|Home | About | Journals | Submit | Contact Us | Français|
Supercontinua generated in highly non-linear fibers by ultrashort-pulse lasers can be used for high resolution Fourier transform absorption spectroscopy. The practical advantages of these bright ultrabroadband light sources for spectroscopy in the near-infrared region are reported. A Cr4+:YAG femtosecond laser broadened by an extruded soft-glass photonic crystal fiber, emitting from 1200 to 2200 nm and from 675 to 950 nm, provides a spectral radiance being 1·105 times higher than that of a 3000 K blackbody and 102 times higher than that of a synchrotron radiation. The C2H2 and NH3 overtone spectra are recorded using this source within a few seconds.
Bright, coherent and broadband radiation brings a number of advantages for high resolution spectroscopy, so that several facilities are, for instance, presently using - or planning to use - synchrotron radiation for gas phase spectroscopy . As a much simpler table-top low-cost alternative, femtosecond (fs) mode-locked lasers and optical parametric oscillators represent the first versatile coherent sources providing broad bandwidth and high brightness. Several spectroscopic methods using fs mode-locked lasers are currently being implemented. Most of them make use of multichannel grating spectrometers [2,3], which limit the resolution and applicable spectral domains. Multiplex spectroscopy does not meet these restrictions and various approaches have been successfully demonstrated [4-7], in particular in the infrared where detector arrays for multichannel recording are expensive or inexistent. These approaches are rather easy and cheap to be put in practice with commercial and laboratory instruments widely used in chemistry and physics. However, their full potential is currently limited by the narrow spectral range of available fs sources in the infrared. The supercontinuum (SC) generation may be a convenient and inexpensive way to overcome this restriction.
SC can be conveniently generated from femtosecond lasers or any high energy pulsed lasers when launched into nonlinear optical fibers. In particular, Photonic Crystal Fibers (PCF) have permitted more than one octave spectral broadening in the near-infrared and visible . Currently, SC is boosting several fields like frequency metrology, pulse compression and optical coherence tomography. Its application to optical gas monitoring is presently restricted to wavelength agile methods [9-11]. Multiplex Fourier Transform (FT) spectroscopy is an interesting opportunity to benefit from these broad sources for high accuracy and high sensitivity gas phase spectroscopy. The aim of this paper is to show that SC may be fully taken advantage of in multiplex spectroscopy and to illustrate the SC potential for high resolution FT spectroscopy on the example of a SC generated in a highly nonlinear fiber coupled to a 1.5 μm fs laser.
The experimental setup is shown in Fig 1. A chirped-mirror-controlled Cr4+:YAG oscillator , pumped by a Nd:YVO4 laser, is modelocked by a commercial SESAM (BATOP Mod. SAM-1550-1). It is operated in the chirped-pulse positive dispersion regime . In this regime, details of which are described elsewhere , the laser emits positively chirped 1.4 ps pulses centered at 1525 nm with a repetition rate of 142 MHz and 100 mW average power. These pulses are compressed down to 120 fs in a 3.2 m piece of a standard SMF28 single mode silica fiber, and launched into the nonlinear fiber with about 550 pJ input energy. We have tested several kinds of nonlinear fibers, including dispersion-shifted germanium-doped silica fibers (DSF) and PCFs. The most effective broadening has been obtained with a 40-cm long PCF made of SF6 glass  in which the light, launched with an efficiency of about 32%, is guided through a 4.5 μm-diameter solid core with nonlinear index n2 = 2.2×10−15 cm2.W−1, surrounded by a periodic arrangement of air holes. After recollimation, the SC beam has about 25 mW average power and propagates through a single-pass 70-cm-long absorption sample cell. The beam is attenuated and analyzed by a commercial rapid-scan FT spectrometer (Bruker IFS66) just as a steady-state source.
The achieved spectral broadening is shown on Fig. 2 at low resolution (50 cm−1 - ca. 10 nm). The spectral domain of the laser emission itself (without broadening) extends over 200 nm at −30 dB level. In the high resolution spectra reported below, this 30 dB attenuation corresponds to the limit beyond which no spectroscopic data are measurable. At the PCF output, the spectrum extends in the infrared over about 1100 nm, from 1200 (8330 cm−1) to 2200 nm (4545 cm−1) at −30 dB level, and in the visible-very near infrared over about 275 nm, from 675 (14815 cm−1) to 950 nm (10525 cm−1) at −30 dB level. This broadening is consistent with previous experimental data [15-18] on the same type of fiber with different core sizes and various seeding sources.
Each high resolution (3.6 GHz - 0.12 cm−1) spectrum of the PCF output, is recorded in just 13.1 s. It is made of 67290 independent useful spectral elements covering 1375 nm (8075 cm−1), with a maximum signal to noise ratio (SNR) about 2400. At this resolution, we observe fringes that scramble the spectral information. Their origin is not completely clear: they do not seem to be due to birefringence from the PCF as rotating the input light polarization has no effect. They are however specific to the employed PCF, because the SC generated in a single mode DSF is fringe-free. We believe that these fringes are due to the mode beating in the multimode PCF that could not be observed previously due to insufficient resolution . The good short-term stability made it possible to suppress the fringes by dividing the spectra with and without gas inside the absorption cell. Since the broadening was much stronger in the multimode PCF, we decided to use it to test the SC potential for high resolution spectroscopy, trading the slightly degraded SNR against the larger bandwidth.
