The ANITA Anomalous Events and Axion Quark Nuggets
The Antarctic Impulse Transient Antenna (\textsc{ANITA}) collaboration \cite{Gorham:2016zah,Gorham:2018ydl,Gorham:2020zne} have reported observation of two anomalous events with noninverted polarity. These events are proven to be hard to explain in terms of conventional cosmic rays (CR). We propose...
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ftdatacite:10.48550/arxiv.2105.01668 2023-05-15T14:00:39+02:00 The ANITA Anomalous Events and Axion Quark Nuggets Liang, Xunyu Zhitnitsky, Ariel 2021 https://dx.doi.org/10.48550/arxiv.2105.01668 https://arxiv.org/abs/2105.01668 unknown arXiv Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 CC-BY High Energy Physics - Phenomenology hep-ph High Energy Astrophysical Phenomena astro-ph.HE Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences Article CreativeWork article Preprint 2021 ftdatacite https://doi.org/10.48550/arxiv.2105.01668 2022-03-10T14:15:45Z The Antarctic Impulse Transient Antenna (\textsc{ANITA}) collaboration \cite{Gorham:2016zah,Gorham:2018ydl,Gorham:2020zne} have reported observation of two anomalous events with noninverted polarity. These events are proven to be hard to explain in terms of conventional cosmic rays (CR). We propose that these anomalous events represent the direct manifestation of the dark matter (DM) annihilation events within the so-called axion quark nugget (AQN) DM model, which was originally invented for completely different purpose to explain the observed similarity between the dark and the visible components in the Universe, i.e. $Ω_{\rm DM}\sim Ω_{\rm visible}$ without any fitting parameters. We support this proposal by demonstrating that the observations \cite{Gorham:2016zah,Gorham:2018ydl,Gorham:2020zne}, including the frequency, intensity and time duration of the radio pulses nicely match the emission features of the upward going AQN events. We list a number of features of the AQN events which are very distinct from conventional CR air showers. The observations (non-observation) of these features may substantiate (refute) our proposal. : 15 pages, 5 figures Article in Journal/Newspaper Antarc* Antarctic DataCite Metadata Store (German National Library of Science and Technology) Antarctic Gorham ENVELOPE(-62.052,-62.052,-74.044,-74.044) The Antarctic |
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DataCite Metadata Store (German National Library of Science and Technology) |
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High Energy Physics - Phenomenology hep-ph High Energy Astrophysical Phenomena astro-ph.HE Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences |
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High Energy Physics - Phenomenology hep-ph High Energy Astrophysical Phenomena astro-ph.HE Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences Liang, Xunyu Zhitnitsky, Ariel The ANITA Anomalous Events and Axion Quark Nuggets |
topic_facet |
High Energy Physics - Phenomenology hep-ph High Energy Astrophysical Phenomena astro-ph.HE Instrumentation and Methods for Astrophysics astro-ph.IM FOS Physical sciences |
description |
The Antarctic Impulse Transient Antenna (\textsc{ANITA}) collaboration \cite{Gorham:2016zah,Gorham:2018ydl,Gorham:2020zne} have reported observation of two anomalous events with noninverted polarity. These events are proven to be hard to explain in terms of conventional cosmic rays (CR). We propose that these anomalous events represent the direct manifestation of the dark matter (DM) annihilation events within the so-called axion quark nugget (AQN) DM model, which was originally invented for completely different purpose to explain the observed similarity between the dark and the visible components in the Universe, i.e. $Ω_{\rm DM}\sim Ω_{\rm visible}$ without any fitting parameters. We support this proposal by demonstrating that the observations \cite{Gorham:2016zah,Gorham:2018ydl,Gorham:2020zne}, including the frequency, intensity and time duration of the radio pulses nicely match the emission features of the upward going AQN events. We list a number of features of the AQN events which are very distinct from conventional CR air showers. The observations (non-observation) of these features may substantiate (refute) our proposal. : 15 pages, 5 figures |
format |
Article in Journal/Newspaper |
author |
Liang, Xunyu Zhitnitsky, Ariel |
author_facet |
Liang, Xunyu Zhitnitsky, Ariel |
author_sort |
Liang, Xunyu |
title |
The ANITA Anomalous Events and Axion Quark Nuggets |
title_short |
The ANITA Anomalous Events and Axion Quark Nuggets |
title_full |
The ANITA Anomalous Events and Axion Quark Nuggets |
title_fullStr |
The ANITA Anomalous Events and Axion Quark Nuggets |
title_full_unstemmed |
The ANITA Anomalous Events and Axion Quark Nuggets |
title_sort |
anita anomalous events and axion quark nuggets |
publisher |
arXiv |
publishDate |
2021 |
url |
https://dx.doi.org/10.48550/arxiv.2105.01668 https://arxiv.org/abs/2105.01668 |
long_lat |
ENVELOPE(-62.052,-62.052,-74.044,-74.044) |
geographic |
Antarctic Gorham The Antarctic |
geographic_facet |
Antarctic Gorham The Antarctic |
genre |
Antarc* Antarctic |
genre_facet |
Antarc* Antarctic |
op_rights |
Creative Commons Attribution 4.0 International https://creativecommons.org/licenses/by/4.0/legalcode cc-by-4.0 |
op_rightsnorm |
CC-BY |
op_doi |
https://doi.org/10.48550/arxiv.2105.01668 |
_version_ |
1766269881174458368 |