First Year Seminar: Strontium Project Graham Lochead 03/06/09 Outline • Introduction and motivation • Second generation cell • Polarization spectroscopy and subDoppler DAVLL • Strontium pyramid MOT • 689 nm locking progress Graham Lochead 03/06/09 Motivation: Rydberg physics • Rydberg states are states with large n • Rydberg states have 2 large orbital radii n • We aim to trap ultracold strontium in a 1-D optical lattice and excite to Rydberg states Graham Lochead 03/06/09 Motivation: Ultracold plasmas • Most plasmas are dominated by their thermal energy • Coulomb coupling parameter is ratio of Coulomb energy to thermal energy • Strong Coulomb interactions lead to spatial corrrelations • Cold plasma in a spatially ordered lattice will be a first T.C. Killian et al., Physics Reports 449, 77 (2007) Graham Lochead 03/06/09 Strontium overview • Alkaline-earth element (Group II) • Atomic number 38 84 Sr 86 Sr 87 Sr 88 Sr 0.6% 9.9% 7% 82.5% Graham Lochead 03/06/09 I=0 I=0 I=9/2 I=0 boson boson fermion boson Electronic structure 3D 3S 1 2 412 nm 1 1P 1 3P 2 1D 2 461 nm /2p = 32 MHz 689 nm /2p = 7.5 kHz ground state – no optical pumping • Low decay rate to metastable state 3P2 1S 0 1 0 698nm /2p = 1 mHz 87Sr 1S 0 • 3 • Broad linewidth for 1S0-1P1 transition • Intercombination line for further cooling Graham Lochead 03/06/09 Why strontium? • Singly ionised strontium has an optical transition at ~ 422 nm for 2S1/2-2P1/2 • Ion transition can be used for: – imaging – observing charge transfer – laser cooling – Rydberg manipulation T.C. Killian et al., Phys. Rev. Lett., 92:143001, 2004. Graham Lochead 03/06/09 Laser frequency stabilization “locking” Laser locking requires an atomic sample to investigate the transition And a detection scheme that gives a slope to lock to Graham Lochead 03/06/09 • Introduction and motivation • Second generation cell • Polarization spectroscopy and subDoppler DAVLL • Strontium pyramid MOT • 689 nm locking progress Graham Lochead 03/06/09 Problems with strontium Locking to a transition requires an atomic sample Atomic strontium has very low vapour pressure Hot strontium reacts with glass and copper M. Asano, K. Kubo J. Nuclear Sci. & Tech. 15 pp. 765~767 (1978) Graham Lochead 03/06/09 Dispenser technology Sr Sr • Sealed in argon with indium plug • Directional source of atomic vapour • Flux is dependent on current supplied Graham Lochead 03/06/09 First generation cell Dispenser • Birefringent sapphire windows not required • No continual pumping • No buffer gas • Lifetime estimate ~ 10000 h • Compact size for Sr • Strontium acts as a getter • Only 15-20% absorbtion stable operation A vapor cell based on dispensers for laser spectroscopy E. M. Bridge, J. Millen, C. S. Adams, M. P. A. Jones Rev. Sci. Instr. 80,013101 (2009) Graham Lochead 03/06/09 Second generation cell 30 cm Dispenser Baffle Designed by Clementine Javaux Graham Lochead 03/06/09 Second cell absorption Doppler FWHM of 1.7 GHz at 50% absorption • Optically thick for 461 nm transition • Wide Doppler profile due to dispenser type Graham Lochead 03/06/09 Second cell saturated absorption 124.5 MHz Probe = 0.14 mW Pump = 7.3 mW Pump Laser probe L 0 k v Probe Cell Frequency axis calibrated from 86Sr-88Sr splitting 88Sr transition peak is ~5% of the optical depth Graham Lochead 03/06/09 • Introduction and motivation • Second generation cell • Polarization spectroscopy and subDoppler DAVLL • Strontium pyramid MOT • 689 nm locking progress Graham Lochead 03/06/09 Polarization spectroscopy theory J=1 mJ = -1 5s5p 1P 1 0 σ- 5s2 1S0 I signal p J=0 mJ = 0 +1 σ+ 1 ( ) 2 2 1 ( ) Cell 2 x I H IV I 0 L 0 1 x2 x 2 0 M. L. Harris, et al. Phys. Rev. A, 73:062509, 2006. C. P. Pearman et al., J. Phys. B, 35:5141, 2002. Graham Lochead 03/06/09 Polarization spectroscopy setup Polarization spectroscopy Frequency calibration Laser Metal mirror 1 ( ) 2 Cell 1 2 Cell 2 Differential photodiode 4 Graham Lochead 03/06/09 Polarization spectroscopy results Signal (mV) • Gives a steep gradient – easy to lock to • 0.8 MHz rms offset stability over an hour 20 0 -20 -40 -400 -200 0 200 Detuning (MHz) 40 20 (a) 0 0 0.2 0.4 0.6 Intensity (W cm-2) 0.8 Gradient (mV MHz-1) Amplitude (mV) 60 1.2 0.8 0.4 00 (b) 0.2 Graham