Unexpected Noise in Next-Generation Mirror Material

Abstract

N ext-generation gravitational-wave detectors need to be less noisy if they are going to help solve lingering mysteries about black holes and neutron stars. One avenue for reducing noise is to improve the quality of the reflective materials used to determine gravitational-wave-induced length changes in such detectors. Now tests of gallium arsenide, a promising alternative mirror substance, reveal an unexpected amount of noise in the light-reflection properties of thin films made from thematerial [1]. The experiments were performed at cryogenic temperatures, which are being considered for some—but not all—future gravitational-wave detectors. Further testing is needed to assess the potential impact of this new noise on mirror design choices.