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The kinetic theory of the mesoscopic spacetime

机译:介观空间的动力学理论

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摘要

At the mesoscopic scales — which interpolate between the macroscopic, classical, geometry and the microscopic, quantum, structure of spacetime — one can identify the density of states of the geometry, which arises from the existence of a zero-point length in the spacetime. This spacetime discreteness also associates an internal degree of freedom with each event, in the form of a fluctuating vector of constant norm. The equilibrium state, corresponding to the extremum of the total density of states of geometry plus matter, leads precisely to Einstein’s equations. In fact, the field equation can now be reinterpreted as a zero-heat-dissipation principle. The analysis of fluctuations around the equilibrium state (which is described by Einstein’s equations), will provide new insights about the quantum gravity.
机译:在介面阶段 - 在宏观,经典,几何形状和微观,时空的结构之间插值 - 一个 - 一个可以识别几何形状的状态的密度,从时空中存在零点长度的存在。 这种时空离散也以恒定规范的波动载体的形式与每个事件相关联的自由度。 对应于几何形状加质的总密度的极值的平衡状态,恰恰是爱因斯坦的方程。 事实上,现场方程现在可以作为零散热原理重新诠释。 围绕均衡状态的波动(由爱因斯坦方程描述)的波动将为对量子重力提供新的见解。

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