gravitational waves detection
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2022 ◽  
Vol 20 (1) ◽  
pp. 011203
Author(s):  
Guanfang Wang ◽  
Zhu Li ◽  
Jialing Huang ◽  
Huizong Duan ◽  
Xiangqing Huang ◽  
...  

2021 ◽  
Vol 103 (4) ◽  
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Stefan Ast ◽  
Sibilla Di Pace ◽  
Jacques Millo ◽  
Mikhaël Pichot ◽  
Margherita Turconi ◽  
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2020 ◽  
Vol 151 ◽  
pp. 113378 ◽  
Author(s):  
Roberto Corizzo ◽  
Michelangelo Ceci ◽  
Eftim Zdravevski ◽  
Nathalie Japkowicz

2019 ◽  
Vol 12 (3) ◽  
pp. 477-485
Author(s):  
陈 琨 CHEN Kun ◽  
蔡志鸣 CAI Zhi-ming ◽  
侍行剑 SHI Xing-jian ◽  
邓剑峰 DENG Jian-feng ◽  
余金培 YU Jin-pei ◽  
...  

2018 ◽  
Vol 30 (6) ◽  
pp. 817-829 ◽  
Author(s):  
Yuqiong Li ◽  
Ziren Luo ◽  
Heshan Liu ◽  
Ruihong Gao ◽  
Gang Jin

2014 ◽  
Vol 85 (2) ◽  
pp. 024503 ◽  
Author(s):  
He-Shan Liu ◽  
Yu-Hui Dong ◽  
Yu-Qiong Li ◽  
Zi-Ren Luo ◽  
Gang Jin

2013 ◽  
Vol 23 ◽  
pp. 135-143
Author(s):  
FLAVIO VETRANO ◽  
GIANLUCA M. GUIDI ◽  
ANDREA VICERÉ ◽  
QUENTIN BODART ◽  
YU-HUNG LIEN ◽  
...  

The output of a simple Mach-Zehnder atom interferometer (with light field beam splitters) is studied in order to obtain sensitivity curves for GW signals in the paraxial approximation by using the ABCD matrices techniques and first order perturbation theory for mirroratom interaction; order of magnitude of relevant physical parameters for a realistic GW detector through atom interferometry is deduced, both for single- and coupled-interferometers configurations. Finally a synthetic overview of ongoing activities of the Florence-Urbino group in this field is presented.


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