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Main Authors: Dasigi, Karthik, Dmitriev, Pavel A., Wo, Kah Jen, Hanamura, Fumiya, Kong, Lingda, Touzard, Steven
Format: Preprint
Published: 2025
Subjects:
Online Access:https://arxiv.org/abs/2509.25950
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author Dasigi, Karthik
Dmitriev, Pavel A.
Wo, Kah Jen
Hanamura, Fumiya
Kong, Lingda
Touzard, Steven
author_facet Dasigi, Karthik
Dmitriev, Pavel A.
Wo, Kah Jen
Hanamura, Fumiya
Kong, Lingda
Touzard, Steven
contents Optical Vector Analysers (OVA) are critical for emerging technologies such as integrated photonics and optical positioning. Achieving a sensitivity near the Standard Quantum Limit (SQL) while acquiring a wide spectrum allows an accurate measurement of targets that are fragile, non-linear, or that scatter most of the probe light away. Existing OVAs operate with a sensitivity orders of magnitude below the SQL. In this paper, we use a free-running interferometer with a frequency range of 20 THz as an OVA. We introduce novel methods to mitigate the phase noise and obtain a unit signal-to-noise ratio for powers at the fW level. We apply this technique towards quantifying the fabrication quality of microring resonators in thin-film Lithium Niobate. Our characterisation yields a signal-to-noise ratio above 1 with much less than 1 circulating photon and reveals a quality factor above 5 millions, unambiguously attributed to low internal losses.
format Preprint
id arxiv_https___arxiv_org_abs_2509_25950
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Quantum-Limited Optical Vector Analysis
Dasigi, Karthik
Dmitriev, Pavel A.
Wo, Kah Jen
Hanamura, Fumiya
Kong, Lingda
Touzard, Steven
Optics
Optical Vector Analysers (OVA) are critical for emerging technologies such as integrated photonics and optical positioning. Achieving a sensitivity near the Standard Quantum Limit (SQL) while acquiring a wide spectrum allows an accurate measurement of targets that are fragile, non-linear, or that scatter most of the probe light away. Existing OVAs operate with a sensitivity orders of magnitude below the SQL. In this paper, we use a free-running interferometer with a frequency range of 20 THz as an OVA. We introduce novel methods to mitigate the phase noise and obtain a unit signal-to-noise ratio for powers at the fW level. We apply this technique towards quantifying the fabrication quality of microring resonators in thin-film Lithium Niobate. Our characterisation yields a signal-to-noise ratio above 1 with much less than 1 circulating photon and reveals a quality factor above 5 millions, unambiguously attributed to low internal losses.
title Quantum-Limited Optical Vector Analysis
topic Optics
url https://arxiv.org/abs/2509.25950