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arXiv · 2212.02662

Branch-Cut Cosmology and the Bekenstein Criterion

José A. de Freitas Pacheco·César A. Zen Vasconcellos·Peter O. Hess·Dimiter Hadjimichef·Benno Bodmann
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Abstract

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.

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José A. de Freitas Pacheco, César A. Zen Vasconcellos, Peter O. Hess, Dimiter Hadjimichef, Benno Bodmann. 2022-12-05. Branch-Cut Cosmology and the Bekenstein Criterion. https://doi.org/10.1002/asna.20220070

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