2022
DOI: 10.1007/jhep06(2022)084
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Dark Matter abundance via thermal decays and leptoquark mediators

Abstract: We explore a new mechanism for reproducing the Dark Matter (DM) abundance: scatterings of one DM particle on light Standard Model particles. Strong bounds on its decays can be satisfied if DM undergoes freeze-in and has a mass around or below the pion mass. This happens, for example, in theories with a right-handed neutrino interacting with charged fermions through a leptoquark exchange. These leptoquarks can be linked to the ones motivated by the B-physics anomalies if assumptions about the flavour structure … Show more

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Cited by 6 publications
(2 citation statements)
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“…A left-handed fermion mediator singlet can also couple to right-handed quarks. For instance, the down-quark singlet d R couples to ψ L with a leptoquark scalar ϕ [85][86][87][88][89]: y ψ,i di,R ψ L ϕ + h.c. , (6.10) where the scalar ϕ is now an SU(3) c triplet and SU(2) L singlet, carrying the hypercharge Y = −1/3 so that ψ is a SM singlet. The thermal mass in this case is given by m 2 ψ (T ) = where the factor of 3 accounts for the color degrees of freedom.…”
Section: Left-handed Fermion Mediatormentioning
confidence: 99%
“…A left-handed fermion mediator singlet can also couple to right-handed quarks. For instance, the down-quark singlet d R couples to ψ L with a leptoquark scalar ϕ [85][86][87][88][89]: y ψ,i di,R ψ L ϕ + h.c. , (6.10) where the scalar ϕ is now an SU(3) c triplet and SU(2) L singlet, carrying the hypercharge Y = −1/3 so that ψ is a SM singlet. The thermal mass in this case is given by m 2 ψ (T ) = where the factor of 3 accounts for the color degrees of freedom.…”
Section: Left-handed Fermion Mediatormentioning
confidence: 99%
“…For the freeze-in mechanism, in which the coupling with the SM plasma is feeble and therefore the dark matter is never in thermal equilibrium, the dark matter density, starting from zero or very small values, slowly grows up to the point it gets frozen-in at its cosmological abundance. Models of this type have a dark matter candidate in the BSM sector featuring also a vector LQ addressing the anomalies [197]. Here the dark matter state is a light (order JHEP08(2022)125 10 KeVs) right-handed neutrino, produced via freeze-in through its interactions with the massive (order TeVs) LQ.…”
Section: Dark Side Of the Anomaliesmentioning
confidence: 99%