Ferromagnetism of Co-doped TiO2(B) nanotubes
Wang, X. W., Gao, Xueping, Li, G. R., Gao, L., Yan, T. Y., & Zhu, Huai Yong (2007) Ferromagnetism of Co-doped TiO2(B) nanotubes. Applied Physics Letters, 91(14), pp. 143102-1.
The Co-doped titanate nanotubes, synthesized via a hydrothermal reaction, are calcined at 300, 400, and 500 degrees Celsius for 2 h in an argon atmosphere to yield Co-doped TiO2(B) nanotubes and anatase nanotubes with a dark gray color. It is shown that all calcined titania nanotubes have a stronger absorption in visible region, attributed to the formation of oxygen vacancies. The saturation magnetization of all Co-doped titania nanotubes is stronger than that of as-prepared Co-doped titanate nanotubes. In particular, Co-doped TiO2(B) nanotubes calcined at 300 degrees Celsius exhibit the strongest ferromagnetism due to the existence of oxygen vacancies, as confirmed further by electron paramagnetic resonance spectra.
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|Item Type:||Journal Article|
|Keywords:||calcination, cobalt, crystal growth from solution, ferromagnetism, magnetisation, nanotechnology, nanotubes, paramagnetic resonance, semiconductor materials, titanium compounds, vacancies (crystal), visible spectra|
|Subjects:||Australian and New Zealand Standard Research Classification > CHEMICAL SCIENCE (030000) > INORGANIC CHEMISTRY (030200) > Transition Metal Chemistry (030207)|
Australian and New Zealand Standard Research Classification > CHEMICAL SCIENCE (030000) > INORGANIC CHEMISTRY (030200) > Solid State Chemistry (030206)
Australian and New Zealand Standard Research Classification > CHEMICAL SCIENCE (030000) > PHYSICAL CHEMISTRY (INCL. STRUCTURAL) (030600) > Colloid and Surface Chemistry (030603)
|Divisions:||Past > QUT Faculties & Divisions > Faculty of Science and Technology|
Past > Schools > School of Physical & Chemical Sciences
|Copyright Owner:||Copyright 2007 American Institute of Physics|
|Copyright Statement:||Reproduced in accordance with the copyright policy of the publisher.|
|Deposited On:||08 Oct 2008|
|Last Modified:||25 Feb 2013 12:50|
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