【摘 要】
：
Considering the expected thermal equilibrium characterizing the physics at the Planck scale,it is here stated, for the first time, that, as a system, the space-
【机 构】
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Mathematical Physics Laboratory CNRS UPRES A 5029
【基金项目】
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the encouragement from Francois Combes, of the Mathematics Department of the University of Orleans;Daniel Sternheimer, of the University of Bourgogne;Jak Verbaarshot, of the University of Stony Broock
论文部分内容阅读
Considering the expected thermal equilibrium characterizing the physics at the Planck scale,it is here stated, for the first time, that, as a system, the space-time at the Planck scale mustbe considered as subject to the Kubo-Martin-Schwinger (KMS) condition. Consequently, inthe interior of the KMS strip, i.e. from the scale B = 0 to the scale B ＝ eplanck, the fourthcoordinate g44 must be considered as complex, the two real poles being B = 0 and B = eplanckThis means that within the limits of the KMS strip, the Lorentzian and the Euclidean metricare in a "quantum superposition state" (or coupled), this entailing a "unification" (or coupling)between the topological (Euclidean) and the physical (Lorentzian) states of space-time.
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