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Gravitational Waves from dark composite dynamics

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arxiv 2211.08877 v1 pith:FUXMGNLA submitted 2022-11-16 hep-ph astro-ph.COhep-lathep-th

Manuel Reichert , Zhi-Wei Wang This is my paper · ORCID
classification hep-phastro-ph.COhep-lathep-th
keywords gravitational-wavedarksignalallowsarbitrarybangchiralcolours
verification ladder T0 review T1 audit T2 compute T3 formal
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We discuss the stochastic gravitational-wave spectrum from dark confinement and chiral phase transitions in the early Universe. Specifically, we look at pure Yang-Mills theory for an arbitrary number of colours as well as SU(3) with quarks in different representations. We utilise thermodynamic lattice data and map it to effective models, such as the Polyakov-loop and the PNJL model. This allows us to compute gravitational-wave parameters and the corresponding gravitational-wave signal. We compare the signal to future gravitational-wave observatories such as the Big Bang Observer and DECIGO.

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Cited by 4 Pith papers

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

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    hep-th 2026-07 conditional novelty 7.0 of 10

    Non-conformal equations of state introduce wall and flow obstructions that delete entire classes of bubble solutions and create 'shocked detonations', shrinking the allowed wall-velocity space and suppressing gravitat...

  2. Meson spectroscopy in the $Sp(4)$ gauge theory with three antisymmetric fermions

    hep-lat 2024-12 conditional novelty 6.0 of 10

    Lattice simulations of Sp(4) with three antisymmetric Dirac fermions find QCD-like confinement and chiral symmetry breaking, and provide a first continuum-extrapolated meson spectrum.

  3. Updates on the density of states method in finite temperature symplectic gauge theories

    hep-lat 2024-11 conditional novelty 4.0 of 10

    LLR simulations of Sp(4) pure gauge theory at finite temperature show that the plaquette distribution at the deconfinement critical point has a plateau between the two peaks, and the thermodynamic extrapolations of th...

  4. Populating dark sectors with relativistic bubble walls

    hep-ph 2024-12 conditional novelty 3.0 of 10

    Relativistic bubble walls can pair-produce dark matter much heavier than the phase transition scale, which then free-streams as warm dark matter.

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