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Small optic suspensions for Advanced LIGO input optics and other precision optical experiments.

G Ciani1, M A Arain1, S M Aston2

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We designed compact optic suspensions to reduce seismic noise for the Advanced Laser Interferometer Gravitational Wave Observatory. These suspensions isolate optics in all six directions, with sensing and damping capabilities.

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Area of Science:

  • Seismology
  • Optics
  • Gravitational Wave Detection

Background:

  • Seismic motion is a significant noise source for sensitive instruments like gravitational wave detectors.
  • Out-of-cavity optics in the input optics subsystem require effective isolation from environmental vibrations.

Purpose of the Study:

  • To design and evaluate small optic suspensions for seismic motion suppression.
  • To improve the performance of the input optics subsystem for gravitational wave observatories.

Main Methods:

  • Development of compact, single-stage optic suspension systems.
  • Implementation of isolation in all six degrees of freedom.
  • Integration of local sensing and actuation for three degrees of freedom.
  • Incorporation of passive damping for the remaining three degrees of freedom.

Main Results:

  • Successful design and performance validation of small optic suspensions.
  • Demonstrated suppression of seismic motion for out-of-cavity optics.
  • Achieved full six-degree-of-freedom isolation with integrated sensing and damping.

Conclusions:

  • The developed optic suspensions effectively mitigate seismic noise in gravitational wave observatories.
  • These compact suspensions are a viable solution for enhancing the sensitivity of the input optics subsystem.
  • The design offers a robust method for isolating critical optical components from environmental disturbances.