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Study of the sub-millikelvin thermal control of a frequency reference cavity

机译:频率参考腔的亚毫米尔文热控制研究

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ESA (European Space Agency) scientific missions like GAIA (Global Astrometric Interferometer for Astrophysics) and LISA (Laser Interferometer Space Antenna) require laser interferometry as driving technology. A frequency-stable light radiation is employed as a dimensional standard for very accurate (below 10pm) distance measurements. The wavelength of the light radiation, emitted by a monolithic laser source, must be stabilized against a frequency standard, which should be provided by a Fabry-Perot cavity which is dimensionally stable better than one part over 10{sup}12. A cavity of this kind, although made by a thermally stable material, must be thermally stabilized better than 0.1 mK. Moreover, construction must absolutely guarantee the only cause of deformation to be thermo-elastic, in order to make decisive and effective thermal control. The paper presents thermal design of the cavity as well as the digital control guaranteeing thermal stability. Simulated results are encouraging. Cavity construction is under way.
机译:ESA(欧洲航天局)像盖亚这样的科学任务(天体物理学的全球星形干涉仪)和LISA(激光干涉仪空间天线)需要激光干涉测量作为驾驶技术。频率稳定的光辐射用作非常精确的(低于10PM)距离测量的尺寸标准。由单片激光源发射的光辐射的波长必须稳定在频率标准,该频率标准应由法布里 - 珀罗腔提供,该法布里 - 珀罗腔尺寸稳定于10°以上的一个部分12。虽然由热稳定的材料制成,但是必须热稳定优于0.1 mk的腔。此外,建设必须绝对保证变形的唯一原因是热弹性,以便进行决定性和有效的热控制。本文介绍了腔的热设计以及保证热稳定性的数字控制。模拟结果令人鼓舞。腔结构正在进行中。

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