Electron Magnetic Dipole Moment
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Gabrielse Most Precise Tests of the Standard Model, Its Extensions and its Symmetries Gerald Gabrielse, Leverett Professor of Physics, Harvard University Spokesperson of the CERN ATRAP Collaboration Testing the Most Precise Prediction of the Standard Model Electron magnetic moment Testing standard model extensions Electron electric dipole moment Testing the Symmetries of the Standard Model Q/M for the antiproton and proton Antiproton and proton magnetic moments Positron and electron magnetic moments (underway) Antihydrogen and hydrogen structure (still in far future) Comparing Antimatter and Mater Gravity Gravitational Redshift of the Antiproton and Proton Supported by US NSF and AFOSR Gabrielse Low Energy Particle Physics AMO Physics, Particle Physics, Plasma Physics methods and funding goals and facility can’t avoid 2 2Mp c LEAR and AD 1010 TRAP 4.2 K 0.3 meV 70 mK, lowest storage energy for any charged particles Gabrielse Gabrielse Electron Magnetic Dipole Moment • Most precise prediction of the standard model • Most precisely measured property of an elementary particle • Most precise confrontation of theory and experiment • Greatest triumph of the standard model Gabrielse The Amazing Electron Electron orbits give atoms their size, but the electron itself may actually have no size 20000 electron masses 20 2 R2 10 m m* 10.3 TeV / c of binding energy for “ingredients” Electron has angular momentum (spin) even though it has no size and nothing is rotating: 2 S m R IA~ R2 Magnetic dipole moment: What about electric dipole? S S d d / 2 / 2 Gabrielse Standard Model of Prediction 2 3 4 5 e 1 CCCCC2 4 6 8 10 ... 2m B a hadronic a weak a new physics Dirac 1 QED essentially exact Hadronic Weak aweak smaller Gabrielse The Standard Model Predicts the Electron Magnetic Moment in terms of the 1e2 1 fine structure 4 c 137 constant 0 Gabrielse Probing 10th Order and Hadronic Terms Dirac QED Gabrielse David Hanneke G.G. Shannon Fogwell Gabrielse Need Good Students and Stable Funding Elise Novitski Joshua Dorr Shannon Fogwell Hogerheide David Hanneke Brian Odom, Brian D’Urso, 20 years Steve Peil, 8 theses Dafna Enzer, Kamal Abdullah Ching-hua Tseng Joseph Tan N$F Gabrielse Cylindrical Penning Trap V~ 2 z2 x 2 y 2 • Electrostatic quadrupole potential good near trap center • Control the radiation field inhibit spontaneous emission by 200x (Invented for this purpose: G.G. and F. C. MacKintosh; Int. J. Mass Spec. Ion Proc. 57, 1 (1984) Gabrielse Trap with One Electron Quantum Cyclotron -charges- - - - - - fc 150 GHz 2 n = 4 n = 3 n = 2 0.1 n = 1 m m hc 7.2 kelvin n = 0 y2 - - - - - - - Need low temperature B 6Tesla cyclotron motion T << 7.2 K 0.1 m m Gabrielse Quantum Measurement of the Electron Magnetic Moment S E ms s ( n 1/ 2) c / 2 Spin flip energy: BB 2 s s eB Cyclotron energy: c 2 B B c B (the magnetometer) m Bohr magneton e 2m Need to resolve the quantum states of the cyclotron motion Relativistic shift is 1 part in 109 per quantum level Gabrielse Quantum Jump Spectroscopy • one electron in a Penning trap • lowest cyclotron and spin states “In the dark” excitation turn off all detection and cooling drives during excitation Gabrielse Inhibited Spontaneous Emission Application of Cavity QED excite, measure time in excited state 30 t= 16 s 15 12 20 9 6 10 Y Axis 2 3 0 0 number of n=1 to n=0 decays -3 axial frequency shift (Hz) 0 10 20 30 40 50 60 0 100 200 300 decay time (s) time (s) many other new methods Most precisely measured property of an elementary particle Gabrielse Electron Magnetic Moment Measured to 3 x 10-13 2.8 1013 (improved measurement is underway) Gabrielse from measured fine structure constant Gabrielse From Freeman Dyson – One Inventor of QED Dear Jerry, ... I love your way of doing experiments, and I am happy to congratulate you for this latest triumph. Thank you for sending the two papers. Your statement, that QED is tested far more stringently than its inventors could ever have envisioned, is correct. As one of the inventors, I remember that we thought of QED in 1949 as a temporary and jerry-built structure, with mathematical inconsistencies and renormalized infinities swept under the rug. We did not expect it to last more than ten years before some more solidly built theory would replace it. We expected and hoped that some new experiments would reveal discrepancies that would point the way to a better theory. And now, 57 years have gone by and that ramshackle structure still stands. The theorists … have kept pace with your experiments, pushing their calculations to higher accuracy than we ever imagined. And you still did not find the discrepancy that we hoped for. To me it remains