Speaker
Keiko Kokeyama
(Cardiff University)
Description
The wavelength of 2um is a candidate for the next generation gravitational-wave detectors such as LIGO Voyager and Einstein Telescope. Although the technical leap of the wavelength change impacts almost all the optical components of laser interferometry, only a few investigations have been ongoing. This poster will present the R&D experiments planned in the Gravitational Exploration Institute, Cardiff University.
Primary author
Keiko Kokeyama
(Cardiff University)
