Predicting spatial curvature $Ω_K$ in globally $CPT$-symmetric universes

Fuente: arXiv
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Auteurs principaux: Deng, Wei-Ning, Handley, Will
Format: Preprint
Publié: 2024
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author Deng, Wei-Ning
Handley, Will
author_facet Deng, Wei-Ning
Handley, Will
contents Boyle and Turok's $CPT$-symmetric universe model posits that the universe was symmetric at the Big Bang, addressing numerous problems in both cosmology and the Standard Model of particle physics. We extend this model by incorporating the symmetric conditions at the end of the Universe, which impose constraints on the allowed perturbation modes. These constrained modes conflict with the integer wave vectors required by the global spatial geometry in a closed universe. To resolve this conflict, only specific values of curvature are permissible, and in particular the curvature density is constrained to be $Ω_K \in \{-0.014, -0.009, -0.003, \ldots\}$, consistent with Planck observations.
format Preprint
id arxiv_https___arxiv_org_abs_2407_18225
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Predicting spatial curvature $Ω_K$ in globally $CPT$-symmetric universes
Deng, Wei-Ning
Handley, Will
Cosmology and Nongalactic Astrophysics
Boyle and Turok's $CPT$-symmetric universe model posits that the universe was symmetric at the Big Bang, addressing numerous problems in both cosmology and the Standard Model of particle physics. We extend this model by incorporating the symmetric conditions at the end of the Universe, which impose constraints on the allowed perturbation modes. These constrained modes conflict with the integer wave vectors required by the global spatial geometry in a closed universe. To resolve this conflict, only specific values of curvature are permissible, and in particular the curvature density is constrained to be $Ω_K \in \{-0.014, -0.009, -0.003, \ldots\}$, consistent with Planck observations.
title Predicting spatial curvature $Ω_K$ in globally $CPT$-symmetric universes
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2407.18225