2013
DOI: 10.1039/c3cp51422f
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Spectral challenges of individual wavelength-scale particles: strong phonons and their distorted lineshapes

Abstract: Beyond our own interest in airborne particulate matter, the prediction of extinction and absorption spectra of single particles of mixed composition has wide use in astronomy, geology, atmospheric sciences, and nanotechnology. Single particle spectra present different challenges than traditional spectroscopic approaches. To quantify the amount of a material in a bulk sample (molecules in solution or the gas phase), one might employ the Beer-Lambert law assuming a simple slab-type assay geometry and averaging o… Show more

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Cited by 5 publications
(12 citation statements)
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“…Finally, the fitted fringe polynomial was used as a transmission background, b i , for the measured vibrational transmission data, s i , to obtain an extinction vibrational lineshape, i.e., −log­( s i / b i ) as shown in Figure b with symbols. The lineshapes were all dominated by absorption and close to Lorentzian shapes, but there can also be dispersive characteristics in thin-film spectra, so each was fit to an absorption/dispersion lineshape (solid lines in Figure b) as where φ is the phase shift, S is the linestrength, ṽ 0 is the transition position (1/λ), and Γ is the half width at half-max (HWHM). If the phase shift is zero, then only the cos φ term survives and the form is pure Lorentzian for absorption.…”
Section: Resultsmentioning
confidence: 99%
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“…Finally, the fitted fringe polynomial was used as a transmission background, b i , for the measured vibrational transmission data, s i , to obtain an extinction vibrational lineshape, i.e., −log­( s i / b i ) as shown in Figure b with symbols. The lineshapes were all dominated by absorption and close to Lorentzian shapes, but there can also be dispersive characteristics in thin-film spectra, so each was fit to an absorption/dispersion lineshape (solid lines in Figure b) as where φ is the phase shift, S is the linestrength, ṽ 0 is the transition position (1/λ), and Γ is the half width at half-max (HWHM). If the phase shift is zero, then only the cos φ term survives and the form is pure Lorentzian for absorption.…”
Section: Resultsmentioning
confidence: 99%
“…Finally, the fitted fringe polynomial was used as a transmission background, b i , for the measured vibrational transmission data, s i , to obtain an extinction vibrational lineshape, i.e., −log(s i /b i ) as shown in Figure 3b with symbols. The lineshapes were all dominated by absorption and close to Lorentzian shapes, but there can also be dispersive characteristics in thin-film spectra, 25 so each was fit to an absorption/dispersion lineshape 25−27 (solid lines in Figure 3b) as…”
Section: ■ Resultsmentioning
confidence: 99%
“…The combination of particles of comparable size to the probing wavelength and the strong vibrational spectra of common mineral components of dust 10,14 warrant the use of Mie theory, which can handle severe lineshape distortions. Mie theory 38 is a complete solution to Maxwell's equations describing the absorption and scattering of light by spherical particles given the spherical particle's complex index of refraction and radius.…”
Section: Resultsmentioning
confidence: 99%
“…Given the known symptoms of inhaling high levels of particulate matter and the risks associated with long-term exposure to elevated levels, there is a need to chemically evaluate such particles. 10 Our previous single particle work [10][11][12][13][14][15] includes the study of a spectral library of 63 individual dust particles extracted from our laboratory air 12 demonstrating chemical variability including minerals, sulfates, nitrates, and organics, as well as a model for analysis of volume fractions. 10 In this work, the study is extended to samples obtained from a home air filter and the 11 September 2001 World Trade Center (WTC) event.…”
Section: Introductionmentioning
confidence: 99%
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