Ultraheavy Atomic Dark Matter Freeze-Out through Rearrangement

Fuente: arXiv
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Autori principali: Qiu, Yu-Cheng, Sheng, Jie, Tan, Liang, Xing, Chuan-Yang
Natura: Preprint
Pubblicazione: 2023
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author Qiu, Yu-Cheng
Sheng, Jie
Tan, Liang
Xing, Chuan-Yang
author_facet Qiu, Yu-Cheng
Sheng, Jie
Tan, Liang
Xing, Chuan-Yang
contents Atomic dark matter is usually considered to be produced asymmetrically in the early Universe. In this work, we first propose that the symmetric atomic dark matter can be thermally produced through the freeze-out mechanism. The dominant atom anti-atom annihilation channel is the atomic rearrangement. It has a geometrical cross section much larger than that of elementary fermions. After the atomic formation, this annihilation process further depletes dark matter particles and finally freezes out. To give the observed dark matter relic, the dark atoms are naturally ultraheavy, ranging from $10^6$ to $10^{10} \,\mathrm{GeV}$.
format Preprint
id arxiv_https___arxiv_org_abs_2312_13758
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Ultraheavy Atomic Dark Matter Freeze-Out through Rearrangement
Qiu, Yu-Cheng
Sheng, Jie
Tan, Liang
Xing, Chuan-Yang
High Energy Physics - Phenomenology
Atomic dark matter is usually considered to be produced asymmetrically in the early Universe. In this work, we first propose that the symmetric atomic dark matter can be thermally produced through the freeze-out mechanism. The dominant atom anti-atom annihilation channel is the atomic rearrangement. It has a geometrical cross section much larger than that of elementary fermions. After the atomic formation, this annihilation process further depletes dark matter particles and finally freezes out. To give the observed dark matter relic, the dark atoms are naturally ultraheavy, ranging from $10^6$ to $10^{10} \,\mathrm{GeV}$.
title Ultraheavy Atomic Dark Matter Freeze-Out through Rearrangement
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2312.13758