Progress towards laser cooling strontium atoms on the intercombination transition

Preview:

DESCRIPTION

Progress towards laser cooling strontium atoms on the intercombination transition. Danielle Boddy Durham University – Atomic & Molecular Physics group. The team. Progress towards laser cooling strontium atoms on the intercombination transition - May 2011. Motivation: Rydberg physics. - PowerPoint PPT Presentation

Citation preview

Progress towards laser cooling strontium atoms on the

intercombination transition

Danielle BoddyDurham University – Atomic & Molecular Physics group

The team

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Motivation: Rydberg physics Ionization

threshold

Ener

gy

States of high principal quantum number n.

Exaggerated size and lifetimes.

Can be prepared through laser excitation.

Greatly enhanced inter-atomic interactions.

Strong, tunable, long-range dipole-dipole

interactions among the atoms.

Applications include quantum computation. M. Saffman et. al., Rev. Mod. Phys. 82, 2313 (2010)

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Motivation: Dipole blockade

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Y Miroshnychenko et al., Nat. Phys. 5, 115-118 (2009)E Urban et al., Nat. Phys. 5, 110-114 (2009)

Sr88 is an alkaline earth metal with no hyperfinestructure.

Two valence electrons permits two electron excitation.

Motivation: An introduction to strontium

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Ground state

Rydberg state

Doubly excited state

Two-electron excitation of an interacting cold Rydberg gas J. Millen, G. Lochead and M. P. A. Jones Phys. Rev. Lett. 105, 213004 (2010)

Spectroscopy of strontium Rydberg states using electromagnetically induced transparency S. Mauger, J. Millen and M. P. A. Jones J. Phys. B: At. Mol. Opt Phys. 40, F319 (2007)

At present, we’re investigating the spatial excited state distribution.

Motivation: Dipole blockade regime

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

rB

T ~ 5 mKDensity ~ 1 x 109 cm-3

T ~ 400 nKDensity ~ 1 x 1012 cm-3

No blockade

How do we enter the dipole blockade regime?

Blockaded

Motivation: Laser cooling of strontium

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

1P1

3P0

3P1

3P2

1S0

λ = 689 nmΓ = 2π x 7.5 kHz2nd stage cooling

λ = 461 nmΓ = 2π x 32

MHz1st stage cooling

1S0 → 3P1 intercombination transition → TD ≈ 180 nK.

Photon recoil limits TD → Tmin ≈ 460 nK.

Introduce two stages of cooling:

First cool on the (5s2) 1S0 → (5s5p) 1P1.

Second cool on the narrow-line (5s2) 1S0 → (5s5p) 3P1 .

Outline

Simple laser stabilization set-up

Laser system

Pound-Drever-Hall (PDH)

Locking to an atomic transition

Fluorescence

Electron shelving

Summary

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Simple laser stabilization set-up

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Laser system

Fabry-Perot

cavity

Atomic signal

Red MOT

Simple laser stabilization set-up

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Laser system

Fabry-Perot

cavity

Atomic signal

Red MOT

Laser system

Laser system

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Compared old and new designs.

Laser system

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

time

frequency

OLD

NEW2 Wavemeter

10 s

1

10 s

OLD

NEW

Wavemeter1

time

frequency2

Laser system

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Old New

New design fluctuates more in the short term.Little difference between the long term stability.

Simple laser stabilization set-up

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Laser system

Fabry-Perot

cavity

Atomic signal

Red MOT

Fabry-Perot

cavity

Pound-Drever-Hall (PDH) technique

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Require the laser linewidth < 7.5 kHz.

Noise broadens the linewidth to the MHz regime.

Uses Fabry-Perot cavity as a frequency reference.

Cavity peaks are spaced by the free spectral range :

Lc

FSR 2

Pound-Drever-Hall (PDH) technique

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Phase modulator adds sidebands to the laser.

High-finesse Fabry-Perot cavity measures the time-varying frequency of the laser input.

An electronic feedback loop works to correct the frequency error and maintain constant optical power.

Laser

Phase modulato

r

FPD

Lock Box

Etalon4

PiezoCurrent

modulation

Theory: See E. Black., Am. J. Phys. 69 (1) 79 (2001)

Pound-Drever-Hall (PDH) technique

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

4

FPD

PS

2

Slow feedback to

piezo

Fast feedback to

diode

Feedback to cavity piezo

Atomic signal

Laser

2

Lock Box

A crystal oscillator phase modulates the 689 nm beam at a frequency of 10 MHz.

Pound-Drever-Hall (PDH) technique

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Laser locks to the central feature of the PDH error signal

Increasing the gradient of the error signal strengthens the lock and reduces the linewidth.

(a) (b) (c) (d)

Gradient depends on sideband power: carrier power ratio.

