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Gravitational waves and monopoles dark matter from first-order phase transition
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We study the possibility of monopoles serving as dark matter when they are produced during the first-order phase transition in the dark sector. Our study shows that dark monopoles can contribute only a small piece of dark matter relic density within parameter spaces where strong gravitational waves can be probed by ET and CE, and the monopoles can contribute a sizable component of the observed dark matter relic density for fast phase transitions with short duration.
Forward citations
Cited by 3 Pith papers
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Self-Consistent Parker Bound on Magnetic Monopoles
A self-consistent Parker bound on magnetic monopoles is derived using the galactic mean-field dynamo eigenmode and turbulent field seeding and acceleration, producing modified flux limits at low and intermediate masse...
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No room for minimal monopole dark matter
In the minimal SO(3) 't Hooft-Polyakov dark sector, the relic abundance of the stable electrically charged W' boson always exceeds the magnetic monopole abundance, so dark monopoles cannot be the dominant dark matter.
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The price for monopole dark matter
Dark matter can consist of 't Hooft-Polyakov monopoles in a dark SU(2) sector, but only in a narrow window with m_M ≳ 10^8 GeV, near-bound dark radiation, and possibly detectable gravitational waves.
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