Details
| Original language | English |
|---|---|
| Pages (from-to) | 124-132 |
| Number of pages | 9 |
| Journal | Physics Letters A |
| Volume | 194 |
| Issue number | 1-2 |
| Publication status | Published - 24 Oct 1994 |
Abstract
Thermal lensing limits the performance of advanced interferometric gravitational wave detectors that use high light powers. We evaluate the effects of thermal lensing in such systems and estimate their gravitational wave sensitivity assuming that fused silica optical substrates are employed. Although useful sensitivity can be achieved with established designs, the new technique of resonant sideband extraction is most promising for wideband detectors.
ASJC Scopus subject areas
- Physics and Astronomy(all)
- General Physics and Astronomy
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In: Physics Letters A, Vol. 194, No. 1-2, 24.10.1994, p. 124-132.
Research output: Contribution to journal › Article › Research › peer review
}
TY - JOUR
T1 - Thermal lensing in recycling interferometric gravitational wave detectors
AU - Strain, K. A.
AU - Danzmann, K.
AU - Mizuno, J.
AU - Nelson, P. G.
AU - Rüdiger, A.
AU - Schilling, R.
AU - Winkler, W.
N1 - Funding Information: We would like to acknowledge the support of this work by the Bundesministerium fur Forschung und Technologie (BMFT) and helpful advice and suggestions from the Glasgow gravitational wave group.
PY - 1994/10/24
Y1 - 1994/10/24
N2 - Thermal lensing limits the performance of advanced interferometric gravitational wave detectors that use high light powers. We evaluate the effects of thermal lensing in such systems and estimate their gravitational wave sensitivity assuming that fused silica optical substrates are employed. Although useful sensitivity can be achieved with established designs, the new technique of resonant sideband extraction is most promising for wideband detectors.
AB - Thermal lensing limits the performance of advanced interferometric gravitational wave detectors that use high light powers. We evaluate the effects of thermal lensing in such systems and estimate their gravitational wave sensitivity assuming that fused silica optical substrates are employed. Although useful sensitivity can be achieved with established designs, the new technique of resonant sideband extraction is most promising for wideband detectors.
UR - http://www.scopus.com/inward/record.url?scp=0000296418&partnerID=8YFLogxK
U2 - 10.1016/0375-9601(94)00717-4
DO - 10.1016/0375-9601(94)00717-4
M3 - Article
AN - SCOPUS:0000296418
VL - 194
SP - 124
EP - 132
JO - Physics Letters A
JF - Physics Letters A
SN - 0375-9601
IS - 1-2
ER -