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Spacetime Metric and the KMS Condition at the Planck Scale

✍ Scribed by Grichka Bogdanoff; Igor Bogdanoff

Publisher: Elsevier Science
Year: 2002
Tongue: English
Weight: 96 KB
Volume: 296
Category: Article
ISSN: 0003-4916
DOI: 10.1006/aphy.2001.6212

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✦ Synopsis

For the first time the present paper shows that the spacetime system must be considered as subject to the Kubo-Martin-Schwinger (KMS) condition at the Planck scale. Consequently in the interior of the KMS strip, i.e., from the scale ß = 0 to the scale ß = Planck , the fourth coordinate g 44 must be considered as complex, the two real poles being ß = 0 and ß = 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), thus entailing a "unification" (or coupling) between the topological (Euclidean) and the physical (Lorentzian) states of spacetime.

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