The Einstein Telescope standard siren simulations for $f(Q)$ cosmologies

To investigate the model and extra frictional effects in standard siren simulation of $f(Q)$ cosmologies, we simulated three types of standard siren data based on different fiducial models ($\mathrm{\Lambda }$CDM and $f(Q)$ models). Both effects are important in standard siren simulation. Explicitly, the $f(Q{)}_P$ and $f(Q{)}_E$ models need more observational data (e.g.growth factor) to further study. The $f(Q{)}_{PE}$ model could be ruled out by the EM data. And both the $f(Q{)}_{HT}$ models will be excluded by the future standard siren data.