Details
| Original language | English |
|---|---|
| Pages (from-to) | 273-276 |
| Number of pages | 4 |
| Journal | Physics Letters A |
| Volume | 175 |
| Issue number | 5 |
| Publication status | Published - 19 Apr 1993 |
| Externally published | Yes |
Abstract
We introduce a new Fabry-Perot based interferometric gravitational wave detector that, compared with previous designs, greatly decreases the amount of power that must be transmitted through optical substrates to obtain a given light power in its arms. This significantly reduces the effects of wavefront distortions caused by heating due to absorption in the optics, and allows an improved broadband sensitivity to be achieved.
ASJC Scopus subject areas
- Physics and Astronomy(all)
- General Physics and Astronomy
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In: Physics Letters A, Vol. 175, No. 5, 19.04.1993, p. 273-276.
Research output: Contribution to journal › Article › Research › peer review
}
TY - JOUR
T1 - Resonant sideband extraction
T2 - a new configuration for interferometric gravitational wave detectors
AU - Mizuno, J.
AU - Strain, K. A.
AU - Nelson, P. G.
AU - Chen, J. M.
AU - Schilling, R.
AU - Rüdiger, A.
AU - Winkler, W.
AU - Danzmann, K.
N1 - Funding Information: The authors would like to thank the gravitational wave group at the University of Glasgow, especially Jim Hough, Euan Morrison, David Robertson, and Harry Ward who all provided helpful insights into the understanding of this system. This work has been supported by the Bundesministerium fir Forschung und Tech-nologie (BMVF). One of the authors (JM) would like to thank the JSPS for its support.
PY - 1993/4/19
Y1 - 1993/4/19
N2 - We introduce a new Fabry-Perot based interferometric gravitational wave detector that, compared with previous designs, greatly decreases the amount of power that must be transmitted through optical substrates to obtain a given light power in its arms. This significantly reduces the effects of wavefront distortions caused by heating due to absorption in the optics, and allows an improved broadband sensitivity to be achieved.
AB - We introduce a new Fabry-Perot based interferometric gravitational wave detector that, compared with previous designs, greatly decreases the amount of power that must be transmitted through optical substrates to obtain a given light power in its arms. This significantly reduces the effects of wavefront distortions caused by heating due to absorption in the optics, and allows an improved broadband sensitivity to be achieved.
UR - http://www.scopus.com/inward/record.url?scp=0000306506&partnerID=8YFLogxK
U2 - 10.1016/0375-9601(93)90620-F
DO - 10.1016/0375-9601(93)90620-F
M3 - Article
AN - SCOPUS:0000306506
VL - 175
SP - 273
EP - 276
JO - Physics Letters A
JF - Physics Letters A
SN - 0375-9601
IS - 5
ER -