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Preparation of azobenzene-intercalated kaolinite and monitoring of the photoinduced activity

Published online by Cambridge University Press:  29 March 2019

Anna Koteja*
Affiliation:
Department of Mineralogy, Petrography and Geochemistry, Faculty of Geology, Geophysics and Environmental Protection, AGH University of Science and Technology, al. Mickiewicza 30, 30-059 Krakow, Poland
Jakub Matusik
Affiliation:
Department of Mineralogy, Petrography and Geochemistry, Faculty of Geology, Geophysics and Environmental Protection, AGH University of Science and Technology, al. Mickiewicza 30, 30-059 Krakow, Poland
*
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Abstract

Systems consisting of layered structures and photoactive molecules have been studied extensively. The structures of resulting complexes may be controlled by UV–Vis radiation, which subsequently affects their materials properties. This study describes a synthesis route for obtaining a photoresponsive kaolinite intercalation compound. The material was prepared by co-intercalating azobenzene and benzylalkylammonium chlorides into a methoxy form of kaolinite. The resultant materials possessed large basal spacing values in the range of 45–55 Å. The UV–Vis and Fourier-transform infrared spectroscopy analyses confirmed the reversible photoisomerization of azobenzene upon exposure to UV and Vis radiation. This phenomenon was significantly influenced by the type and amount of co-intercalated molecules. Upon multiple trans–cis conversions, the azobenzene partially evaporated. For the first time, a kaolinite-based material was prepared that exhibited photochromic behaviour upon UV and Vis irradiation.

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Type
Article
Copyright
Copyright © Mineralogical Society of Great Britain and Ireland 2019 
Figure 0

Table 1. Ammonium salt and Az intercalates: symbols, salt type, Az/MBCn wt. ratio and time of reaction with Az.

Figure 1

Fig. 1. XRD patterns of pure kaolinite (M), MDS intercalate and MM-grafted kaolinite.

Figure 2

Fig. 2. FTIR spectra of a = kaolinite, b = MDS, c = MM, d = MBC12, e = MBC14 and f = MBC16.

Figure 3

Fig. 3. XRD patterns of MBCn intercalates and MBCnA(0.2-3d) samples. Thin lines correspond to pure surfactants or Az.

Figure 4

Fig. 4. FTIR spectra of: a = MBC16, b = MBC16A(0.2-1d), c = MBC16A(0.2-3d), d = MBC16A(0.2-7d), e = MBC16A(0.5-1d), f = MBC16A(1.0-1d) and pure Az.

Figure 5

Fig. 5. TG, DTG and DTA curves and the evolved gas analysis (QMS) of MBC16 and MBC16A(0.2-1d) samples.

Figure 6

Fig. 6. Basal spacing values (d001) of MBCn samples versus time of reaction with Az (a) and initial Az loading (b). The samples marked with ‘–’ are before the reaction with Az.

Figure 7

Fig. 7. Molar amount of Az calculated per 1 mol of MM (upper diagram) and Az/BCn molar ratio (lower diagram) in MBCnA samples obtained in various experimental conditions. Error bars are equal to two standard deviations.

Figure 8

Fig. 8. UV–Vis spectra of: (a) MBC16A(0.2-3d) sample irradiated with UV in 10 min time intervals, starting from 10 min up to 90 min; (b) MBCnA(0.2-3d) samples irradiated with UV for 10 min and after 24 h of exposure to Vis light.

Figure 9

Fig. 9. FTIR spectra of MBC16A(0.2-3d) sample irradiated with UV in time intervals of 0.5, 1.0 and 5.0 min, starting from 0.5 min up to 20 min (lower spectra); and treated with Vis light in time intervals of 0.5–8.0 h, starting from 0.5 h up to 48 h (upper spectra).

Figure 10

Fig. 10. Influence of UV irradiation, Vis irradiation and alternating UV and Vis treatment on the intensities of 788 and 757 cm–1 bands.

Figure 11

Fig. 11. Influence of alternating UV and Vis irradiation on the FTIR spectra of the MBC16A(0.2-3d) sample.

Figure 12

Fig. 12. The d001 value shifts upon alternating UV and Vis radiation.