perpetually amazing that Nature dances to the tune that we scribbled so carelessly 57 years ago. And it is amazing that you can measure her dance to one part per trillion and find her still following our beat. With congratulations and good wishes for more such beautiful experiments, yours ever, Freeman. Gabrielse Test for Physics Beyond the Standard Model g 1 aQED () aSM: Hadronic Weak aNewPhysi c s B 2 Does the electron have internal structure? m* total mass of particles bound together to form electron m 2 limited by the uncertainty in R5 1019 m m* 360 GeV / c a independent a value m R2 1019 m m* 1 TeV / c2 if our uncertainty a was the only limit Not bad for an experiment done at 100 mK, but LEP does better R2 1020 m m* 10.3 TeV / c2 LEP contact interaction limit > 20000 electron masses of binding energy Gabrielse Gabrielse Electron Electric Dipole Moment • Most precise test of extensions to the standard model • 12 times more precise than previous measurements S S Magnetic moment: Electric dipole moment: d d / 2 / 2 Well measured Does this also exist? Gabrielse Particle EDM Requires Both P and T Violation Magnetic moment: Electric dipole Moment: S S d d / 2 / 2 If reality is invariant under parity transformations P P d = 0 T If reality is invariant under time reversal transformations T d = 0 Gabrielse Standard Model of Particle Physics Currently Predicts a Non-zero Electron EDM four-loop -38 Standard model: d ~ 10 e-cm level in perturbation Too small to measure by orders of magnitude theory best measurement: d ~ 2 x 10-27 e-cm Weak interaction couples quark pairs (generations) CKM matrix relates to d, s, b quarks (Cabibbo-Kabayashi-Maskawa matrix) almost the unit matrix Gabrielse Extensions to the Standard Model Much Bigger, Measureable Electron EDM An example Low order contribution larger moment Low order contribution vanishes From Fortson, Sandars and Barr, Physics Today, 33 (June 2003) Gabrielse New Electron EDM Measurement is Almost Done Gabrielse Advanced Cold-Molecule Electron EDM Harvard University Yale University John Doyle Group David DeMille Group Gerald Gabrielse Group Jacob Baron, Wes Campbell, David DeMille, John Doyle, Gerald Gabrielse, Paul Hess, Nick Hutzler, Emil Kirilov, Brendon O’Leary, Cris Panda, Elizabeth Petrik, Ben Spaun, Amar Vutha, Adam West Funding from NSF Gabrielse How to Measure an Electron EDM Put the EDM in an Electric Field bigger is better H d E Measure the energy shift for the system Gabrielse Cannot Use Electric Field Directly on an Electron or Proton Simple E and B can be used for neutron EDM measurement (neutron has magnetic moment but no net charge) Electric field would accelerate an electron out of the apparatus Electron EDM are done within atoms and molecules (first molecular ion measurement is now being attempted) Gabrielse Schiff Theorem – for Electron in an Atom or Molecule Schiff (1963) – no atomic or molecular EDM (i.e. linear Stark effect) • from electron edm • nonrelativistic quantum mechanics limit Sandars (1965) – can get atomic or molecular EDM (i.e. linear Stark effect) • from electron edm • relativistic quantum mechanics • get significant enhancement (D >> d) for large Z Commins, Jackson, DeMille (2007) – intuitive explanation Schiff Lorentz contraction of the electron EDM in lab frame Schiff, Phys. Rev. Lett. 132, 2194 (1963); Sandars, Phys. Rev. Lett. 14, 194 (1965); ibid 22, 290 (1966). Commins, Jackson, DeMille, Am. J. Phys. 75, 532 (2007). Gabrielse Why Use a Molecule? To Make Largest Possible Electric Field on Electron Tl atom (best EDM limit till YbF) ThO molecule Elab123 kV/cm E eff 72 MV/cm EGlab100 V/cm E eff 100 V/cm Molecule can be more easily polarized using nearby energy levels with opposite parity (not generally available in atoms) Gabrielse Detect the Energy Difference S two states evolve differently in time g / 2 i E t /hbar S e de d e / 2 Gabrielse Still, the EDM Gives Tiny Shift of Energy Levels 2 mHz E 7 1018 eV 7 1027 GeV Not so easy to resolve 7 1030 TeV To detect let a prepared wave function evolve for time T large as | (0) |1 | 2 | (T) |1ei | 2 possible E T T1.1 ms 11 106 0.6 10 3 degrees Example is for an electron edm equal the ACME upper limit. Gabrielse Experiment in Two Labs – 100 Meters Separated Harvard Jefferson Building Harvard LISE Building ThO Source and Interaction Chamber 100 m optical fibers (2 floors down) Lasers, Iodine Clock, Comb Gabrielse ThO Molecular Beam Pulse Tube Cooler Molecular Beam “Interaction Source Region”: E- field plates inside, B- field shields Pulsed and coils YAG outside Prep Lasers Probe Lasers Lasers 100m away 34 Gabrielse Magnetic Field Coils and Shielding mu metal 5 shields endplates (no shown) ~ 10-5 ThO beam shielding Interaction Cos(theta) chamber coils