2022
DOI: 10.1103/physrevd.105.015033
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Light dark matter, rare B decays with missing energy in LμLτ model with a scalar leptoquark

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Cited by 14 publications
(8 citation statements)
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“…In complete visible sector models, all scattering cross sections with the SM particles can be computed exactly, and cosmological and experimental limits applied to them. Some examples of this type are NMSSM models of [29] and [30], the Phenomenological Minimal Supersymmetric Models (pMSSM) of [35] and [36], the multiple scalar doublet models of [31] and [37], the U (1) Lµ−Lτ gauge SM extension model of [40], the stable neutral heavy Dirac fermion dark matter (RHN model) in [41], and the pseudo-Goldstone Boson dark matter model of [32], in which the dark matter consists WIMPs of mass in the GeV to 1.5 TeV range with Spin Independent (SI) or Spin Dependent (SD) scattering cross sections off of nuclei. In some visible sector models detailed predictions of the cross section of scattering of the dark matter off nuclei were made while remaining agnostic about how Figure 5: Plots of dark matter-proton cross section σ SI times dark matter fraction f DM versus particle mass M DM for SI scattering cross sections off nuclei.…”
Section: Snowmass2021 Cosmic Frontier Dark Matter Direct Detection To...mentioning
confidence: 99%
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“…In complete visible sector models, all scattering cross sections with the SM particles can be computed exactly, and cosmological and experimental limits applied to them. Some examples of this type are NMSSM models of [29] and [30], the Phenomenological Minimal Supersymmetric Models (pMSSM) of [35] and [36], the multiple scalar doublet models of [31] and [37], the U (1) Lµ−Lτ gauge SM extension model of [40], the stable neutral heavy Dirac fermion dark matter (RHN model) in [41], and the pseudo-Goldstone Boson dark matter model of [32], in which the dark matter consists WIMPs of mass in the GeV to 1.5 TeV range with Spin Independent (SI) or Spin Dependent (SD) scattering cross sections off of nuclei. In some visible sector models detailed predictions of the cross section of scattering of the dark matter off nuclei were made while remaining agnostic about how Figure 5: Plots of dark matter-proton cross section σ SI times dark matter fraction f DM versus particle mass M DM for SI scattering cross sections off nuclei.…”
Section: Snowmass2021 Cosmic Frontier Dark Matter Direct Detection To...mentioning
confidence: 99%
“…7 we reproduce some of the predictions for SD scattering cross sections (in plots of dark matter-proton cross section versus dark matter mass) for the visible sector models Snowmass2021 Cosmic Frontier Dark Matter Direct Detection to the Neutrino Fog of Refs. [29,30,35,40,41].…”
Section: Snowmass2021 Cosmic Frontier Dark Matter Direct Detection To...mentioning
confidence: 99%
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“…Interestingly, scalar leptoquark solutions to the above anomalies still persist after the recent LHCb update, as shown for instance in refs. [27][28][29][30][31][32].…”
Section: Lq Lqmentioning
confidence: 99%
“…Interestingly, scalar leptoquark solutions to the above anomalies still persist after the recent LHCb update, as shown for instance in refs. [27][28][29][30][31][32][33].…”
Section: Introductionmentioning
confidence: 99%