Photothermal spectroscopy

Photothermal spectroscopy is a group of high sensitivity spectroscopy techniques used to measure optical absorption and thermal characteristics of a sample. The basis of photothermal spectroscopy is the change in thermal state of the sample resulting from the absorption of radiation. Light absorbed and not lost by emission results in heating. The heat raises temperature thereby influencing the thermodynamic properties of the sample or of a suitable material adjacent to it. Measurement of the temperature, pressure, or density changes that occur due to optical absorption are ultimately the basis for the photothermal spectroscopic measurements.

As with photoacoustic spectroscopy, photothermal spectroscopy is an indirect method for measuring optical absorption, because it is not based on the direct measure of the light which is involved in the absorption. In another sense, however, photothermal (and photoacoustic) methods measure directly the absorption, rather than e.g. calculate it from the transmission, as is the case of more usual (transmission) spectroscopic techniques. And it is this fact that gives the technique its high sensitivity, because in transmission techniques the absorptance is calculated as the difference between total light impinging on the sample and the transmitted (plus reflected, plus scattered) light, with the usual problems of accuracy when one deals with small differences between large numbers, if the absorption is small. In photothermal spectroscopies, instead, the signal is essentially proportional to the absorption, and is zero when there is zero true absorption, even in the presence of reflection or scattering.

There are several methods and techniques used in photothermal spectroscopy. Each of these has a name indicating the specific physical effect measured.

Photothermal deflection spectroscopy

Photothermal deflection spectroscopy is a kind of spectroscopy that measures the change in refractive index due to heating of a medium by light. It works via a sort of "mirage effect"[1] where a refractive index gradient exists adjacent to the test sample surface. A probe laser beam is refracted or bent in a manner proportional to the temperature gradient of the transparent medium near the surface. From this deflection, a measure of the absorbed excitation radiation can be determined. The technique is useful when studying optically thin samples, because sensitive measurements can be obtained of whether absorption is occurring. It is of value in situations where "pass through" or transmission spectroscopy can't be used.

There are two main forms of PDS: Collinear and Transverse. Collinear PDS was introduced in a 1980 paper by A.C. Boccara, D. Fournier, et al.[2] In collinear, two beams pass through and intersect in a medium. The pump beam heats the material and the probe beam is deflected. This technique only works for transparent media. In transverse, the probe beam heats come in normal to the surface, and the probe beam passes parallel. In a variation on this, the probe beam may reflect off the surface, and measure buckling due to heating. Transverse PDS can be done in Nitrogen, but better performance is gained in a liquid cell: usually an inert, non-absorbing material such as a perfluorocarbon is used.

In both collinear and transverse PDS, the surface is heated using a periodically modulated light source, such as an optical beam passing through a mechanical chopper or regulated with a function generator. A lock-in amplifier is then used to measure deflections found at the modulation frequency. Another scheme uses a pulsed laser as the excitation source. In that case, a boxcar average can be used to measure the temporal deflection of the probe beam to the excitation radiation. The signal falls off exponentially as a function of frequency, so frequencies around 1-10 hertz are frequently used. A full theoretical analysis of the PDS system was published by Jackson, Amer, et al. in 1981.[3] The same paper also discussed the use of PDS as a form of microscopy, called "Photothermal Deflection Microscopy", which can yield information about impurities and the surface topology of materials.[3]

See also

References

  1. ↑ In the true mirage, however, a light ray is bent gradually until it is totally reflected by the very hot air near soil. Here, instead, there is no reflection, and the ray is bent in a smooth way by the refraction index gradient, which acts like a prism.
  2. ↑ Boccara, A.C.; Fournier, D.; Jackson, Warren; Amer, Nabil. (1980). "Sensitive photothermal deflection technique for measuring absorption in optically thin media". Optics Letters 5 (9): 377–379. Bibcode:1980OptL....5..377B. doi:10.1364/OL.5.000377. PMID 19693234.
  3. ↑ 3.0 3.1 Jackson, W.B.; Amer, N.M.; Boccara, A.C.; Fournier, D. (1981-04-15). "Photothermal deflection spectroscopy and detection". Applied Optics 20 (8): 1333–1344. Bibcode:1981ApOpt..20.1333J. doi:10.1364/AO.20.001333.

  • J. A. Sell Photothermal Investigations of Solids and Fluids Academic Press, New York 1989
  • D. P. Almond and P. M. Patel Photothermal Science and Techniques Chapman and Hall, London 1996
  • S. E. Bialkowski Photothermal Spectroscopy Methods for Chemical Analysis John Wiley, New York 1996

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