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arXiv quant-ph/9904053quant-phgr-qc
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干涉型引力波探测器中具有海森堡限制光子计数噪声的最佳光功率的降低

Reduction of optimum light power with Heisenberg-limited photon-counting noise in interferometric gravitational-wave detectors

Constantin Brif

摘要:

我们研究了量子噪声的行为,提出了干涉引力波探测器的灵敏度的基本限制,依赖于输入光的状态的属性。我们分析的情况下,特别准备的非经典输入状态,减少光子计数噪声的海森堡极限。与通常的配置相比,这导致实现标准量子极限所需的最佳光功率的大幅降低。

英文摘要:

We study how the behavior of quantum noise, presenting the fundamental limit on the sensitivity of interferometric gravitational-wave detectors, depends on properties of input states of light. We analyze the situation with specially prepared nonclassical input states which reduce the photon-counting noise to the Heisenberg limit. This results in a great reduction of the optimum light power needed to achieve the standard quantum limit, compared to the usual configuration.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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