4.7 Article

Enhanced magneto-optical effect in Y1.5Ce1.5Fe5O12 thin films deposited on silicon by pulsed laser deposition

Journal

JOURNAL OF ALLOYS AND COMPOUNDS
Volume 703, Issue -, Pages 591-599

Publisher

ELSEVIER SCIENCE SA
DOI: 10.1016/j.jallcom.2017.01.315

Keywords

Magnetooptics; Ce:YIG; Magnetic oxides; Thin films; Pulsed laser deposition; Silicon photonics

Funding

  1. National Natural Science Foundation of China [61475031, 51302027, 51522204]
  2. Fundamental Research Funds for the Central Universities [ZYGX2013J028, ZYGX2014Z001]
  3. Science Foundation for Youths of Sichuan Province [2015JQO014]
  4. Ministry Of Education Program of Introducing Talents of Discipline (111 project) [B13042]
  5. Doctoral Fund of Ministry of Education of China [20130185120009]

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Polycrystalline Ce: YIG thin films deposited on silicon are promising material candidates for integrated nonreciprocal photonic devices. So far, the reported Faraday rotation of polycrystalline Ce: YIG thin films on silicon is much lower than that of their single crystal or epitaxial thin film counterparts, limiting the magneto-optical figure of merit, device bandwidth and fabrication tolerance. In this paper, we report the growth of Ce: YIG thin films on silicon from targets with high Ce concentration up to nominally Y1.5Ce1.5Fe5O12 by pulsed laser deposition. The polycrystalline Y1.5Ce1.5Fe5O12 thin film showed pure garnet phase, smooth surface roughness of 0.7 nm, a dominant Ce(3+)valence state and a bulk-like saturation magnetization of 125 emu/cm(3) at room temperature. This material shows high Faraday rotation of-6410 deg/cm at 1550 nmwavelength, exceeding that of an Y2Ce1Fe5O12 epitaxial thin film on a GGG (100) substrate. However higher loss and lower figure of merit is also observed at 1550 nm wavelength compared to Y2Ce1Fe5O12 thin films, possibly due to the low oxygen partial pressure during fabrication. Low deposition oxygen partial pressure is essential to enhance the Ce solubility and Ce3+ concentration, which results in large Faraday rotation. (C) 2017 Elsevier B. V. All rights reserved.

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