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• W3137673973 abstract "We present a model of radiative neutrino masses which also resolves anomalies reported in $B$-meson decays, $R_{D^{(star)}}$ and $R_{K^{(star)}}$, as well as in muon $g-2$ measurement, $Delta a_mu$. Neutrino masses arise in the model through loop diagrams involving TeV-scale leptoquark (LQ) scalars $R_2$ and $S_3$. Fits to neutrino oscillation parameters are obtained satisfying all flavor constraints which also explain the anomalies in $R_{D^{(star)}}$, $R_{K^{(star)}}$ and $Delta a_mu$ within $1, sigma$. An isospin-3/2 Higgs quadruplet plays a crucial role in generating neutrino masses; we point out that the doubly-charged scalar contained therein can be produced in the decays of the $S_3$ LQ, which enhances its reach to 1.1 (6.2) TeV at $sqrt s=14$ TeV high-luminosity LHC ($sqrt s=100$ TeV FCC-hh). We also present flavor-dependent upper limits on the Yukawa couplings of the LQs to the first two family fermions, arising from non-resonant dilepton ($pp rightarrow ell^+ ell^-$) processes mediated by $t$-channel LQ exchange, which for 1 TeV LQ mass, are found to be in the range $(0.15 - 0.36)$. These limits preclude any explanation of $R_{D^{(star)}}$ through LQ-mediated $B$-meson decays involving $nu_e$ or $nu_mu$ in the final state. We also find that the same Yukawa couplings responsible for the chirally-enhanced contribution to $Delta a_mu$ give rise to new contributions to the SM Higgs decays to muon and tau pairs, with the modifications to the corresponding branching ratios being at (2-6)% level, which could be tested at future hadron colliders, such as HL-LHC and FCC-hh." @default.
• W3137673973 created "2021-03-29" @default.
• W3137673973 creator A5003764900 @default.
• W3137673973 creator A5029753048 @default.
• W3137673973 creator A5079882825 @default.
• W3137673973 creator A5087837530 @default.
• W3137673973 date "2021-03-01" @default.
• W3137673973 modified "2023-10-17" @default.
• W3137673973 title "Unified framework for B-anomalies, muon g − 2 and neutrino masses" @default.
• W3137673973 cites W138462411 @default.
• W3137673973 cites W1506194303 @default.
• W3137673973 cites W1508359047 @default.
• W3137673973 cites W1515030353 @default.
• W3137673973 cites W1521093224 @default.
• W3137673973 cites W1604190277 @default.
• W3137673973 cites W1620183536 @default.
• W3137673973 cites W1814723547 @default.
• W3137673973 cites W1879058903 @default.
• W3137673973 cites W1927657254 @default.
• W3137673973 cites W1969561958 @default.
• W3137673973 cites W1991398012 @default.
• W3137673973 cites W2001911523 @default.
• W3137673973 cites W2002081836 @default.
• W3137673973 cites W2003516924 @default.
• W3137673973 cites W2007590223 @default.
• W3137673973 cites W2012433125 @default.
• W3137673973 cites W2015546321 @default.
• W3137673973 cites W2017744271 @default.
• W3137673973 cites W2017920658 @default.
• W3137673973 cites W2029318680 @default.
• W3137673973 cites W2045402092 @default.
• W3137673973 cites W2062231058 @default.
• W3137673973 cites W2078270404 @default.
• W3137673973 cites W2078281237 @default.
• W3137673973 cites W2080412008 @default.
• W3137673973 cites W2089507017 @default.
• W3137673973 cites W2091605720 @default.
• W3137673973 cites W2094095501 @default.
• W3137673973 cites W2097501548 @default.
• W3137673973 cites W2099535670 @default.
• W3137673973 cites W2101073879 @default.
• W3137673973 cites W2105272349 @default.
• W3137673973 cites W2108249481 @default.
• W3137673973 cites W2110656022 @default.
• W3137673973 cites W2110999179 @default.
• W3137673973 cites W2111341905 @default.
• W3137673973 cites W2115896628 @default.
• W3137673973 cites W2118488783 @default.
• W3137673973 cites W2129188437 @default.
• W3137673973 cites W2130516668 @default.
• W3137673973 cites W2135540890 @default.
• W3137673973 cites W2156526355 @default.
• W3137673973 cites W2158325186 @default.
• W3137673973 cites W2163097950 @default.
• W3137673973 cites W2166252135 @default.
• W3137673973 cites W2199503225 @default.
• W3137673973 cites W2302365184 @default.
• W3137673973 cites W2345317779 @default.
• W3137673973 cites W2398119593 @default.
• W3137673973 cites W2469504568 @default.
• W3137673973 cites W2483337043 @default.
• W3137673973 cites W2520637791 @default.
• W3137673973 cites W2530199168 @default.
• W3137673973 cites W2565617802 @default.
• W3137673973 cites W2608060328 @default.
• W3137673973 cites W2608170661 @default.
• W3137673973 cites W2611074547 @default.
• W3137673973 cites W2614185328 @default.
• W3137673973 cites W2620561867 @default.
• W3137673973 cites W2638422081 @default.
• W3137673973 cites W2731276465 @default.
• W3137673973 cites W2733778877 @default.
• W3137673973 cites W2748963470 @default.
• W3137673973 cites W2757774300 @default.
• W3137673973 cites W2761899819 @default.
• W3137673973 cites W2766841679 @default.
• W3137673973 cites W2780279694 @default.
• W3137673973 cites W2788959184 @default.
• W3137673973 cites W2795417494 @default.
• W3137673973 cites W2796235086 @default.
• W3137673973 cites W2808939453 @default.
• W3137673973 cites W2810153434 @default.
• W3137673973 cites W2881384875 @default.
• W3137673973 cites W2885545292 @default.
• W3137673973 cites W2887887926 @default.
• W3137673973 cites W2891027866 @default.
• W3137673973 cites W2901752741 @default.
• W3137673973 cites W2909142465 @default.
• W3137673973 cites W291582043 @default.
• W3137673973 cites W2941221887 @default.
• W3137673973 cites W2943850397 @default.
• W3137673973 cites W2944034367 @default.
• W3137673973 cites W2945603195 @default.
• W3137673973 cites W2950570720 @default.
• W3137673973 cites W2952915580 @default.
• W3137673973 cites W2995868688 @default.
• W3137673973 cites W3003792631 @default.
• W3137673973 cites W3006566086 @default.
• W3137673973 cites W3007210348 @default.
• W3137673973 cites W3009229510 @default.

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