Figure 11
From: Cold atoms in space: community workshop summary and proposed road-map
Left panel: Sensitivities to the GWs from a network of cosmic strings with tension Gμ of AION-100 and -km, AEDGE [5] and AEDGE+ (a version of AEDGE that would use an ∼100m atomic cloud outside the spacecraft [252]), LIGO, ET and LISA. Right panel: Possible effects on the spectrum of GWs from cosmic strings with tension \(G\mu = 10^{-11}\) of an epoch of matter domination (MD) or of kination [252]