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Physics, Instrumentation and Detectors, physics.ins-det, Astrophysics, Instrumentation and Methods for Astrophysics, astro-ph.IM
Abstract:
We report on the first long-term application of squeezed vacuum states of
light to improve the shot-noise-limited sensitivity of a gravitational-wave
observatory. In particular, squeezed vacuum was applied to the German/British
detector GEO600 during a period of three months from June to August 2011, when
GEO600 was performing an observational run together with the French/Italian
Virgo detector. In a second period squeezing application continued for about 11
months from November 2011 to October 2012. During this time, squeezed vacuum
was applied for 90.2% (205.2 days total) of the time that science-quality data
was acquired with GEO600. Sensitivity increase from squeezed vacuum application
was observed broad-band above 400Hz. The time average of gain in sensitivity
was 26% (2.0dB), determined in the frequency band from 3.7kHz to 4.0kHz. This
corresponds to a factor of two increase in observed volume of the universe, for
sources in the kHz region (e.g. supernovae, magnetars). We introduce three new
techniques to enable stable long-term application of squeezed light, and show
that the glitch-rate of the detector did not increase from squeezing
application. Squeezed vacuum states of light have arrived as a permanent
application, capable of increasing the astrophysical reach of
gravitational-wave detectors.
