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arXiv 2202.02505cond-mat.mtrl-sci
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低温合成具有增强磁化强度和光催化降解染料和析氢性能的BiFeO $_{3}$纳米粒子

Low temperature synthesis of BiFeO$_{3}$ nanoparticles with enhanced magnetization and promising photocatalytic performance in dye degradation and hydrogen evolution

M. A. Basith, Nilufar Yesmin, Rana Hossain

摘要:

在这项调查中,我们已经合成了BiFeO $_{3}$纳米粒子通过不同的水热反应温度从200 $^{\circ}$ C到120 $^{\circ}$ C,以评估其可见光驱动的光催化活性,以及其适用于通过水分解制氢。在水热反应温度高达160 $^{\circ}$ C时形成菱方体钙钛矿结构的BiFeO $_{3}$,然而,在反应温度进一步降低时观察到混合硅线石相。XRD Rietveld分析、XPS分析和FESEM成像确保了在160 $^{\circ}$ C反应温度下形成了平均尺寸为20 nm的单相且结晶良好的纳米颗粒。在该特定反应温度下制备的纳米颗粒还表现出改善的磁化强度、降低的漏电流密度和优异的铁电行为。这些纳米颗粒在可见光范围内表现出相当高的吸光度,具有低的带隙(2.1 eV)。实验观察到的带隙与使用第一性原理计算计算的带隙非常一致。这些纳米颗粒良好的光催化性能能够产生比本体BiFeO $_{3}$以及市售Degussa P25二氧化钛产生的太阳能氢两倍多的氢。值得注意的是,对于在不同反应温度下制备的本体材料和纳米颗粒,实验观察到的带隙几乎相等。因此,在太阳能应用中,在160 $^{\circ}$ C反应温度下制备的BFO纳米颗粒的优越性可能不仅仅归因于它们的带隙,还归因于其他因素,例如减小的颗粒尺寸、优异的形貌、良好的结晶性、大的表面积与体积比、铁电性等。

英文摘要:

In this investigation, we have synthesized BiFeO$_{3}$ nanoparticles by varying hydrothermal reaction temperatures from 200 $^{\circ}$C to 120 $^{\circ}$C to assess their visible-light-driven photocatalytic activity along with their applicability for hydrogen production via water splitting. The rhombohedral perovskite structure of BiFeO$_{3}$ is formed for hydrothermal reaction temperature up to 160 $^{\circ}$C, however, for a further decrement of reaction temperature a mixed sillenite phase is observed. The XRD Rietveld analysis, XPS analysis and FESEM imaging ensure the formation of single-phase and well crystalline nanoparticles at 160 $^{\circ}$C reaction temperature with 20 nm of average size. The nanoparticles fabricated at this particular reaction temperature also exhibit improved magnetization, reduced leakage current density and excellent ferroelectric behavior. These nanoparticles demonstrate considerably high absorbance in the visible range with a low bandgap (2.1 eV). The experimentally observed bandgap is in excellent agreement with the calculated bandgap using the first-principles calculations. The favorable photocatalytic performance of these nanoparticles has been able to generate more than two times of solar hydrogen compared to that produced by bulk BiFeO$_{3}$ as well as commercially available Degussa P25 titania. Notably, the experimentally observed bandgap is almost equal for both bulk material and nanoparticles prepared at different reaction temperatures. Therefore, in solar energy applications, the superiority of BFO nanoparticles prepared at 160 $^{\circ}$C reaction temperature may be attributed not only to solely their bandgap but also to other factors, such as reduced particle size, excellent morphology, well crystallinity, large surface to volume ratio, ferroelectricity and so on.

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