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University of Birmingham > Talks@bham > Astrophysics Talks Series > [Seminar]: ETpathfinder: A cryogenic testbed for interferometric gravitational-wave detectors
[Seminar]: ETpathfinder: A cryogenic testbed for interferometric gravitational-wave detectorsAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Lalitha Sairam. The third-generation of gravitational wave observatories, such as the Einstein Telescope (ET) and Cosmic Explorer, aim for an improvement in sensitivity of at least a factor of ten over a wide frequency range compared to the current advanced detectors. In order to inform the design of the 3G detectors and to develop and qualify their subsystems, dedicated test facilities are required. ETpathfinder prototype uses full interferometer configurations and aims to provide a high sensitivity facility in a similar environment as ET. Along with the interferometry at 1550 nm and silicon test masses, ETpathfinder will focus on cryogenic technologies, lasers and optics at 2090 nm and advanced quantum-noise reduction schemes. In my talk, I will present the status of ETpathfinder and the road towards ET, giving an outlook on the fascinating science of gravitational-wave astronomy. This talk is part of the Astrophysics Talks Series series. This talk is included in these lists:Note that ex-directory lists are not shown. |
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