Govender Malcolm, Shikwambana Lerato, Mwakikunga Bonex Wakufwa, Sideras-Haddad Elias, Erasmus Rudolph Marthinus, Forbes Andrew
CSIR National Laser Centre, P, O, Box 395, Pretoria 0001, South Africa.
Nanoscale Res Lett. 2011 Feb 23;6(1):166. doi: 10.1186/1556-276X-6-166.
In this letter, the production of multi-phase WO3 and WO3-x (where x could vary between 0.1 and 0.3) nanostructures synthesized by CO2-laser pyrolysis technique at varying laser wavelengths (9.22-10.82 mm) and power densities (17-110 W/cm2) is reported. The average spherical particle sizes for the wavelength variation samples ranged between 113 and 560 nm, and the average spherical particle sizes for power density variation samples ranged between 108 and 205 nm. Synthesis of W18O49 (= WO2.72) stars by this method is reported for the first time at a power density and wavelength of 2.2 kW/cm2 and 10.6 μm, respectively. It was found that more concentrated starting precursors result in the growth of hierarchical structures such as stars, whereas dilute starting precursors result in the growth of simpler structures such as wires.
在这封信中,报道了通过二氧化碳激光热解技术在不同激光波长(9.22 - 10.82毫米)和功率密度(17 - 110瓦/平方厘米)下合成的多相WO₃和WO₃₋ₓ(其中x可在0.1至0.3之间变化)纳米结构。波长变化样品的平均球形粒径在113至560纳米之间,功率密度变化样品的平均球形粒径在108至205纳米之间。首次报道了通过该方法在功率密度和波长分别为2.2千瓦/平方厘米和10.6微米的条件下合成W₁₈O₄₉(= WO₂.₇₂)星形结构。结果发现,起始前驱体浓度较高会导致星形等分级结构的生长,而稀释的起始前驱体则会导致线等较简单结构的生长。