570 likes | 716 Views
Muon g-2 Collaboration Meeting Fermilab 18-19 March 2011. Systematics on p. Precision Measurement of the Magnetic Field for a Muon g-2 Determination. Klaus Jungmann Kernfysisch Versneller Instituut University of Groningen Netherlands. Context Basics Fundamental Constants
E N D
Muon g-2 Collaboration Meeting Fermilab 18-19 March 2011 Systematics on p Precision Measurement of the Magnetic Field for a Muon g-2 Determination Klaus Jungmann Kernfysisch Versneller Instituut University of Groningen Netherlands
Context • Basics • Fundamental Constants • Field Measurement • Open Issues
Context • Basics • Fundamental Constants • Field Measurement • Open Issues
Open technical issues • Local magnetic environment • Shimming • Field monitoring • Field analysis • Quench protection • Requires very careful work • nothing less – nothing more K. Jungmann, mar 2011
Context • Basics • Fundamental Constants • Field Measurement • Open Issues
Spin Precession Frequency electric field plays minor role
Two quantities are measured: • magnetic field proton NMR, wp • anomaly frequency decay electrons, wa • BOTH EQUALLY IMPORTANT
Looks like a simple Experiment * One is inclined to believe a and Bare just other constants to be measured. * This were true, if spin could follow field changes adiabatically, i.e. field changes seen by the particle happen on a timescale >> 1 / a * However:
correction = (0,0,Bz) dimension m }jz J • (2* jmax+ 1) possibilities for • mJ =jz • Allow for correction • m = gmB Magnetic Moment – in Quantum Mechanics • Magnetic Moment proportional • to angular Momentum • Energy in external Magnetic Field B • is scalar product of Field and • Magnetic Moment • Precession frequency in external • Magnetic Field
Allows for non-trivial Corrections Contains all interesting physics Magnetic Moment Angular Momentum Gives dimensions and scale for a particle
B0=1.45T n0=62 MHz e.g. Proton NMR to determine a field Lepton Spin Resonance / Nuclear Magnetic Resonance For tranverse polarized particles Precession with frequency n0 : Energy E0+ s mB B Somewhat more QM correct: <sz> =0 <sx(t)> = ssin(2pn0t) <sy(t)> = scos(2pn0t) n0 : Larmor frequency 2 s hn0 E0 S E0– s mB e.g. S =1/2 • measure m, if B is known • measure B, if m is known B0 Magnetic Field
Note: • NMR measures: • Maxwells equations require: • 0th order • 2nd order Zeeman effect • measure • shimming watch out for timedependent correlated field variations
Magnetic Moment Measurements Proton: best measurement from proton NMR in water (spherical water probe) Electron: e.g. from hydrogen maser also calculated from constants Best values: come from least square adjustment of Fundamental Constants. CODATA (NIST, B.Taylor & P. Mohr, ~every 2 years) Finds also way in particle data book Involves heavily theory : Check for intellectual Phase locking !
Context • Basics • Fundamental Constants • Field Measurement • Open Issues
Theory: * need a for muon ! * hadronic and weak corrections *various experimental sources of a<better 100ppb>need constants at very moderate *a no concern for (g-2)maccuracy wa wammc Experiment: wp = am = mm wa emB - wp mp * wa and B (wp) measured in (g-2)m experiment <better 0.35 and 0.1 ppm> * c is a defined quantity <“infinite” accuracy> *mm (mm) is measured in muonium spectroscopy (hfs) <better 120 ppb> NEW 1999 *em is measured in muonium spectroscopy (1s -2s) <better 1.2 ppb> NEW 1999 *mp in water known >> probe shape dependence<< <better 26 ppb> *m3He to mp in water >> gas has no shape effect << <better 4.5 ppb> being improved
m g-2 hadronic contribution weak contribution New Physics QED QED h mm, a, gm mm m+e- DnHFS, n=1 m+e- Dn1S-2S QED mm mm a QED corrections weak contribution mm QED corrections
Solenoid Sm m+ e- Gated Detector m+in MW-Resonator/Kr target Muonium Hyperfine Structure Yale - Heidelberg - Los Alamos
Solenoid Sm m+ e- Gated Detector m+in MW-Resonator/Kr target Muonium Hyperfine Structure Yale - Heidelberg - Los Alamos Very same equipment to calibrate field than for g-2 Therefore:: Use these values, NOT adjusted values !!! unless you are prepared to redo that experiment
History of Muonium Ground State Hyperfine Splitting Measurements NEVIS CHICAGO-SREL LAMPF LAMPF latest experiment Quoted Uncertainty [kHz] Year
Muonium 1s-2s At RAL 1987 -2000
