Direct Frequency Comb Spectroscopy for the Study of Molecular Dynamics in the Infrared Fingerprint Region Adam J. Fleisher, Bryce Bjork, Kevin C. Cossel, Jun Ye JILA|NIST and University of Colorado - Boulder Lora Nugent-Glandorf, Florian Adler, Tyler Neely, Scott A. Diddams National Institute of Standards and Technology Tim Dinneen Precision Photonics FA 11 The 67th OSU International Symposium on Molecular Spectroscopy – June 22, 2012 Cavity-Enhanced Direct FCS 1. Mode-locked laser (fs fiber laser) CE-DFCS 2. Sample interrogation (high-finesse enhancement cavity) 3. Dispersive detection system (VIPA) M.J. Thorpe et al. Science 311, 1595 (2006). 1. Mode-locked laser Yb:Fiber Comb Laser >10 W 110 fs 137 MHz 1070 nm T.R. Schibli et al. Nat. Photonics 2, 355 (2008). F. Adler et al. Opt. Lett. 34, 1330 (2009). 1. Mode-locked laser Optical parametric oscillator Tunable from 2.8 – 4.8 μm (2000 – 3500 cm-1) 150 nm bandwidth at 3.75 μm (100 cm-1 fwhm) > 1 W power from 3.0 – 4.0 μm F. Adler et al. Opt. Lett. 34, 1330 (2009). 2. Sample Interrogation High finesse optical cavity with intra-cavity gas sample VIPA spectrometer Mode-locked laser 99.7% < R < 99.95% 1000 < ℱ < 6000 ROC = 6 m d = 0.8″ ZnSe substrate M.J. Thorpe et al. Opt. Express 16, 2387 (2008). A. Foltynowicz et al. Appl. Phys. B. doi:10.1007/s00340-012-5024-7(2012). 3. Dispersive detector MIR VIPA Collectively, these components create a in = 99.95% powerRtool for the sensitive R = out of98.0% measurement absorption spectra over a broadband on the μs timescale InSb photodiode array 320 x 256 pixels LN2 cooled M.J. Thorpe et al. Science 311, 5767 (2006). S.A. Diddams et al. Nature 445, 627 (2007). InSb Camera M.J. Thorpe et al. Opt. Express 16, 2387 (2008). M.J. Thorpe and J. Ye, Appl. Phys. B 91, 397 (2008). VIPA Characterization and Spectroscopy • Measure the VIPA spectrometer resolution and free spectral range – Fabry-Perot Comb Filter Cavity with FSR = 2.0 GHz – Spectroscopy Cavity with FSR = 546 MHz and Finesse = 1200 • Record broadband molecular spectra on the millisecond (ms) timescale – 100 ppm CH4 in N2 at a total pressure of 30 Torr Comb-Cavity Coupling F. Adler et al. Annu. Rev. Anal. Chem. 3, 175 (2010) Construction of Filter Cavity 𝑐 𝐹𝑆𝑅 = = 𝑛 × 𝑓𝑟𝑒𝑝 2𝐿 𝑓𝑟𝑒𝑝 = 136.6 𝑀𝐻𝑧 n FSR (GHz) L (cm) 14 1.91 7.8 15 2.05 7.3 16 2.19 6.9 Exact n value must be know to precisely determine the filtered comb mode spacing required for VIPA calibration. S.A. Diddams et al. Nature 445, 627 (2007). 