TY - GEN
T1 - Non-classical sources of light and their applications to gravitational wave detection
AU - McClelland, D. E.
AU - Collaboration, L. S.
N1 - Publisher Copyright:
© 2017 OSA.
PY - 2017
Y1 - 2017
N2 - Audio-band laser interferometer gravitational-wave detectors are massive optomechanical devices. Quantum enhancement requires sources at the operating wavelength with more than a factor of 10 squeezing from 1 Hz to 10 kHz, in a frequency-tailored quadrature.
AB - Audio-band laser interferometer gravitational-wave detectors are massive optomechanical devices. Quantum enhancement requires sources at the operating wavelength with more than a factor of 10 squeezing from 1 Hz to 10 kHz, in a frequency-tailored quadrature.
KW - Instrumentation, measurement, and metrology: 120.4880 optomechanics
KW - Quantum optics: 270.6570 squeezed states
UR - http://www.scopus.com/inward/record.url?scp=85020459297&partnerID=8YFLogxK
U2 - 10.1364/CLEO_AT.2017.JTh3G.5
DO - 10.1364/CLEO_AT.2017.JTh3G.5
M3 - Conference contribution
SN - 9781943580279
T3 - Optics InfoBase Conference Papers
BT - CLEO
PB - Optica Publishing Group (formerly OSA)
T2 - CLEO: Applications and Technology, CLEO_AT 2017
Y2 - 14 May 2017 through 19 May 2017
ER -