The Anomalous Magnetic Moment of the Muon

The Anomalous Magnetic Moment of the Muon

The anomalous magnetic moment of the muon Vladimir Tishchenko Brookhaven National Laboratory ISU Colloquium 18 April, 2016 Outline ● Magnetic moment ● History of the magnetic moments ● Future muon g-2 experiment at Fermilab V. Tishchenko Idaho State University, Colloquium 18 April, 2016 2 Magnetic Moment ● … is a vector quantity characterizing magnetic interaction of an object with a magnetic field spinning ball of charge the torque orbiting charged particle current loop S – spin angular momentum (depends on mass distribution) γ - gyromagnetic ratio if charge distribution is not the same as the mass distribution, L – orbital angular momentum introduce g factor, V. Tishchenko Idaho State University, Colloquium 18 April, 2016 3 Some History ● 1896 Zeeman effect – splitting of spectral lines into several components in presence of a magnetic field ● 1922 Stern-Gerlach experiment ● 1924 Pauli postulated a fourth quantum number to explain the anomalous Zeeman effect ● 1925 R. Kronig (20): concept of spinning electron. Unpublished. ● 1925 G. E. Uhlenbeck (25) and S. A. Goudsmit (23): hypothesis of electron spin, with possible quantum numbers of either + ½ or -½. Sent for publication by Ehrenfest: "Well, that is a nice idea, though it may be wrong. But you don't yet have a reputation, so you have nothing to lose". V. Tishchenko Idaho State University, Colloquium 18 April, 2016 4 Solution of the electron g problem ● 1928 P. Dirac (25) ● 1933 O. Stern and I. Estermann: g-factor of the proton Pauli: “Don't you know the Dirac theory? It is obvious that gp=2.” measured value: gp≈5.6 μ turned out to be a harbinger of new physics! p Was finally explained, along with the g value of the BNL neutron, g =-3.8 om the 1960 by the quark model. proton substructure! n V. Tishchenko Idaho State University, Colloquium 18 April, 2016 5 Nature abhors a vacuum ● At least for the electron, things finally in good shape with Dirac's new theory until... ● 1930s Oppenheimer and others tried to calculate correction to ge=2. Result: infinity. ● 1947 P. Kusch and H.M. Foley: ● 1948 J. Schwinger ● QED ● Feynman diagrams... ● 1970s weak interactions unified with QED V. Tishchenko Idaho State University, Colloquium 18 April, 2016 6 anomalous magnetic moment V. Tishchenko Idaho State University, Colloquium 18 April, 2016 7 Present status: electron ● 2008 G. Gabrielse, Harvard PRL 100 (2008) 120801 ● Take α from external measurements to test QED PRA 73 (2006) 032504 PRL 106 (2011) 080801 ● Or, assume ge and calculate α PRL 100 (2008) 120801 μ gives the most precise determination of the fine structure constant! e V. Tishchenko Idaho State University, Colloquium 18 April, 2016 8 Theory ● th QED now calculated ae to 5 order in (12672 diagrams). Kinoshita & collaborator., 2008, 2012 Schwinger 1948 Karplus & Kroll 1950; Petermann, Sommerfield 1957 Elend 1966 Fujikawa, Lee, Sanda 1972; Czarnecki, Krause, Marciano 1996; Knecht, Peris, Perrottet, Rafael, 2002; Czarnecki, Marciano, Vainshtein, 2003; Nomura & Teubner, 2012; Lautrup, Peterman, de Rafael 1974; Laporta, Remiddi 1996; Kinoshita 1995 Prades, Rafael, Vainshtein, 2009 Samuel & Li, 1991 Samuel & Li, 1991 Samuel & Li, 1991 Kinoshita & collaborator., 1983, 2002, 2005, 2007, 2012 Sensitivity of ae to “new physics” at a mass scale Λ Berestetskii, 1956 V. Tishchenko Idaho State University, Colloquium 18 April, 2016 9 choice of heavy particles to probe NP Only exist as complicated multi-body objects Too fleeting or no electric charge