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Waveguides based on TeGe thick films for spatial interferometry

机译:基于TeGe厚膜的波导用于空间干涉测量

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In the present paper we focus on the fabrication of waveguides which will be able to work in the large infrared window [6-20μm], compatible with the ESA requirements in the framework of the detection of Exo-solar planets by nulling interferometry.rnThe first step in the fabrication of such components is the realization of planar waveguides being able to guide light in this spectral range. In order to do so, telluride materials were selected: Te_(75)Ge_(15)Ga_(10) bulk glasses were chosen as substrates and TeGe films as guiding layers. The Te_(75)Ge_(15)Ga_(10) bulk glasses were purified during their synthesis which ensures an optimal transmission in the whole range from 6 to 20 μm. TeGe thick films with different compositions were deposited by thermal co-evaporation. Homogeneous films with thickness up to 15 microns could be produced. The M-lines measurement of their refractive index at λ= 10.6 μm highlighted a linear behavior versus the atomic percentage in tellurium and confirmed their compatibility for the project.rnFirst planar waveguides could be optically characterized after having prepared their input and output facets by an appropriate polishing procedure. Guidance of light was demonstrated in the whole range [6-20
机译:在本文中,我们重点研究能够在较大的红外窗口[6-20μm]中工作的波导,该波导与通过零位干涉法检测外太阳系行星的框架中的ESA要求兼容。制造这种组件的第一步是实现能够在该光谱范围内引导光的平面波导。为此,选择了碲化物材料:选择Te_(75)Ge_(15)Ga_(10)块状玻璃作为衬底,选择TeGe膜作为引导层。 Te_(75)Ge_(15)Ga_(10)大块玻璃在合成过程中进行了纯化,从而确保了从6到20μm的整个范围内的最佳透射率。通过热共蒸发沉积具有不同组成的TeGe厚膜。可以生产厚度不超过15微米的均质薄膜。 M线在λ= 10.6μm处的折射率测量结果表明,线形相对于碲中的原子百分比具有线性关系,并证实了其与该项目的兼容性。抛光程序。在整个范围内都演示了光导[6-20

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