Atom interferometry for gravitational wave detection

被引：1
|
作者：
Vetrano, F. [1 ]
机构：
[1] Univ Urbino Carlo Bo, DiSBeF, Via S Chiara 27, I-61029 Urbino, Italy
来源：
ATOM INTERFEROMETRY | 2014年 / 188卷
关键词：
CLOCKS; OPTICS; LIMIT;
D O I：
10.3254/978-1-61499-448-0-605
中图分类号：
TH7 [仪器、仪表];
学科分类号：
0804 ; 080401 ; 081102 ;
摘要：
After a short review of the properties of gravitational waves as described in Einstein general relativity, the problem of characterizing suitable detectors is addressed in order to define suitable parameters for comparison. The concept of sensitivity as a combination of frequency response function and noise budget at fixed signal to noise ratio is used, looking at the performances of existing optical gravitational waves antennas and of a symmetric Ramsey-Borde (Mach-Zehnder geometry) atom interferometer studied as a prototype of new detectors for gravitational radiation.
引用
收藏
页码：605 / 629
页数：25
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