Neutral (and too light) V. Tishchenko Idaho State University, Colloquium 18 April, 2016 10 tauon ● mτ = 1777 MeV ● 7 (mτ/me)2 ≈ 1.2x10 ● τ meson has heightened sensitivity to higher-mass exchanges ● ττ ~ 0.29 ps ● Limits current precision to - 0.052 < aτ <0.013 V. Tishchenko Idaho State University, Colloquium 18 April, 2016 11 muon ● mμ = 106 MeV ● 4 (mμ/me)2 ≈ 4x10 ● ττ ~ 2.2 μs → convenient for exp. study V. Tishchenko Idaho State University, Colloquium 18 April, 2016 12 muon ● 1933 First observed in cosmic rays. “Particle of uncertain nature”, Paul Kunze, Z. Phys. 83 (1933) 1. ● 1935 Hideki Yukawa: meson theory, Proc. Phys.-Math. Soc. Jap. 17 (1985), 48 ● 1936 Seth Neddermeyer and Carl Anderson: particle in cosmic rays with a mass “greater than an electron but smaller than a proton”. I. I. Rabi: "Who ordered that?" ● … -1957 V.B. Berestetskii, R.P. Feynman, J.S Schwinger: The muon (g − 2) experiment was recognized as a very sensitive test of the existence new fields, and potentially a crucial signpost to the μ–e problem. ● 1956-1957 T.D. Lee, C.N. Yang, C.S. Wu: parity violation ● 1957 R.L. Garwin, L. Lederman, M. Weinrich - antecedent of the (g-2) measurements V. Tishchenko Idaho State University, Colloquium 18 April, 2016 13 muon – “self analyzing polarimeter” q e+ V. Tishchenko Idaho State University, Colloquium 18 April, 2016 14 R.L. Garwin, L. Lederman, M. Weinrich, 1957 The magnetizing coil was close wound directly on the graphite to provide a uniform vertical field of 79 gauss per ampere. The various counters defined the event by use of a coincidence-anticoincidence analyzer V. Tishchenko Idaho State University, Colloquium 18 April, 2016 15 Muon g-2 experiment in a nutshell 1) Take polarized muons (come naturally from pion decay) 2) Inject muons into a uniform magnetic field – Momentum precession (cyclotron frequency) – Spin precession momentum spin V. Tishchenko Idaho State University, Colloquium 18 April, 2016 16 1st CERN muon g-2 experiment 1958-1962 6-m-long 52-cm-wide 14-cm-gap bending magnet, B=1.5 T. 440 turns during τ=2.2 μs. Muon step size from 0.4cm to 11 cm. Time t spent inside the magnet was determined by by coincidence in counters 123 at input, and counters 466'57 at the output. t=2-8 μs depending on the location of the orbit center on the varying gradient field. 150 MeV/c muons V. Tishchenko Idaho State University, Colloquium 18 April, 2016 17 1st CERN muon g-2 experiment 1958-1962 The first CERN g-2 team: Sens, Charpak, Muller, Farley, Zichichi (CERN/1959) → muon behaved so precisely as a structureless point-like QED particle; a heavy twin for the electron V. Tishchenko Idaho State University, Colloquium 18 April, 2016 18 1st muon storage ring at CERN, 1962-1968 features: ● weak focusing ring, n=0.13 ● B=1,.711 T ● orbit diameter: 5m ● aperture: 4cm x 8 cm ● beam: 10.5 GeV protons ● injection time: 10 ns ● rotation time: 50 ns ● stored muons: p=1.28 GeV/c ● γ = 12, t=27 μs problems: ● high background ● low muon polarization V. Tishchenko Idaho State University, Colloquium 18 April, 2016 19 1st muon storage ring at CERN, 1962-1968 … after an error in QED LBL calculations was corrected J. Aldins et al., PRD 1 (1970) 2378 V. Tishchenko Idaho State University, Colloquium 18 April, 2016 20 2nd muon storage ring at CERN, 1969-1976 Motivation ● to look for departures from standard QED ● to detect contributions of strong interactions to aμ through hadron loops in the vacuum polarization ● to search for new interactions of the muon V. Tishchenko Idaho State University, Colloquium 18 April, 2016 21 2nd