THERMAL EQUILIBRIUM AND KMS CONDITION AT THE PLANCK SCALE

Citation:

G. BOGDANOFF,I. BOGDANOFF.THERMAL EQUILIBRIUM AND KMS CONDITION AT THE PLANCK SCALE[J].Chinese Annals of Mathematics B,2003,24(2):267~274
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Authors:

G. BOGDANOFF; I. BOGDANOFF
Abstract: 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 must be considered as subject to the Kubo-Martin-Schwinger (KMS) condition. Consequently, in the interior of the KMS strip, i.e. from the scale $\calb=0$ to the scale $\calb=\ell_{Planck}$, the fourth coordinate $g_{44}$ must be considered as complex, the two real poles being $\calb=0$ and $\calb=\ell_{planck}$. This means that within the limits of the KMS strip, the Lorentzian and the Euclidean metric are 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.

Keywords:

KMS state, Planck scale, KMS strip

Classification:

35Q99
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