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dc.contributor.authorCarmona Bermúdez, Adrián 
dc.contributor.authorScherb, Christiane
dc.contributor.authorSchwaller, Pedro
dc.date.accessioned2021-10-05T11:24:55Z
dc.date.available2021-10-05T11:24:55Z
dc.date.issued2021-08-23
dc.identifier.citationCarmona, A., Scherb, C. & Schwaller, P. Charming ALPs. J. High Energ. Phys. 2021, 121 (2021). [https://doi.org/10.1007/JHEP08(2021)121]es_ES
dc.identifier.urihttp://hdl.handle.net/10481/70653
dc.descriptionWe thank Felix Kahlhofer and Fatih Ertas for useful feedback. AC thanks Mikael Chala, Jorge Martin-Camalich, Matthias Neubert and Robert Ziegler for fruitful discussions. AC acknowledges funding from the European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement No 754446 and UGR Research and Knowledge Transfer Found - Athenea3i. Work in Mainz was supported by the Cluster of Excellence Precision Physics, Fundamental Interactions, and Structure of Matter (PRISMA+ EXC 2118/1) funded by the German Research Foundation (DFG) within the German Excellence Strategy (Project ID 39083149), and by grant 05H18UMCA1 of the German Federal Ministry for Education and Research (BMBF).es_ES
dc.description.abstractAxion-like particles (ALPs) are ubiquitous in models of new physics explaining some of the most pressing puzzles of the Standard Model. However, until relatively recently, little attention has been paid to its interplay with flavour. In this work, we study in detail the phenomenology of ALPs that exclusively interact with up-type quarks at the tree-level, which arise in some well-motivated ultra-violet completions such as QCD-like dark sectors or Froggatt-Nielsen type models of flavour. Our study is performed in the low-energy effective theory to highlight the key features of these scenarios in a model independent way. We derive all the existing constraints on these models and demonstrate how upcoming experiments at fixed-target facilities and the LHC can probe regions of the parameter space which are currently not excluded by cosmological and astrophysical bounds. We also emphasize how a future measurement of the currently unavailable meson decay D -> pi + invisible could complement these upcoming searches.es_ES
dc.description.sponsorshipEuropean Commission 754446es_ES
dc.description.sponsorshipUGR Research and Knowledge Transfer Found - Athenea3ies_ES
dc.description.sponsorshipGerman Research Foundation (DFG) EXC 2118/1 39083149es_ES
dc.description.sponsorshipFederal Ministry of Education & Research (BMBF) 05H18UMCA1es_ES
dc.language.isoenges_ES
dc.publisherSpringeres_ES
dc.rightsAtribución 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.subjectPhenomenological Modelses_ES
dc.titleCharming ALPses_ES
dc.typejournal articlees_ES
dc.relation.projectIDinfo:eu-repo/grantAgreement/EC/H2020/754446es_ES
dc.rights.accessRightsopen accesses_ES
dc.identifier.doi10.1007/JHEP08(2021)121
dc.type.hasVersionVoRes_ES


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