Figure 12From: Cold atoms in space: community workshop summary and proposed road-mapLeft panel: Sensitivities of AION-100 and -km, AEDGE, AEDGE+ and LISA in the \((T_{*}, \alpha )\) plane to GWs from generic first-order transitions with a transition rate \(\beta /H = 100\) [260]. Right panel: The expected signal-to-noise ratio (SNR) with AEDGE for observing the stochastic GW background from a U(1)\(_{B-L}\)-breaking phase transition. In the red regions SNR >1000 and the solid gray contour corresponds to SNR =10 [260]Back to article page