Crystalline silicon is currently being discussed as test-mass material for future generations of gravitational wave detectors that will operate at cryogenic temperatures. We present optical absorption measurements on a large-dimension sample of crystalline silicon at a wavelength of 1550nm at room temperature. The absorption was measured in a monolithic cavity setup using the photo-thermal self-phase modulation technique. The result for the absorption coefficient of this float-zone sample with a specific resistivity of 11kOhm cm was measured to be \alpha_A=(264 +/- 39)ppm/cm
Current interferometric gravitational wave detectors use the combination of quasi-monochromatic, con...
Crystalline silicon has been proposed as a new test mass material in third generation gravitational ...
Future laser-interferometric gravitational wave detectors (GWDs) will potentially employ test mass m...
Crystalline silicon is currently being discussed as test-mass material for future generations of gra...
Crystalline silicon is currently being discussed as test-mass material for future generations of gra...
The sensitivity of future gravitational wave (GW) observatories will be limited by thermal noise in ...
Abstract. The sensitivity of future gravitational wave (GW) observatories will be limited by thermal...
The announcement of the direct detection of gravitational waves (GW) by the LIGO and Virgo collabora...
International audienceWe report in this article on the measurement of the optical absorption of mode...
A key element for the next-generation gravitational wave interferometers are optical substrates char...
Mirrors made of silicon have been proposed for use in future cryogenic gravitational-wave detectors,...
Current interferometric gravitational wave detectors use the combination of quasi-monochromatic, con...
Crystalline silicon has been proposed as a new test mass material in third generation gravitational ...
Future laser-interferometric gravitational wave detectors (GWDs) will potentially employ test mass m...
Crystalline silicon is currently being discussed as test-mass material for future generations of gra...
Crystalline silicon is currently being discussed as test-mass material for future generations of gra...
The sensitivity of future gravitational wave (GW) observatories will be limited by thermal noise in ...
Abstract. The sensitivity of future gravitational wave (GW) observatories will be limited by thermal...
The announcement of the direct detection of gravitational waves (GW) by the LIGO and Virgo collabora...
International audienceWe report in this article on the measurement of the optical absorption of mode...
A key element for the next-generation gravitational wave interferometers are optical substrates char...
Mirrors made of silicon have been proposed for use in future cryogenic gravitational-wave detectors,...
Current interferometric gravitational wave detectors use the combination of quasi-monochromatic, con...
Crystalline silicon has been proposed as a new test mass material in third generation gravitational ...
Future laser-interferometric gravitational wave detectors (GWDs) will potentially employ test mass m...