Just run again ? - Just run again ? - Is there more to it ? - Is there more to it ? What about Theory ? Are there other Experiments Neede to come further in Physics?
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Any New Effort to improve significantly on the Muon Magnetic Anomaly will need better constants ! Where should they come from, if not from Muonium Spectroscopy ?
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J-PARC is one Possibility There are others as well: as well: Neutrino Factory ? Neutrino Factory ? Muon Collider ? Muon Collider ? GSI ? GSI ? …. ….
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