Lochead 03/06/09 0.4 0.6 Intensity (W cm-2) 0.8 400 DAVLL theory Dichroic Atmoic Vapour Laser Lock (DAVLL) 5s5p 1P1 mJ = -1 E J=1 +1 +1 0 mJ = -1 p + σ σ+ σ-σ 5s2 1S0 Apply a uniform magnetic E field to atomic sample with Helmholtz coils J=0 mJ = 0 Creates a difference in frequency between different transitions E mJ g J B B Taking the difference of these signals leads to a dispersion signal with zero crossing at the B=0 transition B B 0 B B 0 Graham Lochead 03/06/09 Sub-Doppler DAVLL setup Sub-Doppler DAVLL DAVLL To frequency calibration Laser 1 ( ) 2 Metal mirror 4 Coils Differential photodiode 1 ( ) 2 M.L. Harris et al., J. Phys. B. Phys. 41 085401 Graham Lochead 03/06/09 Sub-Doppler DAVLL trace • 3 MHz rms offset stability over an hour Graham Lochead 03/06/09 Sub-Doppler DAVLL characteristics Graham Lochead 03/06/09 Laser locking summary • Polarization spectroscopy is used to lock the 461 nm laser with first cell as offset more stable • These two locking schemes have been characterized and written up • Second cell will be used for thermal Rydberg spectroscopy with pulsed dye laser arXiv:0902.1430v1 [physics.atom-ph] Graham Lochead 03/06/09 • Introduction and motivation • Second generation cell • Polarization spectroscopy and subDoppler DAVLL • Strontium pyramid MOT • 689 nm locking progress Graham Lochead 03/06/09 What is a pyramid MOT? Normal (6 beam) MOT Pyramid MOT K. I. Lee et al., Optics Letters, Vol. 21, Issue 15, pp. 1177-1179 Graham Lochead 03/06/09 Pyramid MOT function Acts as a cold atom source Graham Lochead 03/06/09 Benefits of a pyramid MOT • Size – much smaller than a Zeeman slower • Blackbody radiation effects reduced peak T Graham Lochead 03/06/09 P T4 Chamber design 45 cm Design considerations • Trapping gradient of 30 G/cm • No water cooling • Standard vacuum parts 30 cm Graham Lochead 03/06/09 Mirror mount design Most pyramid MOTs are loaded from background atomic vapour or dispensers above pyramid Problem Low vapour pressure and mirrors get coated Solution • Dispensers below mirrors • Slits where mirrors meet in corners Graham Lochead 03/06/09 The mount design 45 mm Mirror size needs to be small to avoid pumping into meta-stable states Graham Lochead 03/06/09 Atomic beam divergence measurement Expanding lens Atomic beam 4 Laser Collimating lens Light sheet Cylindrical lenses AOM Light sheet Graham Lochead 03/06/09 • Introduction and motivation • Second generation cell • Polarization spectroscopy and subDoppler DAVLL • Strontium pyramid MOT • 689 nm locking progress Graham Lochead 03/06/09 Motivation for 689 nm laser We will use a 532 nm optical lattice laser to add periodic spatial confinement to our MOT Doppler limited temperature TD 2k B 1P 1 3P 1D 2 461 nm /2p = 32 MHz TD ≈ 1 mK 2 689 nm /2p = 7.5 kHz TD ≈ 0.2 μK 1S 0 Graham Lochead 03/06/09 1 0 Pound-Drever-Hall FPD Oscilloscope 2 PS 4 Laser Graham Lochead 03/06/09 Pound-Drever-Hall setup FPD Strontium cell Filter Slow feedback to piezo Fast feedback to diode Feedback to cavity piezo 2 PS 4 Laser Graham Lochead 03/06/09 Slow lock 100k * Ramp 100k 1k PDH signal 10nF 100k 1k 2k 100k * 100 AD620 510 +15V REF02 1k 100k 100k 1k 1k 1k 1k +15V Unlocked laser has linewidth of ~ 600 kHz Locked laser has linewidth of ~ 350 kHz Graham Lochead 03/06/09 To piezo Cavity lock to atomic transition Going to use frequency modulation spectroscopy as laser already modulated AOM Probe 80 MHz 20 kHz 10 MHz Pump Lock in amplifier Cell 4 Feedback to cavity piezo Graham Lochead 03/06/09 Summary and future work • Second cell and locking schemes characterized • Pyramid MOT design • 689 nm locking progress Future work • Build the pyramid MOT • Achieve a red MOT • Load 1-D lattice Graham Lochead 03/06/09 Saturated absorption spectroscopy fit Sat. spec. fit is achieved by minimizing sum of six Lorentzians in Matlab 6 a Fit A I i i 1 ( ( sI is 0 ))2 1 c m 2 ( s) 1% scaling accuracy for the frequency Parameters A s Amplitude of trace Scaling factor ω0 Centre frequency Width c Offset m Gradient of background Isotope Abundance (%) Shift (MHz) Rel. Strength a I F 84Sr 0.56 0 - -270.8 1 86Sr 9.86 0 - -124.5 1 7/2 -9.7 4/15 9/2 -68.9 1/3 11/2 -51.9 2/5 - 0 1 87Sr 88Sr Graham Lochead 03/06/09 I 7.00 82.58 9/2 0 I s