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Soft X-Ray Magneto-optical Faraday Effect around Ni M2,3 Edges

Soft X-Ray Magneto-optical Faraday Effect around Ni M2,3 Edges
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摘要 We present magneto-optical (MO) Faraday spectra measured around the M2,3 edges (60-70eV) of Ni films at the Beijing Synchrotron Radiation Facility (BSI^F). A polarization analysis of the final state of the transmitted radiation from the Ni film is employed to determine the Faraday rotation at the edges. The MO effect becomes resonantly enhanced at the M2,3 edges, and accordingly large values for the rotation angle β of 1.85 ± 0.19° for this ferromagnetic Ni film with thickness of 31 nm are measured. Without the magnetic field, the azimuthal angles do not shift; with parallel and antiparallel magnetic field the rotation angles shift in the opposite way and they are symmetrical. The uncertainty of Faraday rotation angles mainly comes from the data fitting and the state change of the beamline when the angles are measured. We present magneto-optical (MO) Faraday spectra measured around the M2,3 edges (60-70eV) of Ni films at the Beijing Synchrotron Radiation Facility (BSI^F). A polarization analysis of the final state of the transmitted radiation from the Ni film is employed to determine the Faraday rotation at the edges. The MO effect becomes resonantly enhanced at the M2,3 edges, and accordingly large values for the rotation angle β of 1.85 ± 0.19° for this ferromagnetic Ni film with thickness of 31 nm are measured. Without the magnetic field, the azimuthal angles do not shift; with parallel and antiparallel magnetic field the rotation angles shift in the opposite way and they are symmetrical. The uncertainty of Faraday rotation angles mainly comes from the data fitting and the state change of the beamline when the angles are measured.
出处 《Chinese Physics Letters》 SCIE CAS CSCD 2008年第3期1110-1112,共3页 中国物理快报(英文版)
基金 Supported by the National Natural Science Foundation of China under Grant Nos 10275078 and 10435050. The authors thank Dr Wang Zhan-Shan for the Mo/Si multilayer fabrication.
关键词 supernova explosion proto-neutron star shock wave supernova explosion, proto-neutron star, shock wave
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  • 1Chen C T, Idzerda Y U, Lin H J, Smith N V, Meigs G, Chaban E, Ho G H, Pellegrin E and Sette F 1995 Phys. Rev. Lett, 75 152 被引量:1
  • 2Kortright J B, Awschalom D D, Stohr J, Bader S D, Idzerda Y U, Parkin S P, Schuller I K and Siegmann H C 1999 J. Magn. Magn. Mater. 207 7 被引量:1
  • 3Mertins H C, Schafers F, Cann X L, Gaupp A and Gudat W 2000 Phys. Rev. B 61 874 被引量:1
  • 4Mertins H C, Valencia S, Abramsohn D, Gaupp A, Gudat W and Oppeneer P M 2004 Phys. Rev. B 69 064407 被引量:1
  • 5Valencia S, Gaupp A, Gudat W, Mertins H C, Oppeneer P M, Abramsohn D, and Schneider C M 2006 New J. Phys. 8 254 被引量:1
  • 6Hatano T, Hu W, Saito K and Watanabe M 1999 J. Electron. Spectrosc. Relat. Phenom. 101-103 287 被引量:1
  • 7Mertinsa H C, Schafersa F, Gauppa A, Gudata W, Kunesb J and Oppeneer P M 2001 Nucl. Instrum. Methods A 467- 468 1407 被引量:1
  • 8Sun L J, CUI M Q, Zhu J, Zhao Y D, Zheng L, Ma C Y, Chen K, Zhao J, Zhou K J, Wang Z S and Wang H C 2007 High Energy Phys. Nuel. Phys. 31 400 (in Chinese) 被引量:1
  • 9Zhu J, Cui M Q, Zheng L, Zhao Y D and Wang Z S 2004 Nucl. Tech. 27 489 (in chinese) 被引量:1
  • 10Sun L J 2007 PhD Dissertation (Institute of High Energy Physics, Chinese Academy of Sciences) pp 113-114 144 (in Chinese) 被引量:1

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