物理
普朗克长度
量子引力
干涉测量
噪音(视频)
量子
理论物理学
长度刻度
弦(物理)
宇宙
空格(标点符号)
比例(比率)
弦论
量子涨落
统计物理学
经典力学
量子力学
普朗克标度
计算机科学
图像(数学)
操作系统
人工智能
作者
Giovanni Amelino‐Camelia
出处
期刊:Nature
[Springer Nature]
日期:2001-04-01
卷期号:410 (6832): 1065-1067
被引量:64
摘要
Space-time 'foam' is a geometric picture of the smallest size scales in the Universe, which is characterized mainly by the presence of quantum uncertainties in the measurement of distances. All quantum-gravity theories should predict some kind of foam, but the description of the properties of this foam varies according to the theory, thereby providing a possible means of distinguishing between such theories. I previously showed that foam-induced distance fluctuations would introduce a new source of noise to the measurements of gravity-wave interferometers, but the theories are insufficiently developed to permit detailed predictions that would be of use to experimentalists. Here I propose a phenomenological approach that directly describes space-time foam, and which leads naturally to a picture of distance fluctuations that is independent of the details of the interferometer. The only unknown in the model is the length scale that sets the overall magnitude of the effect, but recent data already rule out the possibility that this length scale could be identified with the 'string length' (10-34 m < Ls < 10-33 m). Length scales even smaller than the 'Planck length' (LP approximately 10-35 m) will soon be probed experimentally.
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