Enhanced Dark Matter Abundance in First-Order Phase Transitions

We propose a novel scenario to obtain the correct relic abundance for thermally under-produced dark matter. This scenario utilizes a strongly first-order phase transition at temperature $T_{\mathrm{P}\mathrm{T}}$ that gives rise to dark matter mass $m$. Freeze-out in the broken phase can yield the desired abundance in the entire region currently allowed by observational bounds and theoretical constraints for ${10}^2{T}_{\mathrm{P}\mathrm{T}}\lesssim m\lesssim {10}^4{T}_{\mathrm{P}\mathrm{T}}$. We show that the accompanying gravitational waves are strong enough to be detected by many upcoming and proposed experiments. This, in tandem with dark matter indirect searches, provides a multi-messenger probe of such models. Positive signals in the future can help reconstruct the potential governing the phase transition and shed light on an underlying particle physics realization.