Cavity decay rate in presence of a SlowLight

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Cavity decay rate in presence of a Slow-Light medium Laboratoire Aimé Cotton, Orsay, France

Cavity decay rate in presence of a Slow-Light medium Laboratoire Aimé Cotton, Orsay, France Thomas Lauprêtre Fabienne Goldfarb Fabien Bretenaker School of Physical Sciences, Jawaharlal Nehru University, Delhi, India Rupamanjari Ghosh Santosh Kumar Thales R&T, Palaiseau, France Sylvain Schwartz 1

Outline • • • Issues: the ring laser gyro EIT and dispersion Experimental set-up

Outline • • • Issues: the ring laser gyro EIT and dispersion Experimental set-up Cavity decay rate Negative dispersion in He* 2

Inertial navigation Problem: allow a vehicle to know its attitude and position at any

Inertial navigation Problem: allow a vehicle to know its attitude and position at any moment by knowing only the coordinates of its starting point and using internal ax measurements only. ? Start Wx Wy Wz az ay Solution: continuously measure three linear accelerations and three angular velocities. Error smaller than 1 nautical mile per hour: Drift of the gyros < 0. 01 °/hour (Earth rotation≈ 15 °/ hour) Till the 1960’s: undisputed reign of mechanical gyros! 3

Sagnac effect CCW Wave O O’ W R = 0. 1 m et Ω

Sagnac effect CCW Wave O O’ W R = 0. 1 m et Ω = 0. 01 °/h L+- L- = 4πR 2Ω/c Δφ < 1 nanoradian 4

Principle of the ring laser gyro CCW Modes W Dn n CCW Wave CW

Principle of the ring laser gyro CCW Modes W Dn n CCW Wave CW Modes Gain medium c/L CW Wave 5

Dispersion in cavity Positive dispersion reduces the linewidth of a resonator Þ Could dispersion

Dispersion in cavity Positive dispersion reduces the linewidth of a resonator Þ Could dispersion enhance sensitivity of cavity based sensors? 6

Cavity filled with a dispersive medium Cavity resonance condition: Sagnac effect: with W with

Cavity filled with a dispersive medium Cavity resonance condition: Sagnac effect: with W with Dispersive medium If , Sensitivity 7

Ring laser gyro The fundamental noise is given by the Schawlow-Townes linewidth of the

Ring laser gyro The fundamental noise is given by the Schawlow-Townes linewidth of the laser: Lifetime of photons in the cavity 8

Lifetime of photons • 2 different points of view Δt 1) Phase velocity Resonant

Lifetime of photons • 2 different points of view Δt 1) Phase velocity Resonant cavity: monochromatic field 2) Group velocity ÞGaussian pulse ÞΔt ∞ ? 9

Sensitivity? • Lifetime driven by phase velocity: Scale factor: Þ Scale factor increased and

Sensitivity? • Lifetime driven by phase velocity: Scale factor: Þ Scale factor increased and noise unchanged gain on sensitivity But • Lifetime driven by group velocity Linewidth: Þ Scale factor increased so is the noise no gain on sensitivity How does the cavity photons lifetime tcav depend on dispersion ? 10

Outline • • • Issues: the ring laser gyro EIT and dispersion Experimental set-up

Outline • • • Issues: the ring laser gyro EIT and dispersion Experimental set-up Cavity decay rate Negative dispersion in He* 11

Electromagnetically Induced Transparency ? • Fact: Optical transition is made transparent for a resonant

Electromagnetically Induced Transparency ? • Fact: Optical transition is made transparent for a resonant field (otherwise opaque medium) • How it happens: A quantum interference effect, induced by a control field applied on a second transition 12

One optical transition Λ system Induced WidthÞ of. Electromagnetically transparency window Transparency (EIT) 13

One optical transition Λ system Induced WidthÞ of. Electromagnetically transparency window Transparency (EIT) 13

EIT and Slow Light • Kramers-Kronig Slow Light ! Strong positive dispersion Kash &

EIT and Slow Light • Kramers-Kronig Slow Light ! Strong positive dispersion Kash & al, PRL, 1999: 90 m. s-1 in Rb Hau & al, Nature, 1999: 17 m. s-1 in cold Na 14

Outline • • • Issues: the ring laser gyro EIT and dispersion Experimental set-up

Outline • • • Issues: the ring laser gyro EIT and dispersion Experimental set-up Cavity decay rate Negative dispersion in He* 15

Metastable 4 He m= -1 wp 0 s+ Wp 1 d s- 3 P

Metastable 4 He m= -1 wp 0 s+ Wp 1 d s- 3 P 1 3 S 1 wc Wc RF discharge 1 S 0 • Lifetime ~8000 s Þ polarization selected Λ system 16

Room temperature 4 He* • Spin conservation through collisions with He M. Pinard and

