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 ...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.展开更多
文摘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.
