Parametric oscillatory instability in a signal-recycled LIGO interferometer

The undesirable effect of parametric oscillatory instability in a LIGO (Laser Interferometer Gravitational-Wave Observatory) laser gravitational-wave antenna with a signal-recirculation mirror is analysed in detail. The instability is manifested in excitation of the Stokes optical mode and elastic m...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	Quantum electronics (Woodbury, N.Y.) N.Y.), 2007-12, Vol.37 (12), p.1097-1101
Hauptverfasser:	Vyatchanin, S P, Strigin, S E
Format:	Artikel
Sprache:	eng
Schlagworte:	ANTENNAS CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS EIGENFREQUENCY ELECTRICAL EQUIPMENT ELECTRONIC EQUIPMENT ENERGY-LEVEL TRANSITIONS EXCITATION FABRY-PEROT INTERFEROMETER GRAVITATIONAL WAVES INSTABILITY INTERFEROMETERS LASERS MEASURING INSTRUMENTS MIRRORS OPTICAL MODES OSCILLATION MODES PARAMETRIC INSTABILITIES PLASMA INSTABILITY PLASMA MACROINSTABILITIES RESONATORS SIGNALS
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

Beschreibung
Zusammenfassung:	The undesirable effect of parametric oscillatory instability in a LIGO (Laser Interferometer Gravitational-Wave Observatory) laser gravitational-wave antenna with a signal-recirculation mirror is analysed in detail. The instability is manifested in excitation of the Stokes optical mode and elastic mechanical mode of the mirror. It is shown that, if the eigenfrequencies of Fabry-Perot resonators in the interferometer arms are different, the parametric instability is quite small due to a small passband band width. (fifth seminar in memory of d.n. klyshko)
ISSN:	1063-7818 1468-4799
DOI:	10.1070/QE2007v037n12ABEH013675