International audienceWe report in this article on the measurement of the optical absorption of moderately doped crystalline silicon samples at 1550 nm, which is a candidate material for the main optics of the low temperature interferometer of the Einstein Telescope (ET). We observe a nearly constant absorption from room temperature down to cryogenic temperatures for two silicon samples presenting an optical absorption of 0.029 cm −1 and 780 ppm cm −1 , both crystals doped with boron. This is in contradiction to what was assumed previously—a negligible optical absorption at low temperature due to the carrier freezeout. As the main consequence, if the silicon intrinsic absorption can not be lowered , the cross section of the mirror suspensio...
Amorphous silicon (aSi) is a promising material for application in mirror coatings with low thermal ...
Crystalline silicon has been proposed as a new test mass material in third generation gravitational ...
Amorphous silicon has ideal properties for many applications in fundamental research and industry. H...
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 ...
The announcement of the direct detection of gravitational waves (GW) by the LIGO and Virgo collabora...
A key element for the next-generation gravitational wave interferometers are optical substrates char...
Abstract. The sensitivity of future gravitational wave (GW) observatories will be limited by thermal...
Amorphous silicon has ideal properties for many applications in fundamental research and industry. H...
Planned, cryogenic gravitational-wave detectors will require improved coatings with a strain thermal...
Current interferometric gravitational wave detectors use the combination of quasi-monochromatic, con...
Crystalline silicon is currently being discussed as test-mass material for future generations of gra...
Amorphous silicon (aSi) is a promising material for application in mirror coatings with low thermal ...
Crystalline silicon has been proposed as a new test mass material in third generation gravitational ...
Amorphous silicon has ideal properties for many applications in fundamental research and industry. H...
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 ...
The announcement of the direct detection of gravitational waves (GW) by the LIGO and Virgo collabora...
A key element for the next-generation gravitational wave interferometers are optical substrates char...
Abstract. The sensitivity of future gravitational wave (GW) observatories will be limited by thermal...
Amorphous silicon has ideal properties for many applications in fundamental research and industry. H...
Planned, cryogenic gravitational-wave detectors will require improved coatings with a strain thermal...
Current interferometric gravitational wave detectors use the combination of quasi-monochromatic, con...
Crystalline silicon is currently being discussed as test-mass material for future generations of gra...
Amorphous silicon (aSi) is a promising material for application in mirror coatings with low thermal ...
Crystalline silicon has been proposed as a new test mass material in third generation gravitational ...
Amorphous silicon has ideal properties for many applications in fundamental research and industry. H...