The sensitivity of a resonant-mass gravitational radiation antenna coupled to a motion detector with given noise properties is calculated in detail. It is shown that the quantum-mechanical limit of linear amplifier performance implies an important restriction on the sensitivity for any system using a linear motion detector. For a signal frequency ωₐ, this fundamental limit requires that the gravitational radiation pulse be capable of driving the antenna from rest to an energy level exceeding 2ωₐ.
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R. P. Giffard (1976) studied this question.
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