Revisiting magnetic properties of γ- Fe2WO6
ORAL
Abstract
Heda Zhang1, Gordon Peiker2, Mengze Zhu1, Brian Phelan1, Clarina dela Cruz3, Xianglin Ke1 (1. Physics and astronomy, Michigan State University; 2. Skyline high school; 3. Neutron scattering division, Oak Ridge National Lab)
Fe2WO6 is a p-type semiconductor with a large band gap (1.68 eV), serving as a promising photoelectrode material for water oxidation. Furthermore, this material also exhibits interesting magnetic properties depending on the crystalline phase. In this talk, we revisit the magnetic properties of gamma phase Fe2WO6 via magnetic susceptibility, heat capacity and neutron diffraction measurements. Comparing to an earlier study, we found some inconsistencies regarding the magnetic pattern and the temperature dependence of the magnetic ordering vector . Detailed discussions will be presented.
Fe2WO6 is a p-type semiconductor with a large band gap (1.68 eV), serving as a promising photoelectrode material for water oxidation. Furthermore, this material also exhibits interesting magnetic properties depending on the crystalline phase. In this talk, we revisit the magnetic properties of gamma phase Fe2WO6 via magnetic susceptibility, heat capacity and neutron diffraction measurements. Comparing to an earlier study, we found some inconsistencies regarding the magnetic pattern and the temperature dependence of the magnetic ordering vector . Detailed discussions will be presented.
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Presenters
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B. D. Phelan
Physics and Astronomy, Michigan State University
Authors
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HEDA ZHANG
Physics and Astronomy, Michigan State University
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Gordon Peiker
Skyline high school
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Mengze Zhu
Physics and Astronomy, Michigan State University
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B. D. Phelan
Physics and Astronomy, Michigan State University
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Clarina Dela Cruz
Neutron Scattering Division, Oak Ridge National Lab, Oak Ridge National Laboratory, Neutron Scattering Division, Oak Ridge National Laboratory, Oak Ridge National Lab, Neutron scattering devision, Oak Ridge National Lab, Neutron Scattering Science Division, Oak Ridge National Laboratory
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Xianglin Ke
Physics and Astronomy, Michigan State University, Michigan State University