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Beyond freeze-in: Dark Matter via inverse phase transition and gravitational wave signal

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arxiv 2104.13722 v3 pith:C6TQLPCK submitted 2021-04-28 hep-ph astro-ph.COgr-qchep-th

classification hep-phastro-ph.COgr-qchep-th
keywords darkgravitationalmatterinversephasetransitioncouplingdomain
verification ladder T0 review T1 audit T2 compute T3 formal
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We propose a novel scenario of Dark Matter production naturally connected with generation of gravitational waves. Dark Matter is modelled as a real scalar, which interacts with the hot primordial plasma through a portal coupling to another scalar field. For a particular sign of the coupling, this system exhibits an inverse second order phase transition. The latter leads to an abundant Dark Matter production, even if the portal interaction is so weak that the freeze-in mechanism is inefficient. The model predicts domain wall formation in the Universe, long time before the inverse phase transition. These domain walls have a tension decreasing with time, and completely disappear at the inverse phase transition, so that the problem of overclosing the Universe is avoided. The domain wall network emits gravitational waves with characteristics defined by those of Dark Matter. In particular, the peak frequency of gravitational waves is determined by the portal coupling constant, and falls in the observable range for currently planned gravitational wave detectors.

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Forward citations

Cited by 5 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Caustic formation in DBI models: Wave propagation on planar domain walls

    hep-th 2026-04 accept novelty 7.0 of 10

    Hyperbolic DBI remains caustic-free for generic waves on planar domain walls in 2D flat space and under realistic deformations; only hyperbolicity loss produces cusp caustics.

  2. Domain walls through different cosmologies

    astro-ph.CO 2026-07 accept novelty 6.5 of 10

    Domain-wall network area scales as S ≈ 2ξV/τ with ξ≈1.2 across cosmologies from dust to near-Minkowski, so the particle horizon—not H⁻¹—sets the correlation length and GW peak.

  3. Fixing IR tail of gravitational waves from domain walls

    gr-qc 2026-07 conditional novelty 6.0 of 10

    Per-mode time averaging after source shutdown removes nonphysical IR wiggles in simulated GW spectra from domain walls; PRS scaling yields incorrect spectra even with rescaled sources.

  4. Spontaneous Space-Time Parity Breaking Without Thermal Restoration

    hep-th 2025-07 conditional novelty 6.0 of 10

    A 2+1 dimensional QFT is constructed whose parity symmetry is unbroken at zero temperature but spontaneously breaks at all sufficiently high temperatures.

  5. About electroweak domain walls in Majoron models

    hep-ph 2025-06 conditional novelty 5.0 of 10

    Electroweak instantons alone do not produce Majoron domain walls; a tiny instanton mass from B+L breaking is cosmologically negligible and can act as a bias or dark energy.

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