The influence of laser parameters, such as the excitation wavelength, on the emission signal obtained by laser-induced breakdown spectroscopy (LIBS), has been studied since the beginning of the technique’s applications, until today. Choosing the best wavelength for a given sample, or a unique emission line, is always a challenge for researchers. This work evaluates the influence of excitation wavelength for the analyse of a full-width LIBS spectrum range. Particularly, eight different mortar samples were used in this study. Firstly, the average spectra obtained with the two excitations (266 and 1064 nm) were evaluated by superimposing the two acquired spectra, and, a trend of different behavior was observed, depending on the emission spectral region. Excitation using the 1064 nm laser was favorable for the spectral range of 180–310 nm, on the other hand, the 266 nm was for the range of 312 nm − 1000 nm. The intensities of the C I, Si I, Zr III, Sb I, Fe II, Mg I, Mg II, Ca I, Ca II, Li I, K I, and, Na I emission lines were evaluated individually, and the results followed the same behavior. The size of the crater was assessed for both lasers and showed more effectiveness for 266 nm than 1064 nm. It is observed that the temperature or ablated size was not exclusively determined for the emission signal. A competition of physical phenomena must be contributing to this. For 1064 nm excitation, the inverse Bremsstrahlung (IB) phenomenon and higher temperature caused by the greater absorption of laser light at this wavelength favored emission in the UV region of the spectrum. On the other hand, the spectra obtained by 266 nm excitation, where Photoionization (PI) effect prevail the temperature achieved in this case is more favorable for filling the levels involved in transitions in the visible and IR range.
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