Dark matter as a QCD effect in an anti de Sitter geometry: Cosmogonic implications of de Sitter, anti de Sitter and Poincaré symmetries

The $\Lambda$CDM standard model of cosmology involves two dark components of the universe, dark energy and dark matter. Whereas dark energy is usually associated with the (positive) cosmological constant $\Lambda$ associated with a de Sitter geometry, we propose to explain dark matter as a pure QCD...

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Main Author: Gilles Cohen-Tanoudji, Jean-Pierre Gazeau
Format: Article
Language:English
Published: SciPost 2023-11-01
Series:SciPost Physics Proceedings
Online Access:https://scipost.org/SciPostPhysProc.14.004
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author Gilles Cohen-Tanoudji, Jean-Pierre Gazeau
author_facet Gilles Cohen-Tanoudji, Jean-Pierre Gazeau
author_sort Gilles Cohen-Tanoudji, Jean-Pierre Gazeau
collection DOAJ
description The $\Lambda$CDM standard model of cosmology involves two dark components of the universe, dark energy and dark matter. Whereas dark energy is usually associated with the (positive) cosmological constant $\Lambda$ associated with a de Sitter geometry, we propose to explain dark matter as a pure QCD effect, namely a gluonic Bose Einstein condensate with the status of a Cosmic Gluonic Background (CGB). This effect is due to the trace anomaly viewed as an effective negative cosmological constant determining an Anti de Sitter geometry and accompanying baryonic matter at the hadronization transition from the quark gluon plasma phase to the colorless hadronic phase. Our approach also allows to assume a ratio Dark/Visible equal to 11/2.
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spelling doaj.art-9ab457d267f043d7980b3e11da53a1f22023-11-23T09:25:27ZengSciPostSciPost Physics Proceedings2666-40032023-11-011400410.21468/SciPostPhysProc.14.004Dark matter as a QCD effect in an anti de Sitter geometry: Cosmogonic implications of de Sitter, anti de Sitter and Poincaré symmetriesGilles Cohen-Tanoudji, Jean-Pierre GazeauThe $\Lambda$CDM standard model of cosmology involves two dark components of the universe, dark energy and dark matter. Whereas dark energy is usually associated with the (positive) cosmological constant $\Lambda$ associated with a de Sitter geometry, we propose to explain dark matter as a pure QCD effect, namely a gluonic Bose Einstein condensate with the status of a Cosmic Gluonic Background (CGB). This effect is due to the trace anomaly viewed as an effective negative cosmological constant determining an Anti de Sitter geometry and accompanying baryonic matter at the hadronization transition from the quark gluon plasma phase to the colorless hadronic phase. Our approach also allows to assume a ratio Dark/Visible equal to 11/2.https://scipost.org/SciPostPhysProc.14.004
spellingShingle Gilles Cohen-Tanoudji, Jean-Pierre Gazeau
Dark matter as a QCD effect in an anti de Sitter geometry: Cosmogonic implications of de Sitter, anti de Sitter and Poincaré symmetries
SciPost Physics Proceedings
title Dark matter as a QCD effect in an anti de Sitter geometry: Cosmogonic implications of de Sitter, anti de Sitter and Poincaré symmetries
title_full Dark matter as a QCD effect in an anti de Sitter geometry: Cosmogonic implications of de Sitter, anti de Sitter and Poincaré symmetries
title_fullStr Dark matter as a QCD effect in an anti de Sitter geometry: Cosmogonic implications of de Sitter, anti de Sitter and Poincaré symmetries
title_full_unstemmed Dark matter as a QCD effect in an anti de Sitter geometry: Cosmogonic implications of de Sitter, anti de Sitter and Poincaré symmetries
title_short Dark matter as a QCD effect in an anti de Sitter geometry: Cosmogonic implications of de Sitter, anti de Sitter and Poincaré symmetries
title_sort dark matter as a qcd effect in an anti de sitter geometry cosmogonic implications of de sitter anti de sitter and poincare symmetries
url https://scipost.org/SciPostPhysProc.14.004
work_keys_str_mv AT gillescohentanoudjijeanpierregazeau darkmatterasaqcdeffectinanantidesittergeometrycosmogonicimplicationsofdesitterantidesitterandpoincaresymmetries