Energetic Quantum Limit in Large-Scale Interferometers

(2) Theoretical Astrophysics; California Institute of Technology); Farid Ya. Khalili (1); Kip S. Thorne (2) ((1) Physics Faculty; Mikhail L. Gorodetsky (1); Moscow State University; Vladimir B. Braginsky (1)

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arxiv gr-qc/9907057 v2 pith:G33ALT5K submitted 1999-07-16 gr-qc quant-ph

Energetic Quantum Limit in Large-Scale Interferometers

Vladimir B. Braginsky (1) , Mikhail L. Gorodetsky (1) , Farid Ya. Khalili (1) , Kip S. Thorne (2) ((1) Physics Faculty , Moscow State University , (2) Theoretical Astrophysics , California Institute of Technology) This is my paper

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For each optical topology of an interferometric gravitational wave detector, quantum mechanics dictates a minimum optical power (the ``energetic quantum limit'') to achieve a given sensitivity. For standard topologies, when one seeks to beat the standard quantum limit by a substantial factor, the energetic quantum limit becomes impossibly large. Intracavity readout schemes may do so with manageable optical powers.

Energetic Quantum Limit in Large-Scale Interferometers

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