Details
| Originalsprache | Englisch |
|---|---|
| Seiten (von - bis) | 270-275 |
| Seitenumfang | 6 |
| Fachzeitschrift | Journal of Physics: Conference Series |
| Jahrgang | 32 |
| Ausgabenummer | 1 |
| Publikationsstatus | Veröffentlicht - 29 März 2006 |
| Veranstaltung | Sixth Edoardo Amaldi Conference on gravitational waves - Okinawa, Japan Dauer: 20 Juni 2005 → 24 Juni 2005 |
Abstract
Second generation gravitational wave detectors require high power lasers with several 100W of output power and with very low temporal and spatial fluctuations. In this paper we discuss possible setups to achieve high laser power and describe a 200W prestabilized laser system (PSL). The PSL noise requirements for advanced gravitational wave detectors will be discussed in general and the stabilization scheme proposed for the Advanced LIGO PSL will be described. Special emphasis will be given to the most demanding power stabilization requiremets and new results (RIN ≤ 4×10 -9/√Hz) will be presented.
ASJC Scopus Sachgebiete
- Physik und Astronomie (insg.)
- Allgemeine Physik und Astronomie
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in: Journal of Physics: Conference Series, Jahrgang 32, Nr. 1, 29.03.2006, S. 270-275.
Publikation: Beitrag in Fachzeitschrift › Konferenzaufsatz in Fachzeitschrift › Forschung › Peer-Review
}
TY - JOUR
T1 - Stabilized High Power Laser for Advanced Gravitational Wave Detectors
AU - Willke, B.
AU - Danzmann, K.
AU - Fallnich, C.
AU - Frede, M.
AU - Heurs, M.
AU - King, P.
AU - Kracht, D.
AU - Kwee, P.
AU - Savage, R.
AU - Seifert, F.
AU - Wilhelm, R.
PY - 2006/3/29
Y1 - 2006/3/29
N2 - Second generation gravitational wave detectors require high power lasers with several 100W of output power and with very low temporal and spatial fluctuations. In this paper we discuss possible setups to achieve high laser power and describe a 200W prestabilized laser system (PSL). The PSL noise requirements for advanced gravitational wave detectors will be discussed in general and the stabilization scheme proposed for the Advanced LIGO PSL will be described. Special emphasis will be given to the most demanding power stabilization requiremets and new results (RIN ≤ 4×10 -9/√Hz) will be presented.
AB - Second generation gravitational wave detectors require high power lasers with several 100W of output power and with very low temporal and spatial fluctuations. In this paper we discuss possible setups to achieve high laser power and describe a 200W prestabilized laser system (PSL). The PSL noise requirements for advanced gravitational wave detectors will be discussed in general and the stabilization scheme proposed for the Advanced LIGO PSL will be described. Special emphasis will be given to the most demanding power stabilization requiremets and new results (RIN ≤ 4×10 -9/√Hz) will be presented.
UR - http://www.scopus.com/inward/record.url?scp=33645524549&partnerID=8YFLogxK
U2 - 10.1088/1742-6596/32/1/040
DO - 10.1088/1742-6596/32/1/040
M3 - Conference article
AN - SCOPUS:33645524549
VL - 32
SP - 270
EP - 275
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
SN - 1742-6588
IS - 1
T2 - Sixth Edoardo Amaldi Conference on gravitational waves
Y2 - 20 June 2005 through 24 June 2005
ER -