Forecast constraints on cosmic string parameters from gravitational wave   direct detection experiments
  Gravitational waves (GWs) are one of the key signatures of cosmic strings. If GWs from cosmic strings are detected in future experiments, not only their existence can be confirmed but also their properties might be probed. In this paper, we study the determination of cosmic string parameters through direct detection of GW signatures in future ground-based GW experiments. We consider two types of GWs, bursts and the stochastic GW background, which provide us with different information about cosmic string properties. Performing the Fisher matrix calculation on the cosmic string parameters, such as parameters governing the string tension $G\mu$ and initial loop size $\alpha$ and the reconnection probability $p$, we find that the two different types of GW can break degeneracies in some of these parameters and provide better constraints than those from each measurement. 
Sachiko Kuroyanagi, Koichi Miyamoto, Toyokazu Sekiguchi, Keitaro   Takahashi, Joseph Silk
astro-ph.CO gr-qc hep-ph hep-th