• 文献检索
  • 文档翻译
  • 深度研究
  • 学术资讯
  • Suppr Zotero 插件Zotero 插件
  • 邀请有礼
  • 套餐&价格
  • 历史记录
应用&插件
Suppr Zotero 插件Zotero 插件浏览器插件Mac 客户端Windows 客户端微信小程序
定价
高级版会员购买积分包购买API积分包
服务
文献检索文档翻译深度研究API 文档MCP 服务
关于我们
关于 Suppr公司介绍联系我们用户协议隐私条款
关注我们

Suppr 超能文献

核心技术专利：CN118964589B侵权必究
粤ICP备2023148730 号-1Suppr @ 2026

文献检索

告别复杂PubMed语法，用中文像聊天一样搜索，搜遍4000万医学文献。AI智能推荐，让科研检索更轻松。

立即免费搜索

文件翻译

保留排版，准确专业，支持PDF/Word/PPT等文件格式，支持 12+语言互译。

免费翻译文档

深度研究

AI帮你快速写综述，25分钟生成高质量综述，智能提取关键信息，辅助科研写作。

立即免费体验

用于物质波激光干涉引力天线（MIGA）的冷原子源。

Cold-atom sources for the Matter-wave laser Interferometric Gravitation Antenna (MIGA).

作者信息

Beaufils Quentin, Sidorenkov Leonid A, Lebegue Pierre, Venon Bertrand, Holleville David, Volodimer Laurent, Lours Michel, Junca Joseph, Zou Xinhao, Bertoldi Andrea, Prevedelli Marco, Sabulsky Dylan O, Bouyer Philippe, Landragin Arnaud, Canuel Benjamin, Geiger Remi

机构信息

LNE-SYRTE, Observatoire de Paris, Université PSL, CNRS:UMR 8630, Sorbonne Université, 61 avenue de l'Observatoire, 75014, Paris, France.

LP2N, Laboratoire Photonique, Numérique et Nanosciences, Université Bordeaux-IOGS-CNRS:UMR 5298, rue F. Mitterrand, 33400, Talence, France.

出版信息

Sci Rep. 2022 Nov 8;12(1):19000. doi: 10.1038/s41598-022-23468-3.

DOI:10.1038/s41598-022-23468-3
PMID:36347902
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC9643383/
Abstract

The Matter-wave laser Interferometric Gravitation Antenna (MIGA) is an underground instrument using cold-atom interferometry to perform precision measurements of gravity gradients and strains. Following its installation at the low noise underground laboratory LSBB in the South-East of France, it will serve as a prototype for gravitational wave detectors with a horizontal baseline of 150 meters. Three spatially separated cold-atom interferometers will be driven by two common counter-propagating lasers to perform a measurement of the gravity gradient along this baseline. This article presents the cold-atom sources of MIGA, focusing on the design choices, the realization of the systems, the performances and the integration within the MIGA instrument.

摘要

物质波激光干涉引力天线（MIGA）是一种地下仪器，利用冷原子干涉测量法来精确测量重力梯度和应变。在安装于法国东南部低噪声地下实验室LSBB之后，它将作为基线水平为150米的引力波探测器的原型。三个空间分离的冷原子干涉仪将由两束反向传播的共用激光驱动，以测量沿此基线的重力梯度。本文介绍了MIGA的冷原子源，重点关注设计选择、系统实现、性能以及在MIGA仪器中的集成情况。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/ff129b9e238c/41598_2022_23468_Fig10_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/d849bdd7af72/41598_2022_23468_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/a7024d1eb013/41598_2022_23468_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/c855c717d43f/41598_2022_23468_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/c1e9e81fc895/41598_2022_23468_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/2d8b8a3aa7e1/41598_2022_23468_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/894053839451/41598_2022_23468_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/9ea3c846b448/41598_2022_23468_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/e5daebc2be26/41598_2022_23468_Fig8_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/4a95771f4423/41598_2022_23468_Fig9_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/ff129b9e238c/41598_2022_23468_Fig10_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/d849bdd7af72/41598_2022_23468_Fig1_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/a7024d1eb013/41598_2022_23468_Fig2_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/c855c717d43f/41598_2022_23468_Fig3_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/c1e9e81fc895/41598_2022_23468_Fig4_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/2d8b8a3aa7e1/41598_2022_23468_Fig5_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/894053839451/41598_2022_23468_Fig6_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/9ea3c846b448/41598_2022_23468_Fig7_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/e5daebc2be26/41598_2022_23468_Fig8_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/4a95771f4423/41598_2022_23468_Fig9_HTML.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/13e3/9643383/ff129b9e238c/41598_2022_23468_Fig10_HTML.jpg

