Branch‐cut cosmology and the Bekenstein Criterion

In this contribution, we address the implications of the Bekenstein Criterion in the branch‐cut cosmology. The impossibility of packaging energy and entropy according to the Bekenstein Criterion in a finite size makes the transition phase of the branch‐cut cosmology very peculiar, imposing a topolog...

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Published in:Astronomische Nachrichten 2023-01, Vol.344 (1-2), p.n/a
Main Authors: Freitas Pacheco, José A., Zen Vasconcellos, César A., Hess, Peter O., Hadjimichef, Dimiter, Bodmann, Benno
Format: Article
Language:English
Subjects:
Bekenstein bound
branch‐cut cosmology
Cosmology
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Summary:In this contribution, we address the implications of the Bekenstein Criterion in the branch‐cut cosmology. The impossibility of packaging energy and entropy according to the Bekenstein Criterion in a finite size makes the transition phase of the branch‐cut cosmology very peculiar, imposing a topological leap between the contraction and expansion phases of the primordial universe or a transition region similar to a wormhole, with space–time shaping itself topologically in the format of a helix‐format around a branch point. Singularity means that there is no way for space–time to begin smoothly. The branch‐cut cosmology alternatively proposes a non‐temporal beginning at all, a pure space configuration, through a Wick rotation which replaces the imaginary time component by the temperature, the cosmological time.
ISSN:0004-6337
1521-3994
DOI:10.1002/asna.20220070