Details
| Originalsprache | Englisch |
|---|---|
| Aufsatznummer | 022001 |
| Fachzeitschrift | Physical Review D - Particles, Fields, Gravitation and Cosmology |
| Jahrgang | 74 |
| Ausgabenummer | 2 |
| Publikationsstatus | Veröffentlicht - 6 Juli 2006 |
| Extern publiziert | Ja |
Abstract
We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) interferometer with power recycling. The purpose of the detuned RSE configuration is to manipulate and optimize the optical response of the interferometer to differential displacements (induced by gravitational waves) as a function of frequency, independently of other parameters of the interferometer. The design of our interferometer results in an optical gain with two peaks: an RSE optical resonance at around 4 kHz and a radiation pressure induced optical spring at around 41 Hz. We have developed a reliable procedure for acquiring lock and establishing the desired optical configuration. In this configuration, we have measured the optical response to differential displacement and found good agreement with predictions at both resonances and all other relevant frequencies. These results build confidence in both the theory and practical implementation of the more complex optical configuration being planned for Advanced LIGO.
ASJC Scopus Sachgebiete
- Physik und Astronomie (insg.)
- Kern- und Hochenergiephysik
- Physik und Astronomie (insg.)
- Physik und Astronomie (sonstige)
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in: Physical Review D - Particles, Fields, Gravitation and Cosmology, Jahrgang 74, Nr. 2, 022001, 06.07.2006.
Publikation: Beitrag in Fachzeitschrift › Artikel › Forschung › Peer-Review
}
TY - JOUR
T1 - Measurement of optical response of a detuned resonant sideband extraction gravitational wave detector
AU - Miyakawa, Osamu
AU - Ward, Robert
AU - Adhikari, Rana
AU - Evans, Matthew
AU - Abbott, Benjamin
AU - Bork, Rolf
AU - Busby, Daniel
AU - Heefner, Jay
AU - Ivanov, Alexander
AU - Smith, Michael
AU - Taylor, Robert
AU - Vass, Stephen
AU - Weinstein, Alan
AU - Varvella, Monica
AU - Kawamura, Seiji
AU - Kawazoe, Fumiko
AU - Sakata, Shihori
AU - Mow-Lowry, Conor
PY - 2006/7/6
Y1 - 2006/7/6
N2 - We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) interferometer with power recycling. The purpose of the detuned RSE configuration is to manipulate and optimize the optical response of the interferometer to differential displacements (induced by gravitational waves) as a function of frequency, independently of other parameters of the interferometer. The design of our interferometer results in an optical gain with two peaks: an RSE optical resonance at around 4 kHz and a radiation pressure induced optical spring at around 41 Hz. We have developed a reliable procedure for acquiring lock and establishing the desired optical configuration. In this configuration, we have measured the optical response to differential displacement and found good agreement with predictions at both resonances and all other relevant frequencies. These results build confidence in both the theory and practical implementation of the more complex optical configuration being planned for Advanced LIGO.
AB - We report on the optical response of a suspended-mass detuned resonant sideband extraction (RSE) interferometer with power recycling. The purpose of the detuned RSE configuration is to manipulate and optimize the optical response of the interferometer to differential displacements (induced by gravitational waves) as a function of frequency, independently of other parameters of the interferometer. The design of our interferometer results in an optical gain with two peaks: an RSE optical resonance at around 4 kHz and a radiation pressure induced optical spring at around 41 Hz. We have developed a reliable procedure for acquiring lock and establishing the desired optical configuration. In this configuration, we have measured the optical response to differential displacement and found good agreement with predictions at both resonances and all other relevant frequencies. These results build confidence in both the theory and practical implementation of the more complex optical configuration being planned for Advanced LIGO.
UR - http://www.scopus.com/inward/record.url?scp=33745748890&partnerID=8YFLogxK
U2 - 10.48550/arXiv.gr-qc/0604078
DO - 10.48550/arXiv.gr-qc/0604078
M3 - Article
AN - SCOPUS:33745748890
VL - 74
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
SN - 1550-7998
IS - 2
M1 - 022001
ER -