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arXiv 2512.17536physics.opticsphysics.ins-det

用于光学光谱分析仪频率校准的完全稳定25 GHz频率梳

Fully stabilized 25 GHz frequency comb for frequency calibration of optical spectrum analyzer

Yoonkwon On, Dae Hee Kim, Sujin Kim, Yong Jin Kim, Jong-Ahn Kim, Sunghoon Eom, Jae Yong Lee, Yoon-Soo Jang

AI总结:

本文提出一种完全稳定25 GHz频率梳,用于高精度光学光谱分析仪的频率校准,提供多个校准点,提升校准精度和性能评估。

摘要:

光学光谱仪在科学和工业应用中被广泛应用,精确的频率校准对于确保其可靠性能至关重要。传统上,光谱仪是通过参考气体细胞或参考灯进行校准的。然而,这些传统方法无法满足对高精度和稳定性的需求。尽管频率稳定激光器提供极佳的频率不确定性,但它们只能在固定频率提供一个校准点,这不适合宽范围的光谱仪校准。在本工作中,我们展示了一种完全稳定、高重复率的电光频率梳(EO梳),作为绝对频率参考,提供多个校准点,覆盖宽谱范围。我们的25 GHz EO梳提供了一个宽谱带,从189.5 THz到196 THz(对应1530 nm到1582 nm),可追溯到频率标准,相对标准不确定度为10^-13。通过常规光学光谱仪可以解析这些明确且均匀分布的梳模式,从而实现宽范围、高精度的频率校准。我们通过将商用光谱仪的测量频率值参考到我们明确定义的梳模式上,从而评估频率误差,标准不确定度为20 MHz(或相对标准不确定度为10^-7),这受限于光谱仪的类型A不确定度(重复性)。所提出的方法易于实施,并在宽谱范围内提供多个参考频率标准的校准点。这种方法提高了光谱仪的校准和性能评估,有助于光学计量学的发展。

英文摘要:

Optical spectrometers are widely used in scientific and industrial applications, and precise frequency calibration is essential for ensuring their reliable performance. Traditionally, spectrometers have been calibrated using reference gas cells or reference lamps. However, such conventional methods are not enough to meet the demands for high accuracy and stability. Although frequency-stabilized lasers offer excellent frequency uncertainty, they provide only a single calibration point at a fixed frequency, which is unsuitable for wide-range spectrometer calibration. In this work, we demonstrate a fully stabilized, high-repetition rate electro-optic frequency comb (EO comb) as an absolute frequency reference providing multiple calibration points over a broad spectral range. Our 25 GHz EO comb provides a broadband spectrum spanning from 189.5 THz to 196 THz (corresponding to 1530 nm to 1582 nm), traceable to a frequency standard with a relative standard uncertainty of 10^-13. The well-defined and evenly spaced comb modes can be spectrally resolved by conventional optical spectrometers, enabling wide-range, high-precision frequency calibration. We directly calibrated a commercial spectrometer by referencing its measured frequency values to our well-defined comb modes, thereby evaluating the frequency error with a standard uncertainty of 20 MHz (or relative standard uncertainty of 10^-7), which is limited by the Type A uncertainty (repeatability) of the spectrometer. The proposed method is simple to implement and provides multiple calibration points referenced to the frequency standards over a broad spectral range. This approach improves both the calibration and performance evaluation of spectrometers, and it contributes to the advancement of optical metrology.

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