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Spin Seebeck Effect from Antiferromagnetic Magnons and Critical Spin Fluctuations in Epitaxial FeF_{2} Films.
Li, Junxue; Shi, Zhong; Ortiz, Victor H; Aldosary, Mohammed; Chen, Cliff; Aji, Vivek; Wei, Peng; Shi, Jing.
Afiliação
  • Li J; Department of Physics and Astronomy, University of California, Riverside, California 92521, USA.
  • Shi Z; School of Physics Science and Engineering, Tongji University, Shanghai 200092, China.
  • Ortiz VH; Department of Physics and Astronomy, University of California, Riverside, California 92521, USA.
  • Aldosary M; Department of Physics and Astronomy, University of California, Riverside, California 92521, USA.
  • Chen C; Department of Physics and Astronomy, King Saud University, Riyadh 11451, Saudi Arabia.
  • Aji V; Department of Physics and Astronomy, University of California, Riverside, California 92521, USA.
  • Wei P; Department of Physics and Astronomy, University of California, Riverside, California 92521, USA.
  • Shi J; Department of Physics and Astronomy, University of California, Riverside, California 92521, USA.
Phys Rev Lett ; 122(21): 217204, 2019 May 31.
Article em En | MEDLINE | ID: mdl-31283322
ABSTRACT
We report a longitudinal spin Seebeck effect (SSE) study in epitaxially grown FeF_{2}(110) antiferromagnetic (AFM) thin films with strong uniaxial anisotropy over the temperature range of 3.8-250 K. Both the magnetic-field and temperature-dependent SSE signals below the Néel temperature (T_{N}=70 K) of the FeF_{2} films are consistent with a theoretical model based on the excitations of AFM magnons without any net induced static magnetic moment. In addition to the characteristic low-temperature SSE peak associated with the AFM magnons, there is another SSE peak at T_{N} which extends well into the paramagnetic phase. All the SSE data taken at different magnetic fields up to 12 T near and above the critical point T_{N} follow the critical scaling law very well with the critical exponents for magnetic susceptibility of 3D Ising systems, which suggests that the AFM spin correlation is responsible for the observed SSE near T_{N}.

Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Ano de publicação: 2019 Tipo de documento: Article

Texto completo: 1 Base de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Ano de publicação: 2019 Tipo de documento: Article