Rainer Weiss analyzed a broadband interferometric detector for gravitational waves. His 1972 report compared the response of separated freely moving masses with an optical readout, and calculated competing sources of instrumental noise.
A gravitational wave produces a differential change in the arms of an interferometer; the associated phase change in laser light supplies the observable. The difficulty is distinguishing that tiny relative response from mirror motion, thermal fluctuations and optical noise. Treating the signal and its noise budget together made the proposal a testable instrument design.[ref]
Figure 1.
Portrait of Rainer Weiss
. Michael Hauser; required Commons attribution Dhs at English Wikipedia; existing crop by Neegzistuoja and level adjustment by WikiPedant. Creative Commons Attribution-ShareAlike 3.0 Unported (selected from Commons GFDL migration licensing)., via Wikimedia Commons. Source.

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Rainer Weiss is a prominent American physicist known for his contributions to the field of gravitational physics and astrophysics. He is best known as one of the co-founders of the Laser Interferometer Gravitational-Wave Observatory (LIGO), which made groundbreaking discoveries in the detection of gravitational waves. This achievement, announced in 2015, confirmed a key prediction of Albert Einstein's general theory of relativity and opened a new era in astrophysics.