1. Experimental Atomic Physics Research in the Budker Group Tests of fundamental symmetries using atomic physics: Parity Time-reversal invariance Permutation Postulate/Spin-Statistics Connection Temporal variation of fundamental “constants” Applied atomic spectroscopy Sensitive magnetometry and electrometry Nonlinear optics with atoms Optical properties of superfluid helium “New” atomic energy levels Properties of complex atoms: the rare earths, Ba

2. Group Demographics and Philosophy 6 graduate students 1 - 3 undergrads 2 staff scientists (1 senior, 1 junior) Part-time technician Lots of visitors from US and abroad Each student has their own project Lots of interactions within group Variety of experiences and techniques: lasers, optics, atomic beams and vapor cells, cryogenics, computer control and data acquisition, vacuum, electronics, theory, scientific writing and editing, …..

3. Further information: http://socrates.berkeley.edu/~budker budker@socrates.berkeley.edu Office: 273 Birge; labs: 217,219,221,230,241, and 245 Birge

4. Z e e  Weak interaction (violates parity) Electromagnetic interaction (conserves parity) Atomic Parity Nonconservation  Small Modifications of the Optical Properties of Atoms Provides Unique Low-Energy Test of the Standard Model

5. Electric and magnetic fields define a handedness PNC effects show up as dependence of atom-photon interaction on handedness PNC Experiments Two Experiments in Progress: Dysprosium (Z=66) and Ytterbium (Z=70)

6. How constant is the fine structure “constant”  ? Theories that unify gravity with other forces either allow or necessitate  variation THEORETICAL Laboratory: H-maser vs. Hg+ microwave clock:  /  < 3.7  10 -14 /yr Rb vs. Cs microwave clocks:  /  < 1.1  10 -14 /yr Hg+ optical vs. Cs microwave clocks:  /  < 1.2  10 -15 /yr... Geophysical: Oklo natural nuclear reactor 1.8 billion years ago:  /  < 10 -18 /yr. Astrophysical: [J. K. Webb, et al., Phys. Rev. Lett. 87, 091301 (2001).]  /  = (-7.2  1.8)  10 -16 /yr. EXPERIMENTAL

7. AB Ground State 0 20,000 Energy (cm -1 ) levels A and B are highly sensitive to variations in   in dysprosium ’ ~ 3-2000 MHz atomic beam PMT atomic freq. standard rf freq. generator fluor. E-field plates  ~ 2  10 15 Hz |  /  | i.e. for |  /  | ~ 10 -15 /yr  ~ 2 Hz/yr    

8. NONLINEAR MAGNETO-OPTICAL ROTATION Goal: Obtain highest possible sensitivity to magnetic fields. Use laser light to polarize atoms: (1)Aligns magnetic dipole moments; (2)Creates preferred optical axis. F = 1 F ’ = 0 M F = -1M F = 0M F = +1 Magnetic moments precess in magnetic field: Optical axis rotates  causes light polarization to rotate.  g F  rel  g F  rel ) 2

9. Paraffin-coated cells smuggled in as Christmas ornaments!  rel  1 Hz Slow relaxation of atomic polarization:  ~ 1  G ~ 0.1 nT (For FSB agents: this is a joke!)

10. FM NMOR magnetometry: Phys.Rev.A65, 055403 (2002) Pumping and probing with FM light

11. Precision magetometry and atomic EDM measurement using spin-polarized atoms in a buffer gas at cryogenic temperatures Problem: to measure very small B; to measure electron EDM Paramagnetic atom magnetometer; He buffer gas at T=4K to increase spin-relaxation time to minutes Measuring the Kerr effect in LHe and the LANL neutron EDM experiment Problem: to measure strong electric fields (50kV/cm) inside a bath of LHe at 300mK. Kerr effect: an initially isotropic medium acquires birefringence when electric field is applied, measure this.

12. 241 Birge, midnight, 8/25/03

13. Light Guides Cells Between Electrodes HV and Ground Electrodes Beam Entrance Window HV Variable Capacitor SQUID Enclosure Cos  Coil Neutron EDM experiment at LANSCE

14.  Motivation: BEV exp  Lifetimes, branching ratios, new levels, polarizabilities (Ba)  Unusually large polarizabilities “new” opposite-parity levels Electron EDM exp Noncontact circuit board testing (100 times; for n<10, only smaller than 2s,2p of H) Laser spectroscopy for fundamental symmetry tests

15. 6s6p 1 P 1 6s6p 3 P 0,1,2 Laser Excitation 554.7 nm Fluorescence ~ 435 nm 6s 2 1 S 0 Probed States Even ParityOdd Parity 559 - 569.5 nm Laser Excitation

16. What is the experiment? A test of the spin statistics theorem (SST) for photons. What is the SST?

17. Barium How we do it

18. Interaction region

19. Power Build-up Cavity

20. Oven Housing w/Collimator

21. Chamber

22. Numbers

23. Experimental Atomic Physics Research in the Budker Group