0000000000069783

AUTHOR

Salvador Centelles-chuliá

0000-0001-6579-1067

showing 6 related works from this author

Dark matter stability and Dirac neutrinos using only Standard Model symmetries

2020

We provide a generic framework to obtain stable dark matter along with naturally small Dirac neutrino masses generated at the loop level. This is achieved through the spontaneous breaking of the global $U(1)_{B-L}$ symmetry already present in Standard Model. The $U(1)_{B-L}$ symmetry is broken down to a residual even $\mathcal{Z}_n$; $n \geq 4$ subgroup. The residual $\mathcal{Z}_n$ symmetry simultaneously guarantees dark matter stability and protects the Dirac nature of neutrinos. The $U(1)_{B-L}$ symmetry in our setup is anomaly free and can also be gauged in a straightforward way. Finally, we present an explicit example using our framework to show the idea in action.

Physics010308 nuclear & particles physicsDark matterDirac (software)FOS: Physical sciencesComputer Science::Digital Libraries01 natural sciencesAction (physics)Symmetry (physics)ddc:Standard Model (mathematical formulation)Theoretical physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesHomogeneous spaceAnomaly (physics)Neutrino010306 general physics
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Asymmetric tri-bi-maximal mixing and residual symmetries

2019

Asymmetric tri-bi-maximal mixing is a recently proposed, grand unified theory (GUT) based, flavor mixing scheme. In it, the charged lepton mixing is fixed by the GUT connection to down-type quarks and a $\mathcal{T}_{13}$ flavor symmetry, while neutrino mixing is assumed to be tri-bi-maximal (TBM) with one additional free phase. Here we show that this additional free phase can be fixed by the residual flavor and CP symmetries of the effective neutrino mass matrix. We discuss how those residual symmetries can be unified with $\mathcal{T}_{13}$ and identify the smallest possible unified flavor symmetries, namely $(\mathbb{Z}_{13}\times\mathbb{Z}_{13})\rtimes \mathrm{D}_{12}$ and $(\mathbb{Z}_…

PhysicsQuarkNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyFOS: Physical sciencesAstronomy and AstrophysicsHigh Energy Physics - ExperimentConnection (mathematics)High Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Double beta decayHomogeneous spaceCP violationGrand Unified TheoryHigh Energy Physics::ExperimentMixing (physics)Lepton
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CP symmetries as guiding posts: Revamping tribimaximal mixing. II.

2019

In this follow up of arXiv:1812.04663 we analyze the generalized CP symmetries of the charged lepton mass matrix compatible with the complex version of the Tri-Bi-Maximal (TBM) lepton mixing pattern. These symmetries are used to `revamp' the simplest TBM \textit{Ansatz} in a systematic way. Our generalized patterns share some of the attractive features of the original TBM matrix and are consistent with current oscillation experiments. We also discuss their phenomenological implications both for upcoming neutrino oscillation and neutrinoless double beta decay experiments.

Physics010308 nuclear & particles physicsPhysics beyond the Standard ModelHigh Energy Physics::PhenomenologyFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyTheoretical physicsMatrix (mathematics)High Energy Physics - Phenomenology (hep-ph)Mixing patterns0103 physical sciencesHomogeneous spaceCP violationHigh Energy Physics::Experiment010306 general physicsNeutrino oscillationMixing (physics)AnsatzPhysical Review D
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Seesaw Dirac neutrino mass through dimension-six operators

2018

In this paper, a follow-up of [S. C. Chuliá, R. Srivastava, and J. W. F. Valle, Phys. Lett. B 781, 122 (2018)], we describe the many pathways to generate Dirac neutrino mass through dimension-six operators. By using only the standard model Higgs doublet in the external legs, one gets a unique operator 1Λ2L¯Φ¯Φ¯ΦνR. In contrast, the presence of new scalars implies new possible field contractions, which greatly increase the number of possibilities. Here, we study in detail the simplest ones, involving SU(2)L singlets, doublets, and triplets. The extra symmetries needed to ensure the Dirac nature of neutrinos can also be responsible for stabilizing dark matter.

PhysicsParticle physics010308 nuclear & particles physicsDirac (video compression format)High Energy Physics::PhenomenologyDimension (graph theory)Field (mathematics)Lambda01 natural sciencesStandard Model0103 physical sciencesHomogeneous spaceHiggs bosonNeutrino010306 general physicsPhysical Review D
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Seesaw roadmap to neutrino mass and dark matter

2018

We describe the many pathways to generate Majorana and Dirac neutrino mass through generalized dimension-5 operators a la Weinberg. The presence of new scalars beyond the Standard Model Higgs doublet implies new possible field contractions, which are required in the case of Dirac neutrinos. We also notice that, in the Dirac neutrino case, the extra symmetries needed to ensure the Dirac nature of neutrinos can also be made responsible for stability of dark matter.

PhysicsNuclear and High Energy PhysicsParticle physicsField (physics)010308 nuclear & particles physicsPhysics beyond the Standard ModelHigh Energy Physics::LatticeDirac (software)Dark matterHigh Energy Physics::PhenomenologyFOS: Physical sciences01 natural scienceslcsh:QC1-999MAJORANAHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesHiggs bosonHigh Energy Physics::ExperimentNeutrino010306 general physicslcsh:PhysicsPhysics Letters B
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Generalized bottom-tau unification, neutrino oscillations and dark matter: Predictions from a lepton quarticity flavor approach

2017

We propose an $A_4$ extension of the Standard Model with a Lepton Quarticity symmetry correlating dark matter stability with the Dirac nature of neutrinos. The flavor symmetry predicts (i) a generalized bottom-tau mass relation involving all families, (ii) small neutrino masses are induced a la seesaw, (iii) CP must be significantly violated in neutrino oscillations, (iv) the atmospheric angle $\theta_{23}$ lies in the second octant, and (v) only the normal neutrino mass ordering is realized.

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsDirac (video compression format)Dark matterHigh Energy Physics::PhenomenologyFOS: Physical sciences01 natural sciencesSymmetry (physics)lcsh:QC1-999Standard ModelHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationlcsh:PhysicsLeptonPhysics Letters B
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