This can be seen in Figure 5a (Bi-301) and 5b (Bi-302). The reduction https://www.selleckchem.com/products/Adriamycin.html of the formation of BiNPs is due to the oxidation with the substrates. High-resolution XRD spectrum of the BiNPs prepared on c-plane sapphire at 200°C (Bi-304) is shown in Figure 5c. A sharp peak can be ascribed to Al2O3 (006)

at 2θ = 42°, together with a broadened minor peak at 2θ = 27.5°. A closer look from 2θ = 24° to 2θ = 30° shown in Figure 5d reveals that this minor peak can be considered as the combination of two distinct peaks, Bi (003) at 27.17° and Bi2O3 at 27.92°. The same conditions occurred on BiNPs deposited on ITO glass. Since pure bismuth samples suffer oxidation gradually, as can be checked by the XRD spectrum measured day by day, we can thus rule out the possibility that the samples were oxidized after they were taken outside.

This oxidation effect can be explained by comparing the bonding energies of oxygen with other elements [33–35]. The bonding enthalpies (in unit of kJ/mol) are 337.2 ± 12.6 for Bi-O, 320.1 ± 41.8 for In-O, 531.8 ± 12.6 for Sn-O, 511 ± 3 for Al-O, and 799.6 ± 13.4 for Si-O. As can be clearly seen from this table, the bonding enthalpy between Bi and O is significantly lower than the values between O and other elements, except In-O. This indicates that Bi2O3 can be formed easier than SiO2, Al2O3, In2O3, and Selonsertib research buy SnO2. Once the temperature during deposition process is high enough, the bonding between Al-O, In-O, and Sn-O may be weakened and increase the possibility of the formation of Bi2O3. On the other hand, Si-O bonding is too high for the oxidation process to take place. We thus conclude that once the substrate temperature is high enough, Bi can react with oxygen from substrates to form Bi2O3, which compromises its ability to form BiNPs. Figure 5 SEM images and XRD spectra in experiment C. (a)

SEM images of BiNPs deposited on ITO glass substrates at 160 °C (Bi-301). (b) SEM images of BiNPs deposited on ITO glass substrates at 200°C (Bi-302). (c) XRD spectra of the BiNPs prepared on c-plane sapphire at 200°C and 0.12 W/cm2 for 60 s (Bi-304). (d) A closer look from 2θ = 24° to 2θ = 30°, in which Bi(003) and Bi2O3 diffraction peaks can be identified. Conclusions We present a systematic experiment to measure the optimal Erastin datasheet conditions to grow a single layer of BiNPs on various substrates by using a RF sputtering JAK inhibitor system at 200 °C, using 0.12 W/cm2. With suitable chosen parameters, BiNP samples were successfully fabricated, instead of BiNWs and Bi thin films. Since the optical bandgap decreases as the diameter of BiNPs increases, we were able to modulate their values by depositing various sizes of BiNPs. All these data and sample statistics are listed in the tables for future references. Authors’ information HYL obtained his Ph.D. degree at National Taiwan University (NTU) and is currently a post-doctoral fellow of the Department of Physics, NTU.