Gradient steepest when Ps = 0.42 Pc

Theory: See E. Black., Am. J. Phys. 69 (1) 79 (2001)

Pound-Drever-Hall (PDH) summary

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Generate PDH signal

Gradient of error signal → strength of lock and laser linewidth

NEXT STEP: Finish high bandwidth servo

IMPROVEMENTS: Build high-finesse cavity

Simple laser stabilization set-up

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Laser system

Fabry-Perot

cavity

Atomic signal

Red MOT

Atomic signal

Locking to an atomic transition

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

CHALLENGE: Detecting the transition.

Two detection methods:

1. Electron Shelving

2. Fluorescence

Electron shelving

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Excite atoms to the 3P1 and measure the rate at which these atoms decay out of the state.

Photon scattering rate is proportional to the linewidth of the transition.

1P1

3P1

1S0

λ = 689 nm

λ = 461 nm

Electron shelving

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

1P1

3P1

1S0

λ = 461 nm

atomic beam

photodiode

The amount of scattered light is proportional to the

number of atoms initially in the 1S0 ground state.

Electron shelving

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

1P1

3P1

1S0

λ = 689 nm

λ = 461 nm

atomic beam

photodiode

Electron shelving: Experiment

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

atomic beam

photodiode

Electron shelving: Experiment

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

atomic beam

photodiode

Electron shelving: Experiment

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

atomic beam

photodiode

Electron shelving: Experiment

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

≈ 32 MHz

Electron shelving: Lifetime measurement

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Using a velocity of 500 ms-1

Lifetime of 3P1 is (23 ± 1) μs

Gradient: (8.9 ± 0.2) x 10-2 mm-1

Electron shelving: Crossed beams

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

atomic beam

photodiode

FWHM crossed beams is ≈ 20 MHz.Linewidth has reduced by 1/3.

This is not narrow enough for the Fabry-Perot to lock to!

Electron shelving: Summary

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Detected the transition indirectly via electron shelving.

Determined the lifetime of the 3P1 state.

And the lineshape?

Tried crossing the beams:

Did the linewidth reduce? Is this narrow enough for the laser to lock to?

Work in progress

Try a direct method of detection.

Fluorescence: The experiment

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Strontium has negligible vapour pressure at room temperature → heated to 900 K.

atomic beam

CCD camera takes spatially resolved images of the fluorescence.

Exposure length set to 65.5 ms.

Fluorescence: The experiment

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

(a) Slice along direction of laser beam → absorption and decay.

(b) Slice along direction of atomic

beam → transverse velocity distribution.

(b)(a)

Fluorescence: The experiment

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Gradient: (9.0 ± 0.3) x 10-2 mm-1

Using a velocity of 500 ms-1

Lifetime of 3P1 is (22.2 ± 0.7) μs

Other time resolved fluorescence detection: τ = (21.3 ± 0.5) μs See R Drozdowski., Phys. D. 41:125 (1997)

Fluorescence: The experiment

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

BUT what about the absorption?

Fluorescence: The model

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Solves optical bloch equations (OBEs) for a two level atom as a function of

distance.

Velocity distribution of atoms α Tk

mv

Bev 23

2

)(vf

Randomly selects a value of and .

If the value of is kept.

)(vf 'v

)'()( vfvf 'v

Fluorescence: The model

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

x

Assuming the laser is on resonance the only other unknown in the OBEs is

the Rabi frequency.

Top hat pulse: Ed.

x

Gaussian pulse: 2

2)(2. waistwaistx

eEd

Fluorescence: The model

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

0 .0 002 0 .0 004 0 .0 006 0 .00 08 0 .0 010 0 .00 12D istan cem0 .2

0 .4

0 .6

0 .8

1 .0

E xci ted po pu lat io n state 22

Top hat pulse Gaussian pulse

Velocity of 500 ms-1

Fluorescence: The model

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

0 .00 1 0 .00 2 0 .0 03 0 .00 4 0 .00 5 0 .0 06D is tancem0 .1

0 .2

0 .3

0 .4

0 .5

0 .6

0 .7

E xcited pop u lat ion state 22

0 .001 0 .0 02 0 .003 0 .00 4 0 .00 5 0 .00 6D is tancem0 .2

0 .4

0 .6

E xcited po pu latio n state 22

2 x waist

Fluorescence: Summary

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Detected the transition directly.

Determined the lifetime of the 3P1 state.

Written code to model absorption and decay.

Data and theory don’t quite agree.

NEXT: Try locking to this fluorescence signal.

Need to find source of problem.

Summary

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

689 nm laser built and tested.

Need to finish PDH high bandwidth servo circuit.

Build high-finesse cavity.

Tested an indirect and direct method to detect the transition.

Measured lifetime of 3P1 state from both methods.

Try locking to fluorescence signal.

If this works….GREAT!

If it doesn’t work….try pump-probe spectroscopy

Red MOT → colder atoms

Questions?

Progress towards laser cooling strontium atoms on the intercombination transition - May 2011

Thanks for listening Any questions?

Recommended