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Quantum gravity, minimum length and holography

机译:量子重力,最小长度和全息术

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The Karolyhazy uncertainty relation states that if a device is used to measure a length $l$, there will be a minimum uncertainty $delta l$ in the measurement, given by $(delta l)^3$ ~ $L^2_Pl$. This is a consequence of combining the principles of quantum mechanics and general relativity. In this letter we show how this relation arises in our approach to quantum gravity, in a bottom-up fashion, from the matrix dynamics of atoms of space–time–matter. We use this relation to define a space–time–matter (STM) foam at the Planck scale, and to argue that our theory is holographic. By coarse graining over time-scales larger than Planck time, one obtains the laws of quantum gravity. Quantum gravity is not a Planck scale phenomenon; rather it comes into play whenever classical space–time background is not available to describe a quantum system. Space–time and classical general relativity arise from spontaneous localisation in a highly entangled quantum gravitational system. The Karolyhazy relation continues to hold in the emergent theory. An experimental confirmation of this relation will constitute a definitive test of the quantum nature of gravity.
机译:karolyhazy不确定性关系指出,如果使用设备来测量长度$ l $,则以$( delta l)^ 3 $〜$ l ^ 2_pl给出了测量中的最小不确定性$ delta l $。 $。这是结合量子力学和一般相对性的原理的结果。在这封信中,我们展示了这种关系如何在我们的空间时代的原子的基质动态中以自下而上的方式在量子重力方面产生这种关系。我们使用这一关系来定义普朗克规模的时空(STM)泡沫,并争辩说我们的理论是全息的。通过比普朗克时间大的时间尺度粗糙的粗糙度,获得量子重力定律。量子重力不是普朗克规模的现象;相反,只要经典的时空背景不可用以描述量子系统,它就会发挥作用。空间时间和经典一般相对性来自高度缠绕的量子重力系统中的自发定位。 karolyhazy关系继续持有紧急理论。这种关系的实验证实将构成对重力的量子性质的最终试验。

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