Dark matter in the form of axion quark nuggets : formation, detections, and evidence ...

Over two decades of development since its establishment, the axion quark nugget (AQN) model is one of the best-studied macroscopic dark matter (DM) candidates, with a mass of grams and a size of around 0.1 micrometres. It naturally explains the observed similarity between the dark and visible densit...

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Main Author: Liang, Xunyu
Format: Text
Language:English
Published: University of British Columbia 2022
Subjects:
Online Access:https://dx.doi.org/10.14288/1.0418614
https://doi.library.ubc.ca/10.14288/1.0418614
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spelling ftdatacite:10.14288/1.0418614 2024-04-28T07:58:36+00:00 Dark matter in the form of axion quark nuggets : formation, detections, and evidence ... Liang, Xunyu 2022 https://dx.doi.org/10.14288/1.0418614 https://doi.library.ubc.ca/10.14288/1.0418614 en eng University of British Columbia article-journal Text ScholarlyArticle 2022 ftdatacite https://doi.org/10.14288/1.0418614 2024-04-02T09:31:21Z Over two decades of development since its establishment, the axion quark nugget (AQN) model is one of the best-studied macroscopic dark matter (DM) candidates, with a mass of grams and a size of around 0.1 micrometres. It naturally explains the observed similarity between the dark and visible densities in the Universe, i.e. Ωᴅᴍ~Ω????i????, with no fitting parameters, while many conventional DM candidates such as the weakly interacting massive particles (WIMPs) and axions do not. This dissertation presents numerous key developments of the AQN model, including the formation mechanism for AQNs in the early Universe and new search strategies such as axion detection and a global network of synchronized detectors. Lastly, we discuss potential evidence of AQNs from the anomalous events recently observed by the Telescope Array (TA) and ANtarctic Impulse Transient Antenna (ANITA) experiments. ... Text Antarc* Antarctic DataCite Metadata Store (German National Library of Science and Technology)
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description Over two decades of development since its establishment, the axion quark nugget (AQN) model is one of the best-studied macroscopic dark matter (DM) candidates, with a mass of grams and a size of around 0.1 micrometres. It naturally explains the observed similarity between the dark and visible densities in the Universe, i.e. Ωᴅᴍ~Ω????i????, with no fitting parameters, while many conventional DM candidates such as the weakly interacting massive particles (WIMPs) and axions do not. This dissertation presents numerous key developments of the AQN model, including the formation mechanism for AQNs in the early Universe and new search strategies such as axion detection and a global network of synchronized detectors. Lastly, we discuss potential evidence of AQNs from the anomalous events recently observed by the Telescope Array (TA) and ANtarctic Impulse Transient Antenna (ANITA) experiments. ...
format Text
author Liang, Xunyu
spellingShingle Liang, Xunyu
Dark matter in the form of axion quark nuggets : formation, detections, and evidence ...
author_facet Liang, Xunyu
author_sort Liang, Xunyu
title Dark matter in the form of axion quark nuggets : formation, detections, and evidence ...
title_short Dark matter in the form of axion quark nuggets : formation, detections, and evidence ...
title_full Dark matter in the form of axion quark nuggets : formation, detections, and evidence ...
title_fullStr Dark matter in the form of axion quark nuggets : formation, detections, and evidence ...
title_full_unstemmed Dark matter in the form of axion quark nuggets : formation, detections, and evidence ...
title_sort dark matter in the form of axion quark nuggets : formation, detections, and evidence ...
publisher University of British Columbia
publishDate 2022
url https://dx.doi.org/10.14288/1.0418614
https://doi.library.ubc.ca/10.14288/1.0418614
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