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dc.contributor.authorHernández Tomé, G.
dc.contributor.authorIllana Calero, José Ignacio 
dc.contributor.authorMasip Mellado, Manuel 
dc.date.accessioned2021-03-15T11:30:52Z
dc.date.available2021-03-15T11:30:52Z
dc.date.issued2020
dc.identifier.citationHernández-Tomé, G., Illana, J. I., & Masip, M. (2020). ρ parameter and H 0→ ℓ i ℓ j in models with TeV sterile neutrinos. Physical Review D, 102(11), 113006. [DOI: 10.1103/PhysRevD.102.113006]es_ES
dc.identifier.urihttp://hdl.handle.net/10481/67226
dc.description.abstractThe presence of massive sterile neutrinos N mixed with the active ones induces flavor violating processes in the charged lepton sector at the loop level. In particular, the amplitude of H 0 → ¯ ℓ i ℓ j is expected to be proportional to the product of heavy-light Yukawa couplings y i y j = 2 s ν i s ν j m 2 N / v 2 , where s ν i , j express the heavy-light neutrino mixings. Here, we revisit these Higgs decays in the most generic extension of the neutrino sector, focusing on large values of y i . We show that decoupling effects and a cancellation between the two dominant contributions to these processes makes the amplitude about 100 times smaller than anticipated. We find that perturbative values of y i giving an acceptable contribution to the ρ parameter imply B ( H 0 → ¯ ℓ i ℓ j ) < 10 − 8 for any lepton flavors, a rate that is not accessible at current colliders.es_ES
dc.description.sponsorshipSpanish Ministry of Science, Innovation and Universities FPA2016-78220-C3 PID2019-107844GB-C21/AEI/10.13039/501100011033es_ES
dc.description.sponsorshipJunta de Andalucia FQM 101 SOMM17/6104/UGR P18-FR-1962 P18-FR-5057es_ES
dc.description.sponsorshipConsejo Nacional de Ciencia y Tecnologia (CONACyT)es_ES
dc.language.isoenges_ES
dc.publisherAMER PHYSICAL SOCes_ES
dc.rightsAtribución 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/es/*
dc.titleρ parameter and H 0 → ℓ i ℓ j in models with TeV sterile neutrinoses_ES
dc.typejournal articlees_ES
dc.rights.accessRightsopen accesses_ES
dc.identifier.doi10.1103/PhysRevD.102.113006


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