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Autori principali: Jiang, Siyu, Huang, Fa Peng, Ko, Pyungwon
Natura: Preprint
Pubblicazione: 2024
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Accesso online:https://arxiv.org/abs/2404.16509
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author Jiang, Siyu
Huang, Fa Peng
Ko, Pyungwon
author_facet Jiang, Siyu
Huang, Fa Peng
Ko, Pyungwon
contents As a new type of dynamical dark matter mechanism, we discuss the stability of the gauged Q-ball dark matter and its production mechanism through a cosmological first-order phase transition. This work delves into the study of gauged Q-ball dark matter generated during the cosmic phase transition. We demonstrate detailed discussions on the stability of gauged Q-balls to rigorously constrain their charge and mass ranges. Additionally, employing analytic approximations and the mapping method, we provide qualitative insights into gauged Q-balls. We establish an upper limit on the gauge coupling constant and give the relic density of stable gauged Q-ball dark matter formed during a first-order phase transition. Furthermore, we discuss potential observational signatures or constraints of gauged Q-ball dark matter, including astronomical observations and gravitational wave signals.
format Preprint
id arxiv_https___arxiv_org_abs_2404_16509
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Gauged Q-ball dark matter through a cosmological first-order phase transition
Jiang, Siyu
Huang, Fa Peng
Ko, Pyungwon
High Energy Physics - Phenomenology
As a new type of dynamical dark matter mechanism, we discuss the stability of the gauged Q-ball dark matter and its production mechanism through a cosmological first-order phase transition. This work delves into the study of gauged Q-ball dark matter generated during the cosmic phase transition. We demonstrate detailed discussions on the stability of gauged Q-balls to rigorously constrain their charge and mass ranges. Additionally, employing analytic approximations and the mapping method, we provide qualitative insights into gauged Q-balls. We establish an upper limit on the gauge coupling constant and give the relic density of stable gauged Q-ball dark matter formed during a first-order phase transition. Furthermore, we discuss potential observational signatures or constraints of gauged Q-ball dark matter, including astronomical observations and gravitational wave signals.
title Gauged Q-ball dark matter through a cosmological first-order phase transition
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2404.16509