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Polarized Gravitational Waves from Cosmological Phase Transitions
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We estimate the degree of circular polarization for the gravitational waves generated during the electroweak and QCD phase transitions from the kinetic and magnetic helicity generated by bubble collisions during those cosmological phase transitions.
Forward citations
Cited by 7 Pith papers
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New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions
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Gravitational Waves from Confinement in $SU(N)$ Yang-Mills Theory
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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Gravitational waves from a first-order phase transition of the inflaton
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Gamma-Rays and Gravitational Waves from Inelastic Higgs Portal Dark Matter
An inelastic complex-scalar Higgs portal dark matter model can evade direct detection, explain the Galactic Center gamma-ray excess, and produce a first-order electroweak phase transition with a gravitational wave sig...
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Can a secluded self-interacting dark sector generate detectable gravitational waves?
In a secluded self-interacting dark sector with a dark U(1)' and dark radiation, existing Neff and Lyman-alpha limits remove nearly all gravitational-wave-detectable parameter space; one charge assignment keeps a smal...
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