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2020

Gravitational waves from colliding vacuum bubbles in gauge theories

Lewicki, Marek, Vaskonen, Ville

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We study production of gravitational waves (GWs) in strongly supercooled cosmological phase transitions in gauge theories.

We extract from two-bubble lattice simulations the scaling of the GW source, and use it in many-bubble simulations in the thin-wall limit to estimate the resulting GW spectrum.
We find that in presence of the gauge field the GW source decays with bubble radius as $\propto R^{-3}$ after collisions.
This leads to a GW spectrum that follows $\Omega_{\rm GW} \propto \omega^{2.3}$ at low frequencies and $\Omega_{\rm GW} \propto \omega^{-2.4}$ at high frequencies, marking a significant deviation from the popular envelope approximation.

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