“…Present Bound (90%CL) Future Sensitivity BR(µ → eγ) 4.2 × 10 −13 (MEG 2016) [24] 4 × 10 −14 (MEG-II) [25] BR(τ → eγ) 3.3 × 10 −8 (BABAR 2010) [26] 10 −9 (BELLE-II) [27] BR(τ → µγ) 4.4 × 10 −8 (BABAR 2010) [26] 10 −9 (BELLE-II) [27] BR(µ → eee) 1.0 × 10 −12 (SINDRUM 1988) [28] 10 −16 Mu3E (PSI) [29] BR(τ → eee) 2.7 × 10 −8 (BELLE 2010) [30] 10 −9,−10 (BELLE-II) [27] BR(τ → µµµ) 2.1 × 10 −8 (BELLE 2010) [30] 10 −9,−10 (BELLE-II) [27] BR(τ → µη) 2.3 × 10 −8 (BELLE 2010) [31] 10 −9,−10 (BELLE-II) [27] CR(µ − e, Au) 7.0 × 10 −13 (SINDRUM II 2006) [32] CR(µ − e, Ti) 4.3 × 10 −12 (SINDRUM II 2004) [33] 10 −18 PRISM (J-PARC) [34] CR(µ − e, Al) 3.1 × 10 −15 COMET-I (J-PARC) [35] 2.6 × 10 −17 COMET-II (J-PARC) [35] 2.5 × 10 −17 Mu2E (Fermilab) [36] BR(Z → µe) 1.7 × 10 −6 (LEP 1995) [37], 7.5 × 10 −7 (ATLAS 2014) [9] BR(Z → τ e) 9.8 × 10 −6 (LEP 1995) [37] BR(Z → τ µ) 1.2 × 10 −5 (LEP 1995) [38], 1.69 × 10 −5 (ATLAS 2014) [39] BR(H → µe) 3.6 × 10 −3 (CMS 2015) [40] BR(H → τ e) 1.04 × 10 −2 (ATLAS 2016) [39], 0.7 × 10 −2 (CMS 2015) [40] BR(H → τ µ) 1.43 × 10 −2 (ATLAS 2016) [39], 1.51 × 10 −2 (CMS 2015) [41] In this work, we consider the Inverse Seesaw (ISS) [14,[42][43][44] as a specific realization of the low scale seesaw models. In particular, the ISS extends the SM spectrum with three pairs of RH neutrinos with opposite lepton numbers and considers Majorana masses for some of these new fields, which are assumed to be naturally small since they are the only masses that violate LN.…”