Origin of ultraviolet photovoltaic effect in Fe3O4 thin films | |
K. Zhao; J. F. Feng; Y. H. Huang; J. G. Zhao; H. B. Lu; X. F. Han; W. S. Zhan | |
2005 | |
发表期刊 | Chinese Physics
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ISSN | 1009-1963 |
卷号 | 14期号:12页码:2595-2597 |
摘要 | We have investigated the transport and ultraviolet photovoltaic properties of Fe3O4 thin films grown on glass substrates by facing-target sputtering technique. The nonlinear dependence of current-density on voltage suggests that the transport process is most likely the tunnelling process and grain boundaries act as barriers. Furthermore, nonequilibrium electron-hole pairs are excited in the grains and grain boundary regions for Fe3O4 film under ultraviolet laser, since the energy gap of Fe3O4 is smaller than the ultraviolet photon energy. And then the built-in electric field near the grain boundaries will separate carriers, leading to the appearance of an instant photovoltage. |
部门归属 | chinese acad sci, inst phys, beijing natl lab condensed matter phys, key lab opt phys, beijing 100080, peoples r china. chinese acad sci, inst phys, beijing natl lab condensed matter phys, state key lab magnetism, beijing 100080, peoples r china. chinese acad sci, int ctr mat phys, shenyang 110016, peoples r china.;zhao, k (reprint author), chinese acad sci, inst phys, beijing natl lab condensed matter phys, key lab opt phys, pob 603, beijing 100080, peoples r china;kzhao@aphy.iphy.ac.cn |
关键词 | Photovoltaic Effect Magnetite Thin Film Sandwiches |
URL | 查看原文 |
WOS记录号 | WOS:000233836300035 |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.imr.ac.cn/handle/321006/35261 |
专题 | 中国科学院金属研究所 |
推荐引用方式 GB/T 7714 | K. Zhao,J. F. Feng,Y. H. Huang,et al. Origin of ultraviolet photovoltaic effect in Fe3O4 thin films[J]. Chinese Physics,2005,14(12):2595-2597. |
APA | K. Zhao.,J. F. Feng.,Y. H. Huang.,J. G. Zhao.,H. B. Lu.,...&W. S. Zhan.(2005).Origin of ultraviolet photovoltaic effect in Fe3O4 thin films.Chinese Physics,14(12),2595-2597. |
MLA | K. Zhao,et al."Origin of ultraviolet photovoltaic effect in Fe3O4 thin films".Chinese Physics 14.12(2005):2595-2597. |
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