Energetic Quantum Limit in Large-Scale Interferometers
广义相对论与量子宇宙学
2009-10-31 v2 量子物理
摘要
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.
引用
@article{arxiv.gr-qc/9907057,
title = {Energetic Quantum Limit in Large-Scale Interferometers},
author = {Vladimir B. Braginsky and Mikhail L. Gorodetsky and Farid Ya. Khalili and Kip S. Thorne},
journal= {arXiv preprint arXiv:gr-qc/9907057},
year = {2009}
}
备注
Revised version; to be published in Proceedings of the 1999 Edoardo Amaldi Conference on Gravitational Waves; 11 pages including figures; manuscript is RevTex; figures are .eps; an AIP style file is included