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dc.date.accessioned 2020-06-12T12:31:05Z
dc.date.available 2020-06-12T12:31:05Z
dc.date.issued 2017-06
dc.identifier.uri http://sedici.unlp.edu.ar/handle/10915/98134
dc.description.abstract We present an effective description of a spin two massive state and a pseudo-Nambu-Goldstone boson Higgs in a two site model. Using this framework, we model the spin-two state as a massive graviton and we study its phenomenology at the LHC. We find that a reduced set of parameters can describe the most important features of this scenario. We address the question of which channel is the most sensitive to detect this graviton. Instead of designing search strategies to estimate the significance in each channel, we compare the ratio of our theoretical predictions to the limits set by available experimental searches for all the decay channels and as a function of the free parameters in the model. We discuss the phenomenological details contained in the outcome of this simple procedure. The results indicate that, for the studied masses between 0.5 and 3 TeV, the channels to look for such a graviton resonance are mainly ZZ, WW, and γγ. This is the case even though top and bottom quarks dominate the branching ratios, since their experimental sensitivity is not as good as the one of the electroweak gauge bosons. We find that as the graviton mass increases, the ZZ and WW channels become more important because of its relatively better enhancement over background, mainly due to fat jet techniques. We determine the region of the parameter space that has already been excluded and the reach for the LHC next stages. We also estimate the size of the loop-induced contributions to the production and decay of the graviton, and show in which region of the parameter space their effects are relevant for our analysis. en
dc.language en es
dc.subject LHC es
dc.subject Graviton resonance es
dc.subject Composite models es
dc.title Graviton resonance phenomenology and a pseudo-Nambu-Goldstone boson Higgs at the LHC en
dc.type Articulo es
sedici.identifier.uri https://ri.conicet.gov.ar/11336/63220 es
sedici.identifier.uri http://link.aps.org/doi/10.1103/PhysRevD.95.115012 es
sedici.identifier.uri https://arxiv.org/abs/1610.08451 es
sedici.identifier.other http://dx.doi.org/10.1103/PhysRevD.95.115012 es
sedici.identifier.other arXiv:1610.08451 es
sedici.identifier.other hdl:11336/63220 es
sedici.identifier.issn 2470-0029 es
sedici.creator.person Alvarez, Ezequiel es
sedici.creator.person Da Rold, Leandro es
sedici.creator.person Mazzitelli, Javier Sebastián es
sedici.creator.person Szynkman, Alejandro Andrés es
sedici.subject.materias Física es
sedici.description.fulltext true es
mods.originInfo.place Instituto de Física La Plata es
sedici.subtype Preprint es
sedici.rights.license Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)
sedici.rights.uri http://creativecommons.org/licenses/by-nc-sa/4.0/
sedici.description.peerReview peer-review es
sedici.relation.journalTitle Physical Review D es
sedici.relation.journalVolumeAndIssue vol. 95, no. 11 es


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Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) Except where otherwise noted, this item's license is described as Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)