宇宙视界的投射发生于普朗克尺度，所以在我们所在的时空尺度上，这一投射发生了模糊。
The projection starts off at Planck scale lengths at the Universe’s event horizon, but its projection becomes blurry in our local space-time.
要验证这一点，我们需要深入到普朗克尺度(10 - 35米)进行探测，而GEO600实验中探测到的噪音尺度为不到10 - 15米。
At its finest scale, we should be able to probe down the "Planck length" which measures 10-35 meters. But the GEO600 experiment detected noise at scales of less than 10-15 meters.
要验证这一点，我们需要深入到普朗克尺度(10 - 35米)进行探测，而GEO600实验中探测到的噪音尺度为不到10 - 15米。
At its finest scale, we should be able to probe down the "Planck length" which measures 10-35 meters. But the GEO600 experiment detected noise at scales of less than 10-15 meters.
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