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Advanced LIGO Input Optics

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Input Optics

The input optics (IO) conditions light from the pre-stabilized laser (PSL) for injection into the main interferometer.
The design requirements for the Advanced LIGO Input Optics Subsystem include the requirements for the RF modulation of the light, acquisition and operation of the mode cleaner, mode matching of the light to the interferometer, and beam steering into the interferometer. The scope of the IO includes the following tasks and hardware:
  • phase modulation Pockels cells
  • intermediate frequency and intensity stabilization
  • power control into interferometer
  • photodetectors and related protective shutter (if needed)
  • cabling
  • active jitter suppression system
  • mode cleaner optics
  • Faraday isolators - optical isolation of the PSL
  • mode matching telescopes
  • distribution of light for length and alignment sensing and control
IO scheme
Figure 1 Overall IO Product Specification

IO Team

Univ. of Florida
R. Amin
K. Franzen
G. Hearn
G. Mueller
V. Quetschke
M. Rakhmanov
D. Reitze
D. Tanner
L. Williams


Institute of Applied Physics
(Nizhny Novgorod, Russia)
E. Khazanov
A. Sergeev

LIGO Lab Liaison
P. King

IO Documentation

IO Subsystem Design Requirements
MC curved mirror substrate requirements (doc)
MC flat mirror substrate requirements (doc)
Sideband requirements
Pointing requirements
Signal sensing
Longitudinal and angular alignment
requirements for AdvLIGO MC

EO-modulators for AdvLIGO
Mode matching in AdvLIGO
IO subsystem conceptional design document

IO Subsystems

Modulation
Mode cleaning
Optical isolation
Mode matching

Other relevant links

LIGO
LSC homepage
Advanced LIGO (new version?)
Advanced LIGO (old version?)
LIGO document search
LIGO core optics design links

LIGO pictures - Hanford

Advanced LIGO Mailing lists

IO mailing list
COC mailing list
SUS mailing list

All LIGO mailing lists

Other Advanced Subsystems

Core optics components (COC)

© University of Florida Contact:  Volker Quetschke This page was last updated May 4, 2004.