A participant's history of gravitational wave detector development, explaining how the field converged on the technology and sensitivity needed to detect neutron star binary signals.
Einstein (1916), Sitzungsberichte der Königlich Preussichen Akademie der Wissenschaften Berlin, part 1: 688 – 696; A
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"Sufficiently Advanced Technology" for Gravitational Wave Detection
A participant's history of gravitational wave detector development, explaining how the field converged on the technology and sensitivity needed to detect neutron star binary signals.