• 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

利用铷蓝光跃迁的原子干涉测量法。

Atom Interferometry with Rb Blue Transitions.

作者信息

Salvi L, Cacciapuoti L, Tino G M, Rosi G

机构信息

Dipartimento di Fisica e Astronomia and LENS, Università di Firenze, INFN Sezione di Firenze, via Sansone 1, I-50019 Sesto Fiorentino (FI), Italy.

European Space Agency, Keplerlaan 1, 2201 AZ Noordwijk, Netherlands.

出版信息

Phys Rev Lett. 2023 Sep 8;131(10):103401. doi: 10.1103/PhysRevLett.131.103401.

DOI:10.1103/PhysRevLett.131.103401
PMID:37739366
Abstract

We demonstrate a novel scheme for Raman-pulse and Bragg-pulse atom interferometry based on the 5S-6P blue transitions of ^{87}Rb that provides an increase by a factor ∼2 of the interferometer phase due to accelerations with respect to the commonly used infrared transition at 780 nm. A narrow-linewidth laser system generating more than 1 W of light in the 420-422 nm range was developed for this purpose. Used as a cold-atom gravity gradiometer, our Raman interferometer attains a stability to differential acceleration measurements of 1×10^{-8}  g at 1 s and 2×10^{-10}  g after 2000 s of integration time. When operated on first-order Bragg transitions, the interferometer shows a stability of 6×10^{-8}  g at 1 s, averaging to 1×10^{-9}  g after 2000 s of integration time. The instrument sensitivity, currently limited by the noise due to spontaneous emission, can be further improved by increasing the laser power and the detuning from the atomic resonance. The present scheme is attractive for high-precision experiments as, in particular, for the determination of the Newtonian gravitational constant.

摘要

我们展示了一种基于(^{87}Rb)的(5S - 6P)蓝光跃迁的拉曼脉冲和布拉格脉冲原子干涉测量新方案,与常用的(780nm)红外跃迁相比,该方案因加速度导致的干涉仪相位增加了约(2)倍。为此开发了一种窄线宽激光系统,可在(420 - 422nm)范围内产生超过(1W)的光。用作冷原子重力梯度仪时,我们的拉曼干涉仪在(1s)内对差分加速度测量的稳定性达到(1×10^{-8}g),积分时间为(2000s)后达到(2×10^{-10}g)。当在一阶布拉格跃迁上运行时,干涉仪在(1s)内的稳定性为(6×10^{-8}g),积分时间为(2000s)后平均为(1×10^{-9}g)。目前该仪器的灵敏度受自发发射噪声限制,可通过增加激光功率和与原子共振的失谐来进一步提高。本方案对高精度实验具有吸引力,特别是对于牛顿引力常数的测定。

相似文献

1
Atom Interferometry with Rb Blue Transitions.利用铷蓝光跃迁的原子干涉测量法。
Phys Rev Lett. 2023 Sep 8;131(10):103401. doi: 10.1103/PhysRevLett.131.103401.
2
Determination of the newtonian gravitational constant using atom interferometry.利用原子干涉测量法测定牛顿引力常数。
Phys Rev Lett. 2008 Feb 8;100(5):050801. doi: 10.1103/PhysRevLett.100.050801.
3
Canceling the Gravity Gradient Phase Shift in Atom Interferometry.消除原子干涉测量中的重力梯度相移
Phys Rev Lett. 2017 Dec 22;119(25):253201. doi: 10.1103/PhysRevLett.119.253201. Epub 2017 Dec 19.
4
A dual-magneto-optical-trap atom gravity gradiometer for determining the Newtonian gravitational constant.一种用于测定牛顿引力常数的双磁光阱原子重力梯度仪。
Rev Sci Instrum. 2021 May 1;92(5):053202. doi: 10.1063/5.0040701.
5
Atom interferometer measurement of the newtonian constant of gravity.利用原子干涉仪测量牛顿引力常数
Science. 2007 Jan 5;315(5808):74-7. doi: 10.1126/science.1135459.
6
Atom Interferometer Driven by a Picosecond Frequency Comb.由皮秒频率梳驱动的原子干涉仪
Phys Rev Lett. 2022 Oct 21;129(17):173204. doi: 10.1103/PhysRevLett.129.173204.
7
High-performance silicon photonic single-sideband modulators for cold-atom interferometry.用于冷原子干涉测量的高性能硅光子单边带调制器。
Sci Adv. 2024 Jul 12;10(28):eade4454. doi: 10.1126/sciadv.ade4454. Epub 2024 Jul 10.
8
A compact laser system for a portable atom interferometry gravimeter.一种用于便携式原子干涉重力仪的紧凑型激光系统。
Rev Sci Instrum. 2019 Apr;90(4):043104. doi: 10.1063/1.5053132.
9
Feedback control of atom trajectories in a horizontal atom gravity gradiometer.
Opt Express. 2022 Mar 14;30(6):10071-10083. doi: 10.1364/OE.450276.
10
Large-Area Atom Interferometry with Frequency-Swept Raman Adiabatic Passage.基于扫频拉曼绝热通道的大面积原子干涉测量
Phys Rev Lett. 2015 Sep 4;115(10):103001. doi: 10.1103/PhysRevLett.115.103001. Epub 2015 Aug 31.