A Model of Anthropic Reasoning, Addressing the Dark to Ordinary Matter Coincidence
Frank Wilczek

TL;DR
This paper explores a multiverse-based model where inflation after Peccei-Quinn symmetry breaking allows large axion scales, potentially explaining the dark matter and baryon matter density coincidence.
Contribution
It proposes a novel multiverse scenario linking inflation timing and axion scale, offering an explanation for dark and baryon matter density coincidence.
Findings
Large axion scales are possible with post-Peccei-Quinn inflation.
Regions with small initial misalignment dominate observer count.
The model provides a potential explanation for dark and baryon matter density equality.
Abstract
If inflation occurs after the breaking of Peccei-Quinn symmetry then large values of the breaking scale , which are forbidden in conventional axion cosmology, are permitted, provided that we inhabit a region of the Multiverse where the initial misalignment is small. Regions having approximately this initial misalignment may occupy a small volume of the Multiverse, but they contain a large fraction of potential observers. This scenario has many consequences, including a possible explanation of the approximate equality of dark and baryon matter densities.
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Taxonomy
TopicsSemantic Web and Ontologies