Room temperature 4 He* • Spin conservation through collisions with He M. Pinard and F. Laloë, J. Physique 41 799 (1980) • Almost no Penning ionization (thanks to optical pumping) Shlyapnikov & al, PRL 73 3247 (1994) No loss of coherence time 17

Benefits of collisions • Possibility to pump over the entire Doppler width through Velocity

Benefits of collisions • Possibility to pump over the entire Doppler width through Velocity Changing Collisions (VCCs) • Atoms are confined into the laser beam (diffusive transit instead of ballistic transit) - Increase of coherence time - Co-propagating beams 18

EIT and optical detuning ÞFano profile B. Lounis and C. Cohen-Tannoudji, J. Phys. II

EIT and optical detuning ÞFano profile B. Lounis and C. Cohen-Tannoudji, J. Phys. II (France) 2, 579 (1992) 19

Doppler broadening • Sum of all profiles over the Doppler width d. R 3

Doppler broadening • Sum of all profiles over the Doppler width d. R 3 P 1 ~1 GHz Coupling Wc ~ ~ Probe Wp 3 S 1 Where WD is the half linewidth of the Doppler profile 20

Experimental set-up 21

Experimental set-up 21

Im(χ) (a. u. ) Width at half maximum (k. Hz) Experimental results Group delay

Im(χ) (a. u. ) Width at half maximum (k. Hz) Experimental results Group delay (µs) Raman detuning (k. Hz) Coupling intensity (W. m -2) Þ Group velocity around 8 km. s-1 ! Goldfarb, F. & al. , EPL (Europhysics Letters), 2008, 82, 54002 Coupling intensity (W. m -2) Ghosh, J. & al. , Phys. Rev. A, 2009 22

Outline • • • Issues: the ring laser gyro EIT and dispersion Experimental set-up

Outline • • • Issues: the ring laser gyro EIT and dispersion Experimental set-up Cavity decay rate Negative dispersion in He* 23

EIT inside a cavity: set-up Laser & Beam Shaping λ/2 PBS AO 2 PZ

EIT inside a cavity: set-up Laser & Beam Shaping λ/2 PBS AO 2 PZ ωP , Ω P ωC , Ω C Telescope Shutter PBS PD T=2% AO 1 4 He* cell PBS T=2% 24

Experiment 25

Experiment 25

Global results Decay time of the cavity Group delay introduced by the cell (open

Global results Decay time of the cavity Group delay introduced by the cell (open cavity) • Measured decay time ~ a few µs • ~150 ns with phase velocity Group velocity ! 26

Cavity decay rate T. Lauprêtre, C. Proux, R. Ghosh, S. Schwartz, F. Goldfarb, and

Cavity decay rate T. Lauprêtre, C. Proux, R. Ghosh, S. Schwartz, F. Goldfarb, and F. Bretenaker « Photon lifetime in a cavity containing a slow-light medium » Accepted by OL • Non monochromatic field ÞGroup velocity 27

Cavity decay rate • Consequences on the fundamental noise of laser cavity based sensors?

Cavity decay rate • Consequences on the fundamental noise of laser cavity based sensors? Increase of Δν 28

Negative dispersion in cavity • Lifetime ? Δt Vg>0 29

Negative dispersion in cavity • Lifetime ? Δt Vg>0 29

Negative dispersion in cavity • Lifetime ? Δt Vg<0 30

Negative dispersion in cavity • Lifetime ? Δt Vg<0 30

Outline • • • Issues: the ring laser gyro EIT and dispersion Experimental set-up

Outline • • • Issues: the ring laser gyro EIT and dispersion Experimental set-up Cavity decay rate Negative dispersion in He* 31

Negative dispersion • Optical detuning : asymmetry of the absorption profile Doppler width ~1

Negative dispersion • Optical detuning : asymmetry of the absorption profile Doppler width ~1 GHz Coupling Wc Δ ~ d. R 3 P 1 ~ Probe Wp 3 S 1 Narrow absorption peak of small amplitude Þ Negative dispersion 32

Negative group velocity Doppler width d. R ~1 GHz ~ 3 P 1 ~

Negative group velocity Doppler width d. R ~1 GHz ~ 3 P 1 ~ Probe Wp 3 S 1 Group delay (µs) Coupling Wc Δ Raman detuning (k. Hz) 33

Conclusion • Decay rate of a cavity filled with a strong positive dispersion medium

Conclusion • Decay rate of a cavity filled with a strong positive dispersion medium is governed by the group velocity • Negative group velocity? 34

Advertisment Poster session: Tu-P 15 S. Kumar, T. Lauprêtre, F. Bretenaker, R. Ghosh, and

Advertisment Poster session: Tu-P 15 S. Kumar, T. Lauprêtre, F. Bretenaker, R. Ghosh, and F. Goldfarb Interacting dark resonances in a tripod system of room temperature 4 He* 35

Thank you! 36

Thank you! 36