Domain Walls of Low Tension in Cosmology
Holger Bech Nielsen, Colin D. Froggatt

TL;DR
This paper explores the idea of multiple vacuum phases with low-tension domain walls in cosmology, proposing a dark matter model involving vacuum bubbles and discussing implications for cosmic observations and fundamental constants.
Contribution
It introduces a novel dark matter model based on vacuum bubbles with low-tension domain walls and connects this to cosmological observations and fundamental constant variations.
Findings
Estimated the order of magnitude of domain wall tension compatible with cosmology.
Suggested that early galaxy observations may support the vacuum bubble model.
Discussed the potential impact of domain walls replacing the cosmological constant.
Abstract
In the present article we put up for discussion the idea of there existing several versions, phases, of the vacuum, in the spirit in which we have long worked on this idea, namely the Multiple Point Criticality Principle, which also says that these different vacuum phases have the same energy density. We mention that we indeed predicted the Higgs mass to be 135 plus minus 10 GeV, which when measured turned out to be 125 GeV, using the assumption of this Multiple Point Criticality Principle. We consider the possibility that there is one type of vacuum in the galaxy clusters (the usual vacuum) and another type of vacuum in the voids. The hope that there could indeed be such a low tension S of the domain wall between these two phases, that it would not totally upset cosmology is based on our dark matter model. In this model dark matter consists of pearls or bubbles of a new vacuum phase,…
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Computational Physics and Python Applications