muon storage ring at CERN, 1969-1976 features: ● 40 C-shaped bending magnets ● pole: 38-cm x 14 cm (width x gap) ● field in each magnet stabilized with NMR probes ● electric quadrupoles for vertical focusing ● pion injection! V. Tishchenko Idaho State University, Colloquium 18 April, 2016 22 2nd muon storage ring at CERN, 1969-1976 ● Excellent agreement with theory ● QED calculations verified up to the sixth order ● Confirmation of the existence of hadronic vacuum polarization at the level of 5σ. ● No evidence of special coupling to the muon V. Tishchenko Idaho State University, Colloquium 18 April, 2016 23 Final stop on the history tour...Brookhaven Motivation ● to measure electroweak contributions to aμ which arise from single loop diagrams with vitural W and Z bosons ● to search for new interactions of the muon A picture from 1984 showing the attendees of the first collaboration meeting to develop the BNL g-2 experiment. Standing from left: Gordon Danby, John Field, Francis Farley, Emilio Picasso, and Frank Krienen. Kneeling from left: John Bailey, Vernon Hughes and Fred Combley V. Tishchenko Idaho State University, Colloquium 18 April, 2016 24 SM prediction for aμ QED Weak Hadronic QED: photonic and leptonic (e,τ,μ) loops, Weak: loops involving W±, Z or Higgs suppressed by at least a factor of , Hadronic: quark and gluon loops. at present not calculable from first principles relies on a dispersion relation approach Total: -- PDG-2013 V. Tishchenko Idaho State University, Colloquium 18 April, 2016 25 Brookhaven storage ring ● Long list of innovations beyond CERN III – Flux in 12 bunches from the AGS – Long enough beamline to operate with pion or muon injection – Inflector to get muons through the back yoke...allowed muon injection – High voltage, fast, non-ferric kickers to shift muon onto orbit in first cycle – Thin quadrupoles and scalloped vacuum vessels minimize preshower – In situ, field measurements with NMR trolley – Continuous NMR monitoring and <0.1 ppm absolute calibration – Pb/Scifi calorimeters, hodoscopes, and a traceback wire chambers V. Tishchenko Idaho State University, Colloquium 18 April, 2016 26 BNL g-2 experiment in a nutshell V. Tishchenko Idaho State University, Colloquium 18 April, 2016 27 BNL g-2 experiment in a nutshell Determining the anomalous magnetic moment requires measuring 2001 data from E821 ● The spin precession frequency muon decay is self-analyzing: higher energy positrons are emitted preferen- tially in direction of muon spin wrapped around modulo 100 μs ● The magnetic field B ( ) 375 fixed NMR probes 17 NMR trolley probes V. Tishchenko Idaho State University, Colloquium 18 April, 2016 28 Electric quads to contain the beam vertically +HV -HV -HV +HV E-field contribution vanishes V.

View Full Text

Details

  • File Type
    pdf
  • Upload Time
    -
  • Content Languages
    English
  • Upload User
    Anonymous/Not logged-in
  • File Pages
    84 Page
  • File Size
    -

Download

Channel Download Status
Express Download Enable

Copyright

We respect the copyrights and intellectual property rights of all users. All uploaded documents are either original works of the uploader or authorized works of the rightful owners.

  • Not to be reproduced or distributed without explicit permission.
  • Not used for commercial purposes outside of approved use cases.
  • Not used to infringe on the rights of the original creators.
  • If you believe any content infringes your copyright, please contact us immediately.

Support

For help with questions, suggestions, or problems, please contact us