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Direct Comb Spectroscopy of Buffer-Gas Cooled Molecules Ben Spaun ISMS, 2015 JILA, NIST and University of Colorado at Boulder.

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Presentation on theme: "Direct Comb Spectroscopy of Buffer-Gas Cooled Molecules Ben Spaun ISMS, 2015 JILA, NIST and University of Colorado at Boulder."— Presentation transcript:

1 Direct Comb Spectroscopy of Buffer-Gas Cooled Molecules Ben Spaun ISMS, 2015 JILA, NIST and University of Colorado at Boulder

2 The Optical Frequency Comb.... f rep f CEO N = f CEO + N x f rep

3 Frequency Comb Applications The Astro-Comb E. Hand, Nature 452, 514 (April 3, 2008). N. Newbury, Nature Photonics 5, 186–188 (2011) Schibli et al. Nature Phonics. (2008) Precision Metrology

4 N. Newbury, Nature Photonics 5, 186–188 (2011) Molecular absorption Comb modes Spectroscopy with an OFC : -Thousands of simultaneous absorption measurements. -Inherent high spectral resolution. -Broad bandwidth. -Long interaction length (when comb is coupled to an optical cavity) Frequency Comb Applications

5 N. Newbury, Nature Photonics 5, 186–188 (2011) From Mid-IR to XUV A Cingöz et al. Nature 482, 68-71 (2012) Frequency Comb Applications

6 Mid-IR OPO Freq. Comb Tunable mid-IR frequency comb Yb:fiber Comb 10W, 1 μm Fan-out PPLN Crystal 2.8-4.8 μm Tunable Comb Light Adler et al. Optics Letters (2009) Beat note Supercontinuum Fiber To f CEO control f rep lock: Cs clock

7 Mid-IR OPO Freq. Comb Cavity-Enhanced Direct Comb Spectroscopy High-refl. mirror Broadband, high-reflectivity cavity mirrors: Finesse > 6000 Over 100 nm of comb spectrum coupled through cavity f rep

8 Mid-IR OPO Freq. Comb Cavity-Enhanced Direct Comb Spectroscopy High-refl. mirror

9 Mid-IR OPO Freq. Comb Cavity-Enhanced Direct Comb Spectroscopy High-refl. mirror Scan comb f rep to ensure that no absorption features are skipped over. f rep Molecular absorption

10 Mid-IR OPO Freq. Comb Cavity-Enhanced Direct Comb Spectroscopy High-refl. mirror FTIR Spectrometer wavelength (  m) 3.0 3.23.1 Fast scanning Michelson interferometer provides singe comb-mode resolution

11 Applications and Limitations Applications: Trace-gas detection (e.g. breath analysis) -- sensitivity down to ppb demonstrated for multiple molecules Isotopic analysis Tomography of super-sonic jet -- a complete spatial mapping of density, velocity, and temperature Methane Frequency (cm -1 )

12 Methane Frequency (cm -1 ) Applications and Limitations Applications: Trace-gas detection (e.g. breath analysis) Isotopic analysis Tomography of super-sonic jet Limitations: Spectral congestion makes more complex molecules unresolvable at room temp: Doppler width > line spacing Nitrous Oxide Isoprene

13 T = 300 K Cooling molecules below 10 K: Simplifies spectra since only lowest rotational levels are populated Reduces Doppler linewidth by at least factor of 5 Nitromethane (CH 3 NO 2 ) Frequency (cm -1 ) 2954.2 2954.42954.62954.8 Absorption Simplify spectra by cooling molecules T = 150 K T = 50 K T = 8 K

14 Mid-IR OPO Freq. Comb Add buffer-gas cell inside cavity High-refl. mirror FTIR Spectrometer 300 K 35 K 8 K Molecules He Buffer Gas Edge-welded bellows D. Patterson & J. M. Doyle. Molecular Physics (2012)

15 Buffer Gas Cell (8K) Cavity Mirror and Piezo Cavity Mirror Molecule Inlet Mechanical Isolation (Bellows) Mid-IR Comb Light to FTIR Stainless Steal Cavity Structure Apparatus

16 3 + 6 (sym + asym NO stretch) 1 (sym CH stretch) 2974.63 2974.71 2974.69 2974.67 2974.65 0.06 0.08 0.04 0.02 0 10 (asym CH stretch) Fractional Absorption 0.3 0.2 0.1 0 3050 2960 2990295029402970 2980 3090306030703080 Frequency (cm -1 ) CH 3 NO 2 is a model system for large amplitude motion & internal rotation First high resolution (30 MHz Doppler-limited) spectra of the CH stretch region: >1000 transitions observed in three vibrational bands (2940-3090 cm -1 ) Nitromethane spectrum near 3.3  m

17 Resolving DC Stark shifts High resolution allows unique Stark- shift signatures to be identified: Excited torsional states (|m|=1,2) split symmetrically in applied E-field Energy E-field m = +1 m = -1 m = 0 E-field = 0 V/cm E-field = 400 V/cm

18 Resolving DC Stark shifts High resolution allows unique Stark- shift signatures to be identified: Excited torsional states (|m|=1,2) split symmetrically in applied E-field Closely spaced opposite parity states mix to allow for new transitions Energy E-field E-field = 0 V/cm E-field = 400 V/cm E-field = 0 V/cm E-field = 400 V/cm

19 Resolving DC Stark shifts Grouping lines based on Stark-shift signatures simplifies line assignment process Successfully assigned most lines in ν 3 +ν 6, including many excited torsional transitions.

20 Observed perturbations in ν 3 +ν 6 Interactions with dark states are indicative of intramolecular (ro)vibrational coupling Mixed bright + dark state

21 Conclusion Buffer-gas cooling has been successfully integrated with cavity-enhanced direct frequency comb spectroscopy. Over 1000 nitromethane absorption lines spanning multiple vibrational bands in the mid-IR have been observed for the first time. Line assignment process simplified by resolution of small (10-100 MHz) DC-stark shifts. Outlook: probe larger molecules and search for molecule clusters.

22 Acknowledgments Bryan Changala, Bryce Bjork, Oliver Heckl, Jun Ye JILA|NIST and CU David Patterson and John Doyle Harvard University Physics Dept.


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