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Spectroscopy for Materials Characterization


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the spectral resolution, it is a good practice to use a BW lower than the spectral width of the band (or bands) that is recorded. This spectral width can be experimentally measured by the full width at half maximum (FWHM), that is the spectral distance of the points at half amplitude of the band’s signal maximum. It is opportune to set at least BW < 0.5 FWHM to avoid distortions. After this choice has been done, it is opportune to set RT < BW/SS to avoid other distortions. Indeed, this choice ensures that the time needed for the detector to record a signal is lower than the time necessary for the instrument to change the wavelength in an interval equal to its spectral resolution.

      To show the effects that could be produced by a wrong choice of the instrumental parameters, a holmium glass filter has been employed [26, 27]. This sample is characterized by a series of narrow, well‐defined peaks in the spectral range from the visible to the UV; is commercially available; and can be used for teaching‐calibrating purposes. The spectrophotometer used enables to change the BW in the range 0.1–5 nm. Furthermore, it has SS in the range 10–1000 nm min−1 and RT in the interval 0.03–240 s. After an explorative spectrum, the band of the holmium filter centered at about 360 nm has been selected. The SS has been fixed to 20 nm min−1 and the RT to 0.25 s. The first experiment consists in changing the BW.

Schematic illustration of the absorption spectra of holmium glass filter at various bandwidths of the spectrophotometer from 0.1 to 5 nm. The inset reports the dependence of the full width at half maximum on the various employed bandwidths. Bottom: Absorption spectra of holmium glass filter at various scan speeds of the spectrophotometer from10 to 1000 nm min-1. The inset reports the dependence of the full width at half maximum on the various employed scan speeds.

      In the second experiment, the SS has been changed, fixing the BW = 0.5 nm and the RT = 1 s. As reported in Figure 1.8, the fast scanning of the spectrum induces a strong distortion because of the delay in the response of the detector with respect to the change in the wavelength. These examples show that the instrumental parameters should be opportunely set in order to avoid distortion and at the same time guarantee a good signal‐to‐noise ratio to enable a good analysis of the results.

      1.4.1.2 CCD Fiber Optic Device

      Many setups for absorption measurements are nowadays using fiber optics technology. These systems use compact light sources and CCD detectors coupled to gratings to obtain fiber optics spectrometers. The light from the source is driven by an optical fiber to the sample holder directing the light collimated by a lens perpendicular to the sample surface. The light exiting from the sample is collected by a second lens and is directed to another optical fiber that drives the light to the grating that disperses it and then is detected by a CCD. These systems are typically of small dimension and are portable, with many advantages for coupling them in various kinds of experiments like in situ measurements. The opportune choice of source, fibers, and detector enables to use these systems for UV‐Vis‐IR spectroscopy.

      1.4.2 Photoluminescence

Schematic illustration of absorption spectra of CdSe/ZnS core–shell nanoparticles at different concentrations in toluene solution. The inset shows the peak absorbance amplitude at 585 nm as a function of concentration; the straight line is a guide for the eye.