Figure 6From: AEDGE: Atomic Experiment for Dark Matter and Gravity Exploration in SpaceLeft panel: Example of the GW spectrum in a classical scale-invariant extension of the SM with a massive \(Z^{\prime }\) boson, compared with various experimental sensitivities. The dashed line shows the contribution to the spectrum sourced by bubble collisions, the dot-dashed line shows the contribution from sound waves, and the dotted line shows the contribution from turbulence. Right panel: Examples of spectra with some other reheating temperatures after the transition that may be realized in the same modelBack to article page