m++ e-+ Ekin 0 -.25 Rm 2S 244 nm Energy 244 nm mm n1s2s= ¾ R -Rm 1S me + mm m+ Detection m+ Laser Mirror m+e- Target Diagnostics m+in Muonium 1S-2S Experiment Heidelberg - Oxford - Rutherford - Sussex - Siberia - Yale
exp Dn 1s-2s = 2455 528 941.0(9.1)(3.7) MHz Dn 1s-2s = 2455 528 935.4(1.4) MHz mm+= 206.768 38 (17) me (0.8ppm) qm+= [ -1 -1.1 (2.1) 10-9 ] qe-(2.2 ppb) theo Results:
CODATA CODATA Fine Structure Constant a a-1= 137.035 999 710 (96) a-1= 137.035 999 084 (51) Test of Internalconsistency of QED Test of Internal consistency of QED
Context • Basics • Fundamental Constants • Field Measurement • Open Issues
B0=1.45T n0=62 MHz e.g. Proton NMR to determine a field Lepton Spin Resonance / Nuclear Magnetic Resonance For tranverse polarized particles Precession with frequency n0 : Energy E0+ s mB B 2 s hn0 E0 S E0– s mB e.g. S =1/2 • measure m, if B is known • measure B, if m is known B0 Magnetic Field
Electronics, Computer& Communication Position of NMR Probes Key Elements of the Field Measurement System Absolute Calibration Probe: a Spherical Water Sample Fixed Probes in the walls of the vacuum tank Trolley with matrix of 17 NMR Probes
all probes MUST be checked individually, refurbished and possibly filled with petroleum jelly manpower !(student assistants)
The fixed probes 4 ppm Proton NMR
counting zero crossings • FFT of full 360 signals every second? • (check advantage)
NMR trolley > 15 man years
Magnetic Field vs Azimuth (1999) Before 1999 Inflector fringe field
shimming shimming At this level, one hardly needs to know the muon distribution Improvement of Field 2000 1999 2001
Systematic Uncertainties, Results (m-) • Magnetic Field • wp,0 spherical probe 0.05 ppm • wp(R,ti) 17 trolley probes 0.09 ppm • wp(R,t) 150 fixed probes 0.07 ppm • wp(R) trolley measurement 0.05 ppm • < wp> muon distribution 0.03 ppm • wp (RI) inflector fringe field - - • others 0.10 ppm • total systematic uncertainty • dwp=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 • dwa,sy = 0.21 ppm • total statistical uncertainty • dwa,st = 0.6 ppm wa/2p = 229 073.59(15)(5) Hz wp/2p = 61 791 400 (11) Hz
What needs to be done: • survey magnetic environment • shimming – radial and azimuthal • frequent full field maps (trolley) at random time of day • frequent absolute calibrations (every 5th trolley run) • rigorous susceptibility police • of course, refurbishing of equipment
Open technical issues (I) • Local magnetic environment near the ring • monitor environment : • close ring storage ring AND transients caused far away (accelerator) • on its way ( T. Chupp) • susceptibility ‘Sherif’ : materials, lamps, screwdrivers, … • ( local respected authority !!!!!) • training of technicians AND scientists • we have all necessary tools available – manpower important • people to do the job • everybody needs to know the real issues K. Jungmann, mar 2011
Open technical issues (II) • Shimming • nothing too spectacular (like detectors per se) BUT very important • no showstoppers expected to <.2 ppm integral (aver.) homogeneity • HOWEVER: Time needed! • several rounds: allow for time to do – analyze- learn – do – analyze … • wedges, o.k. just do it • surface coils : most urgent issue - power supplies • shorter cables or new supplies • activate dipole extra shimming coils ? • define TEAM NOW K. Jungmann, mar 2011
Ring relocation • Heavy-lift helicopters bring coils to a barge • Rest of magnet is a “kit” that can be trucked to and from the barge • What’s the effect on the coils?
Electronics, Computer& Communication Position of NMR Probes Don’t even Think about Touching Absolute Calibration Probe: a Spherical Water Sample Trolley with matrix of 17 NMR Probes unless you are prepared to spend >20 man years
Usefull Modifications: Fixed Probes in Orbital Plane Some Fixed Probes relocated
Useful Modification : Trolley Drive Motors it turns out: We could use Stepping Motors advantage: Possible Speed
He3 probes are shape independent nice additional independent absolute field measurement
Evolution uncertainties in muon g-2 Improvements for future Field: temperature stability, absolute calibration, trolley position, more probes Precession: new scraping scheme, thresholds, energy calibration, new calorimeters, more complete digitization Statistics: more muons, backward decaying pions, new inflector