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Anomalies in 𝑏 → 𝑠 Transitions and Dark Matter

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Anomalies in 𝑏 → 𝑠 Transitions and Dark Matter

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dc.contributor.author Vicente Montesinos, Avelino
dc.date.accessioned 2019-02-21T14:52:50Z
dc.date.available 2019-02-21T14:52:50Z
dc.date.issued 2018
dc.identifier.citation Vicente Montesinos, Avelino 2018 Anomalies in 𝑏 → 𝑠 Transitions and Dark Matter Advances In High Energy Physics 2018 3905848
dc.identifier.uri http://hdl.handle.net/10550/69153
dc.description.abstract Since 2013, the LHCb collaboration has reported on the measurement of several observables associated with b -> s transitions, finding various deviations from their predicted values in the Standard Model. These include a set of deviations in branching ratios and angular observables, as well as in the observables Rk and Rk*, specially built to test the possible violation of Lepton Flavor Universality. Even though these tantalizing hints are not conclusive yet, the b -> s anomalies have gained considerable attention in the flavor community. Here we review new physics models that address these anomalies and explore their possible connection to the dark matter of the Universe. After discussing some of the ideas introduced in these works and classifying the proposed models, two selected examples are presented in detail in order to illustrate the potential interplay between these two areas of current particle physics.
dc.language.iso eng
dc.relation.ispartof Advances In High Energy Physics, 2018, vol. 2018, num. 3905848
dc.subject Partícules (Física nuclear)
dc.title Anomalies in 𝑏 → 𝑠 Transitions and Dark Matter
dc.type journal article es_ES
dc.date.updated 2019-02-21T14:52:50Z
dc.identifier.doi 10.1155/2018/3905848
dc.identifier.idgrec 130156
dc.rights.accessRights open access es_ES

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