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Non-ideal Cavity Ring-Down Spectroscopy: Linear Birefringence, Linear Polarization Dependent Loss of Supermirrors, and Finite Extinction Ratio of Light.

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Presentation on theme: "Non-ideal Cavity Ring-Down Spectroscopy: Linear Birefringence, Linear Polarization Dependent Loss of Supermirrors, and Finite Extinction Ratio of Light."— Presentation transcript:

1 Non-ideal Cavity Ring-Down Spectroscopy: Linear Birefringence, Linear Polarization Dependent Loss of Supermirrors, and Finite Extinction Ratio of Light Modulator Haifeng Huang and Kevin K. Lehmann Chemistry Department, University of Virginia 63rd International Symposium on Molecular Spectroscopy Columbus OH, June 20, 2008

2 Cavity ring-down spectroscopy
(mV) Laser Cavity Modulator Detector Absorption enhancement:

3 Experimental setup Lens He-Ne laser DFB diode laser
Laser control board AOM AOM driver Detector Isolator Computer 3PZTs Flat mirror Curved mirror Mode matching optics Cavity Trigger signal Isolator Polarizer or Pockel’s cell λ/2 plate

4 Two polarization eigenmodes
There exist two special angles of the analyzer, perpendicular with each other, at which we have the lowest noise level of τ. Cavity is excited by circular polarization light, but these two angles are independent of the polarization of the incident light.

5 Cavity under vacuum Low stress conditions: 760 torr and tightening screws loosened (front mirror)

6 Polarization dependent loss (PDL) (Linear dichroism)
Cavity under vacuum Back mirror at 7 degree Two modes: 2.5 and 92.5 degree Cavity under vacuum Back mirror at -53 degree Two modes: 14 and 104 degree

7 PDL with back mirror rotation
Δτ τ strongly depends on local conditions (e.g. defects) of mirrors. The incident polarization angle of max τ changes more smoothly.

8 Physical picture diagram
Slow Axis Fast Axis r1max r2max r1min r2min α1 β1 β2 α2 x y z HR coating Waveplate AR coating Laser Single pass phase retardance: ε1 and ε2

9 The model Jones matrices for reflection and wave plate transmission:
Round trip Jones matrix with linear approximation: Round trip net PDL parameters and birefringence values:

10 The Model (continued) Two eigenvalues:
Frequency splitting of two modes: Decay time constant: τ versus Incident polarization direction: Two polarization eigenvectors are no longer orthogonal, but almost perpendicular with each other and almost linearly polarized. Both polarization directions can be calculated from M.

11 Cavity under vacuum Back mirror at ~56 degree, both slow (fast) axes parallel Cavity under low stress conditions Back mirror at ~36 degree, the slow (fast) axis of it is along the x axis.

12 Polarization dependent loss (Linear dichroism)
Cavity under vacuum Back mirror at 7 degree Two modes: 2.5 and 92.5 degree Cavity under vacuum Back mirror at -53 degree Two modes: 14 and 104 degree

13 PDL and back mirror rotation
The main axis direction of polarization dependent loss is less localized.

14 Depolarization and stress
♣ cavity under vacuum ♣ 700 torr, tightening screws not loosened (front mirror) ♣ low stress conditions: 760 torr and all tightening screws loosened (front mirror) Back mirror at 62 degree

15 Noise from light leakage
Decay amplitude: 1.5V Detector noise: 2mV Extinction ratio: 20dB Fitting residue of one decay

16 50dB is not enough! Detector noise limited CRDS
Noise from light leakage, laser always on resonant K. K. Lehmann and H. Huang, Frontiers of Molecular Spectroscopy, chapter 18, Elsevier 2008

17 Noise vs. extinction ratio

18 Conclusions ■ Linear birefringence (10-7~10-6 rad) of supermirrors will lift the polarization degeneracy of TEM00 mode, generating two new polarization eigenmodes with frequency splitting ~0.1 kHz. These two modes are almost linearly polarized. ■ For the first time, we reported the linear polarization dependent loss (~10-8) of supermirrors. The results can only be explained by including both factors. ■ Birefringence of supermirrors can be reduced greatly by releasing the stress on both mirrors. ■ Finite extinction ratio of the light modulator can cause significant noise in CW-CRDS signal. For signal of S/N about 1000, 70 dB extinction ratio is needed in order to reach the noise limit. H. Huang & K. K. Lehmann, Applied Optics, accepted H. Huang & K. K. Lehmann, in preparation

19 Acknowledgements Paul Johnston and Robert Fehnel
Dr. Brooks Pate’s Lab in UVA

20 AOM extinction ratio RF on RF off RF amplifier RF oscillator 80 MHz
Trigger signal Switch 1 Switch 2 RF In 2 1 Attenuator 20 dB Step attenuator 0 – 69 dB Combiner 1512 nm laser diode Optical fiber 0th order 1st order to cavity AOM crystal Isolator Output coupler TTL RF on RF off


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