“…In the recent years, several DM direct detection experiments have reported potential signals for light WIMPs with masses around 1 ∼ 10 GeV, including DAMA [8,9], CoGeNT [10][11][12][13][14], CRESST-II [15] and CDMS-Si [16], while other experiments, such as LUX [17,18], SuperCDMS [19], CDMSlite [20,21], XENON10 [22], XENON100 [23,24], CDEX [25,26] and PandaX [27,28], have only presented null results. In order to reconcile the conflicts among the experiments, several mechanisms have been discussed, among which the isospinviolating interactions [30][31][32][33][34][35][36][37][38][39], exothermic scatterings [40][41][42][43][44][45][46] and the light WIMP-nuclus mediators [47,48] are the three main proposals. In particular, after the releases of the 2013 LUX [17] and 2014 SuperCDMS [19] data, it was found [33,45,…”