As a first demonstration, C2H2 and NH3 spectra are recorded. Figure 3 shows a portion of the acetylene absorption spectrum at two different pressures: 28 and 160 hPa, between 1511 and 1548 nm (6620-6460 cm−1) at 3.6 GHz (0.12 cm−1) resolution. All absorption lines displayed in Fig. 3 are due to acetylene. The most intense band is the ν1+ν3 band of 12C2H2. The rotational lines from the P and R branches of the ν1+ν3+ν41−ν41 and ν1+ν3+ν51−ν51 hot bands of 12C2H2 and the ν1+ν3 cold band of 12C13CH2 are also observed. The ammonia spectrum is shown on the lower trace of Fig.4 at 15 GHz (0.50 cm−1) resolution. The region of the ν2+ν3+ν4 band of NH3 is observed. The spectrum is complex and crowded and to our knowledge, no rotational assignment is available in the literature. For comparison, the upper trace provides a portion of spectrum recorded with a tungsten lamp, which is the most widely used white source in near-infrared absorption FTS. The SNR of this reference spectrum is about 1.7 times better than the SC spectrum, but the recording time is 200 times longer. With the same recording time as with the tungsten lamp, the SNR of the SC spectrum would have been 33 000. One advantage of SC sources is their high spectral radiance, which for the present 25 mW SC source equals 2.8×107 W.m−2.sr−1.nm−1. It is 1×105 times stronger than a tungsten lamp comparable to a 3000 K black body source. A SNR enhancement of about 350 could have then been achieved. This was actually not possible: the detector was saturated by the 25 mW laser beam and a power attenuation by more than one order of magnitude before entering in the interferometer was necessary. On the other hand, tungsten lamps have a flat spectrum, which enables to benefit from the whole spectrum. The SC sources can also be optimized to provide smooth broad spectra by using shorter nonlinear fibers and fs sources with higher pulse energy [8,19], which would further improve their applicability for spectroscopic measurements.
It is also informative to compare the potential of SC sources with the performance of the synchrotron radiation. The expected brightness  of the infrared beamline at the French facility Soleil is 1019 photons/s/1% of BW/mm2.steradian for the near infrared (1 μm), which converts into a spectral radiance equal to 2×105 W.m−2.sr−1.nm−1. This is two orders of magnitude weaker than the present SC, which can still be improved in terms of output power and spectral coverage. Moreover, since such SC source is a table-top device made of commercially available parts, it could even be incorporated into industrial instruments.
Presently the wavelength agile techniques are the fastest gas monitoring methods using the SC sources at comparable resolution [9-11]. They, however, feature frequency-dependent spectral resolution and require long fibers as dispersers, that currently limit their applicability to the telecom bands and involve detectors with GHz bandwidth. A FT spectrometer requires longer acquisition times, seconds instead of milliseconds, but is much more appropriate for accurate measurements of spectroscopic interest. The FT spectral resolution may be improved easily up to 30 MHz, the accuracy in the wavenumber scale may reach 10−9, and several millions of spectral elements may be measured in a single experiment, resulting in spectra spanning more than one octave. In addition, SC can be implemented with the frequency comb spectrometric approach that we reported recently with a mode-locked laser , which enhances sensitivity and enables simultaneous recording of broadband absorption and dispersion spectra.
In this article, supercontinuum femtosecond laser systems are demonstrated to be powerful high-brightness sources for high resolution spectroscopy. The corresponding accurate analysis may be well performed by FT spectrometers over the whole emission range. SC sources become commercially available in the visible and near-infrared ranges and they may be easily implemented on the basis of existing spectroscopic instruments. The development of a table-top ultrabroadband coherent source in the mid/far-infrared should significantly impact the practical applications of spectroscopy, and SC generated by chalcogenide or fluoride fibers  could likely be an efficient approach.
O. Okhotnikov (Tampere University of Technology) is warmly thanked for providing the samples of nonlinear Ge-doped fiber, P. Jacquet (Laboratoire de Photophysique Moléculaire, Orsay) for his participation and M. Hanna (Laboratoire Charles Fabry de l'Institut d'Optique) for useful advices. Efficient technical support was provided by J. Caillaud. I.T Sorokina acknowledges an Invited Professor position with Université Paris-Sud. The Programme Pluri-Formation de l'Université Paris-Sud “Détection de traces de gaz” and the Austrian Fonds zur Förderung der wissenschaftlichen Forschung (project P17973) have funded this work.
OCIS codes: 190.4370 Nonlinear optics, fibers; 060.2390 Fiber optics, infrared; 140.7090 Ultrafast lasers; 230.6080 Optical devices, Sources; 300.6390 Spectroscopy, molecular; 140.3070 Infrared and far-infrared lasers