Affiliation:
1. The University of Adelaide
2. The Australian Research Council Centre of Excellence for Gravitational Wave Discovery
Abstract
Future gravitational wave detectors (GWDs) require low noise, single
frequency, continuous wave lasers with excellent beam quality and
powers in excess of 500 W. Low noise laser amplifiers with high
spatial purity have been demonstrated up to 300 W. For higher powers,
coherent beam combination can overcome scaling limitations. In this
Letter we introduce a new, to the best of our knowledge, combination
scheme that uses a bow-tie resonator to combine three laser beams with
simultaneous spatial filtering performance.
Funder
Deutsche
Forschungsgemeinschaft
National Science Foundation
Australian Research Council
Subject
Atomic and Molecular Physics, and Optics