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Main Author: Van Waerbeke, Ludovic
Format: Preprint
Published: 2026
Subjects:
Online Access:https://arxiv.org/abs/2603.15585
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author Van Waerbeke, Ludovic
author_facet Van Waerbeke, Ludovic
contents The nature of dark matter remains a central problem in cosmology. A compelling possibility is that dark matter is macroscopic, consisting of composite objects formed in the early Universe. We introduce the QCD-AQN framework, a well-motivated scenario in which dark matter is composed of dense aggregates of quark and antiquark matter stabilised by axion domain walls. The framework proposes a unified explanation for both dark matter and the observed matter-antimatter asymmetry. Particular emphasis is placed on existing observational constraints and on observational tests. Finally, we explore a possible QCD-based scenario for dark energy.
format Preprint
id arxiv_https___arxiv_org_abs_2603_15585
institution arXiv
publishDate 2026
record_format arxiv
spellingShingle QCD-driven dark matter: AQNs formation and observational tests
Van Waerbeke, Ludovic
High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
The nature of dark matter remains a central problem in cosmology. A compelling possibility is that dark matter is macroscopic, consisting of composite objects formed in the early Universe. We introduce the QCD-AQN framework, a well-motivated scenario in which dark matter is composed of dense aggregates of quark and antiquark matter stabilised by axion domain walls. The framework proposes a unified explanation for both dark matter and the observed matter-antimatter asymmetry. Particular emphasis is placed on existing observational constraints and on observational tests. Finally, we explore a possible QCD-based scenario for dark energy.
title QCD-driven dark matter: AQNs formation and observational tests
topic High Energy Physics - Phenomenology
Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2603.15585