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Cosmological Phase Transition of Spontaneous Confinement

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arxiv 1910.06238 v2 pith:VN32OJ5O submitted 2019-10-14 hep-ph hep-th

classification hep-phhep-th
keywords transitionphaseconfinementassociatedcompositecosmologicaldilatondiscussed
verification ladder T0 review T1 audit T2 compute T3 formal
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The dynamics of a cosmological (de)confinement phase transition is studied in nearly conformally invariant field theories, where confinement is predominantly spontaneously generated and associated with a light "dilaton" field. We show how the leading contribution to the transition rate can be computed within the dilaton effective theory. In the context of Composite Higgs theories, we demonstrate that a simple scenario involving two renormalization-group fixed points can make the transition proceed much more rapidly than in the minimal scenario, thereby avoiding excessive dilution of matter abundances generated before the transition. The implications for gravitational wave phenomenology are discussed. In general, we find that more (less) rapid phase transitions are associated with weaker (stronger) gravitational wave signals. The various possible features of the strongly coupled composite Higgs phase transition discussed here can be concretely modeled at weak coupling within the AdS/CFT dual Randall-Sundrum extra-dimensional description, which offers important insights into the nature of the transition and its theoretical control. These aspects will be presented in a companion paper.

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Cited by 5 Pith papers

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

  1. Conformal Freeze-in Dark Matter: 5D Dual and Phase Transition

    hep-ph 2025-02 conditional novelty 7.0 of 10

    The authors construct a 5D Randall-Sundrum holographic dual of Conformal Freeze-In dark matter, find two branches of boundary CFTs, and show the dark confinement phase transition completes without significant supercoo...

  2. Probing Confining Dark Sectors with Cosmological Perturbations

    hep-ph 2026-06 unverdicted novelty 6.0 of 10

    Composite dark matter from a keV–MeV confining phase transition sources an IR-enhanced curvature spectrum that competes with free-streaming suppression, yielding concrete CMB and Lyman-α bounds on transition strength ...

  3. Primordial Black Hole from Tensor-induced Density Fluctuation: First-order Phase Transitions and Domain Walls

    astro-ph.CO 2026-05 unverdicted novelty 6.0 of 10

    Tensor perturbations from FOPT and domain-wall sources are claimed to induce second-order scalar perturbations large enough to form primordial black holes, potentially all of the dark matter.

  4. Confinement in Holographic Theories at Finite Theta

    hep-th 2026-03 unverdicted novelty 6.0 of 10

    Holographic 5D model shows confinement critical temperature falls quadratically with vacuum angle, matches lattice QCD, and allows time-dependent theta to trigger supercooling and altered gravitational-wave spectra.

  5. Gravitational Waves from Confinement in $SU(N)$ Yang-Mills Theory

    hep-ph 2025-12 conditional novelty 6.0 of 10

    For pure SU(N) Yang-Mills dark sectors, confinement transitions produce gravitational waves too weak for LISA, ET, CE, DECIGO or BBO, with peak amplitude at N≈20 and a large-N decay h²Ω_peak ∝ N^{-14/3}.

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