相似文献

1
Cold-atom sources for the Matter-wave laser Interferometric Gravitation Antenna (MIGA).用于物质波激光干涉引力天线（MIGA）的冷原子源。
Sci Rep. 2022 Nov 8;12(1):19000. doi: 10.1038/s41598-022-23468-3.
2
Exploring gravity with the MIGA large scale atom interferometer.利用MIGA大型原子干涉仪探索引力。
Sci Rep. 2018 Sep 14;8(1):14064. doi: 10.1038/s41598-018-32165-z.
3
A fibered laser system for the MIGA large scale atom interferometer.一种用于MIGA大型原子干涉仪的光纤激光系统。
Sci Rep. 2020 Feb 24;10(1):3268. doi: 10.1038/s41598-020-59971-8.
4
Arm-length stabilisation for interferometric gravitational-wave detectors using frequency-doubled auxiliary lasers.使用倍频辅助激光器对干涉式引力波探测器进行臂长稳定化。
Opt Express. 2012 Jan 2;20(1):81-9. doi: 10.1364/OE.20.000081.
5
High power, low-noise, and multiply resonant photodetector for interferometric gravitational wave detectors.用于干涉式引力波探测器的高功率、低噪声和多重谐振光电探测器。
Rev Sci Instrum. 2007 May;78(5):054704. doi: 10.1063/1.2735559.
6
Comparison of atom interferometers and light interferometers as space-based gravitational wave detectors.原子干涉仪与光干涉仪在基于空间的引力波探测器中的比较。
Phys Rev Lett. 2012 May 25;108(21):211101. doi: 10.1103/PhysRevLett.108.211101. Epub 2012 May 21.
7
Transponder-type laser interferometer prototype for spaceborne gravitational wave detectors.用于星载引力波探测器的应答器型激光干涉仪原型。
Appl Opt. 2024 Feb 1;63(4):1032-1038. doi: 10.1364/AO.511022.
8
Gravitational wave detection using laser interferometry beyond the standard quantum limit.利用激光干涉测量法突破标准量子极限进行引力波探测。
Philos Trans A Math Phys Eng Sci. 2018 May 28;376(2120). doi: 10.1098/rsta.2017.0289.
9
Displacement noise from back scattering and specular reflection of input optics in advanced gravitational wave detectors.先进引力波探测器中输入光学元件的背向散射和镜面反射产生的位移噪声。
Opt Express. 2013 May 6;21(9):10546-62. doi: 10.1364/OE.21.010546.
10
Time-Delay Interferometry.时间延迟干涉测量法
Living Rev Relativ. 2014;17(1):6. doi: 10.12942/lrr-2014-6. Epub 2014 Aug 5.

本文引用的文献

1
A fibered laser system for the MIGA large scale atom interferometer.一种用于MIGA大型原子干涉仪的光纤激光系统。
Sci Rep. 2020 Feb 24;10(1):3268. doi: 10.1038/s41598-020-59971-8.
2
Interleaved atom interferometry for high-sensitivity inertial measurements.用于高灵敏度惯性测量的交错原子干涉测量法。
Sci Adv. 2018 Dec 21;4(12):eaau7948. doi: 10.1126/sciadv.aau7948. eCollection 2018 Dec.
3
Exploring gravity with the MIGA large scale atom interferometer.利用MIGA大型原子干涉仪探索引力。
Sci Rep. 2018 Sep 14;8(1):14064. doi: 10.1038/s41598-018-32165-z.
4
Prospects for Multiband Gravitational-Wave Astronomy after GW150914.GW150914之后的多波段引力波天文学前景。
Phys Rev Lett. 2016 Jun 10;116(23):231102. doi: 10.1103/PhysRevLett.116.231102. Epub 2016 Jun 8.
5
Atom interferometer based on Bragg scattering from standing light waves.基于驻波光布拉格散射的原子干涉仪。
Phys Rev Lett. 1995 Oct 2;75(14):2638-2641. doi: 10.1103/PhysRevLett.75.2638.
6
Atom wave interferometry with diffraction gratings of light.基于光衍射光栅的原子波干涉测量法。
Phys Rev Lett. 1995 Oct 2;75(14):2633-2637. doi: 10.1103/PhysRevLett.75.2633.
7
Bragg scattering of atoms from a standing light wave.原子从驻波光中的布拉格散射。
Phys Rev Lett. 1988 Feb 8;60(6):515-518. doi: 10.1103/PhysRevLett.60.515.