2.05 GHz Filter Cavity Change in cavity length (L) vs. Change in cavity free spectral range (FSR) L = c / (2FSR) At 15 x frep, the comb line spacing is filtered to 2.05 GHz Center point is 14, 15, or 16 x frep S.A. Diddams et al. Nature 445, 627 (2007). Comb Mode Resolution Detector Image Plane 15° InSb Camera pixels VIPA Dispersion pixels Grating Dispersion Observed FWHM = 600 MHz L. Nugent-Glandorf et al. Opt. Lett., in press (2012). arXiv: 1206.1316 VIPA Performance Calculate FSR at 25° 𝑐 = = 60.3 GHz 2𝑛𝑡 cos 𝜃𝑖 Finesse = 𝜋 = 105, assuming R = 0.97, and lossless front face 1−𝑅 𝐹𝑆𝑅 Resolution = = 60.3 GHz/105 ~ 574 MHz, measured = 600 MHz ℱ Measured FSR at 25° = 55 GHz, therefore ℱ = 92 and R = 0.966 S. Xiao et al. IEEE J. Quant. Elec. 40, 420 (2004). L. Nugent-Glandorf et al. Opt. Lett., in press (2012). arXiv: 1206.1316 Direct FCS Cavity Characterization ℱ = 2𝜋𝜏0 𝐹𝑆𝑅 𝜋 𝑅 ℱ= 1−𝑅 ℱ𝑚𝑎𝑥 = 1200 𝑅𝑚𝑎𝑥 = 99.74% 𝜆 = 3780 𝑛𝑚 𝜐 = 2645 𝑐𝑚−1 Direct FCS Cavity N2 reference 0.2% N2O in N2 at 40 torr Cavity finesse ~1000 Direct FCS Cavity Experimental Frequency Axis Calibrated to HITRAN ax2 + bx +c VIPA 𝜃𝑖 = 25° Wavelength (nm) 2,300 comb modes in the above spectral bandwidth. 1 1 1 R2 ln 1 2 L R 2 1 I I 0 Wavelength (nm) K.C. Cossel et al, Appl. Phys. B, 100, 917 (2010). L.S. Rothman et al. J. Quant. Spectrosc. Radiat. Transfer 96 139 (2005). Molecular Gas Dynamics CH4 gas cell filling dynamics - NIST Noise 5 x 10-4 noise floor (ms) 1 x 10-8 cm-1 (5 avr., 42 ms, 200 m path length) 640 x 512 pixel camera 120 Hz repetition rate L. Nugent-Glandorf et al. Opt. Lett., in press (2012). arXiv: 1206.1316 Future: MIR Reaction Dynamics • • • • • Enhancement factor of ≥ 300 leads to mW/mode of intracavity power 5,000 lasers available for cavity-enhanced spectroscopy 100 cm-1 simultaneous bandwidth Integration time as low as 10 μs (camera limit) Experimental repetition rate of up to 400 Hz (camera limit) Inlet MIR Comb Outlet VIPA and Camera Enhancement Cavity PZT A. Foltynowicz et al. Appl. Phys. B. doi:10.1007/s00340-012-5024-7(2012). L. Nugent-Glandorf et al. Opt. Lett., in press (2012). arXiv: 1206.1316 Acknowledgements Bryce Bjork, Kevin C. Cossel, Jun Ye JILA|NIST and CU Lora Nugent-Glandorf, Florian Adler, Tyler Neely, Scott A. Diddams National Institute of Standards and Technology Tim Dinneen Precision Photonics L. Nugent-Glandorf et al. Optics Letters (2012). arXiv: 1206.1316 Virtually Imaged Phased Array M. Shirasaki Fujitsu Sci. Tech J. 35, 113 (1999). Noise Analysis Insert Citation Here Signal Averaging Single 2ms shot 20 averaged shots 1 FSR Insert Citation Here Frequency Comb Time Domain Frequency Domain ADD SINGLE PULSE VS. PULSE TRAIN IMAGE HERE Frequency comb structure: n nfr f o Cavity mode structure: FSR c d 2L c d Cavity modes Frequency comb Insert Citation Here 1. Mode-locked laser Yb:fiber mode-locked laser OPO >10 W 110 fs 137 MHz 1070 nm T.R. Schibli et al. Nat. Photonics 2, 355 (2008). F. Adler et al. Opt. Lett. 34, 1330 (2009).