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Wheeler's it from bit proposal in loop quantum gravity

机译:惠勒的循环量子重力的比特提案

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摘要

As an attempt to realize Wheeler's "it-from-bit proposal" that physics should be reduced to simple yes-no questions, we consider a model of loop quantum gravity, where the only allowed values of the quantum numbers j(p) at the punctures p of the spin network on the spacelike two surfaces of spacetime are 0 and 1/2. When j(p) = 0, the puncture is in the vacuum, and it does not contribute to the area of the two surface, whereas when j(p) = 1/2, the puncture is in an excited state, and the allowed values of the associated quantum number m(p) are -1/2 and +1/2. As a consequence, the spin network used as a model of spacetime is analogous to a system of particles with spin 1/2, and every puncture carries exactly one bit of information. When applied to spacetimes with horizon, our model enables us to find an explicit expression for the partition function of spacetime. Using this partition function we may, among other things, obtain the Bekenstein-Hawking entropy law for black holes. When applied to cosmological models with horizon, the partition function predicts a cosmic phase transition in the early universe, where the cosmological constant went through a dramatic decrease and the matter of the universe was created out of the vacuum.
机译:作为实现Wheeler的“IT-From-Bit提议”的尝试,物理学应减少到简单的是 - 否问题,我们考虑了环路量子重力的模型,其中量子号j(p)的唯一允许值Spacelike上的Spacelike上的旋转网络的刺穿P为0和1/2。当j(p)= 0时,穿刺在真空中,它没有贡献两种表面的面积,而当j(p)= 1/2时,穿刺处于激励状态,允许的相关量子数m(p)的值是-1/2和+1/2。结果,用作时空模型的旋转网络类似于旋转1/2的颗粒系统,并且每个穿刺都恰好地带有一点信息。当使用Horizo​​ n应用于Spacetime时,我们的模型使我们能够找到Spacetime分区功能的显式表达式。使用本分区功能,我们可以在其他方面获得黑洞的Bekenstein-Hapking熵法。当应用于地平线的宇宙学模型时,分区功能预测了早期宇宙中的宇宙阶段过渡,其中宇宙学常数经历了戏剧性的减少,宇宙的问题被创造出真空。

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