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Beating the classical precision limit with spin-1 Dicke states of more than 10,000 atoms.


ABSTRACT: Interferometry is a paradigm for most precision measurements. Using N uncorrelated particles, the achievable precision for a two-mode (two-path) interferometer is bounded by the standard quantum limit (SQL), [Formula: see text], due to the discrete (quanta) nature of individual measurements. Despite being a challenging benchmark, the two-mode SQL has been approached in a number of systems, including the Laser Interferometer Gravitational-Wave Observatory and today's best atomic clocks. For multimode interferometry, the SQL becomes [Formula: see text] using M modes. Higher precision can also be achieved using entangled particles such that quantum noises from individual particles cancel out. In this work, we demonstrate an interferometric precision of [Formula: see text] dB beyond the three-mode SQL, using balanced spin-1 (three-mode) Dicke states containing thousands of entangled atoms. The input quantum states are deterministically generated by controlled quantum phase transition and exhibit close to ideal quality. Our work shines light on the pursuit of quantum metrology beyond SQL.

SUBMITTER: Zou YQ 

PROVIDER: S-EPMC6016791 | biostudies-other | 2018 Jun

REPOSITORIES: biostudies-other

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Beating the classical precision limit with spin-1 Dicke states of more than 10,000 atoms.

Zou Yi-Quan YQ   Wu Ling-Na LN   Liu Qi Q   Luo Xin-Yu XY   Guo Shuai-Feng SF   Cao Jia-Hao JH   Tey Meng Khoon MK   You Li L  

Proceedings of the National Academy of Sciences of the United States of America 20180601 25


Interferometry is a paradigm for most precision measurements. Using N uncorrelated particles, the achievable precision for a two-mode (two-path) interferometer is bounded by the standard quantum limit (SQL), [Formula: see text], due to the discrete (quanta) nature of individual measurements. Despite being a challenging benchmark, the two-mode SQL has been approached in a number of systems, including the Laser Interferometer Gravitational-Wave Observatory and today's best atomic clocks. For multi  ...[more]

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