Search results for "SAW"

showing 10 items of 204 documents

Supersymmetric mass spectra and the seesaw type-I scale

2012

We calculate supersymmetric mass spectra with cMSSM boundary conditions and a type-I seesaw mechanism added to explain current neutrino data. Using published, estimated errors on SUSY mass observables for a combined LHC+ILC analysis, we perform a theoretical $\chi^2$ analysis to identify parameter regions where pure cMSSM and cMSSM plus seesaw type-I might be distinguishable with LHC+ILC data. The most important observables are determined to be the (left) smuon and selectron masses and the splitting between them, respectively. Splitting in the (left) smuon and selectrons is tiny in most of cMSSM parameter space, but can be quite sizeable for large values of the seesaw scale, $m_{SS}$. Thus,…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaObservableSupersymmetryParameter spaceType (model theory)01 natural sciencesSelectron tubeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw mechanismSeesaw molecular geometry0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physics
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Supersymmetric type-III seesaw mechanism: Lepton flavor violating decays and dark matter

2011

We study a supersymmetric version of the seesaw mechanism type III. The model consists of the minimal supersymmetric extension of the standard model particle content plus three copies of $\mathbf{24}$ superfields. The fermionic part of the $SU(2)$ triplet contained in the $\mathbf{24}$ is responsible for the type-III seesaw, which is used to explain the observed neutrino masses and mixings. Complete copies of $\mathbf{24}$ are introduced to maintain gauge coupling unification. These additional states change the beta functions of the gauge couplings above the seesaw scale. Using minimal Supergravity boundary conditions, we calculate the resulting supersymmetric mass spectra at the electrowea…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaSupersymmetryType (model theory)01 natural sciencesStandard ModelSeesaw mechanismSeesaw molecular geometry0103 physical sciencesContent (measure theory)Grand Unified TheoryElectroweak scale010306 general physicsPhysical Review D
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CP Violation in the SUSY Seesaw: Leptogenesis and Low Energy

2008

We suppose that the baryon asymmetry is produced by thermal leptogenesis (with flavour effects), at temperatures $\sim 10^{9} - 10^{10}$ GeV, in the supersymmetric seesaw with universal and real soft terms. The parameter space is restricted by assuming that $l_\alpha \to l_\beta \gamma$ processes will be seen in upcoming experiments. We study the sensitivity of the baryon asymmetry to the phases of the lepton mixing matrix, and find that leptogenesis can work for any value of the phases. We also estimate the contribution to the electric dipole moment of the electron, arising from the seesaw, and find that it is (just) beyond the sensitivity of next generation experiments ($\lsim 10^{-29} e$…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyPontecorvo–Maki–Nakagawa–Sakata matrixFísicaFOS: Physical sciencesSupersymmetryParameter space01 natural sciencesHigh Energy Physics - PhenomenologyElectric dipole momentBaryon asymmetryHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryLeptogenesis[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]0103 physical sciencesCP violation010306 general physics
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Lepton Flavor Violation and non-unitarity Lepton Mixing in Low-Scale Type-I Seesaw

2011

Within low-scale seesaw mechanisms, such as the inverse and linear seesaw, one expects (i) potentially large lepton flavor violation (LFV) and (ii) sizeable non-standard neutrino interactions (NSI). We consider the interplay between the magnitude of non-unitarity effects in the lepton mixing matrix, and the constraints that follow from LFV searches in the laboratory. We find that NSI parameters can be sizeable, up to percent level in some cases, while LFV rates, such as that for \mu -> e \gamma, lie within current limits, including the recent one set by the MEG collaboration. As a result the upcoming long baseline neutrino experiments offer a window of opportunity for complementary LFV and …

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyPontecorvo–Maki–Nakagawa–Sakata matrixInverseFOS: Physical sciencesFísica01 natural sciencesUnitary stateHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsScale typeFlavorLepton
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Systematic study of the d=5 Weinberg operator at one-loop order

2012

We perform a systematic study of the $d=5$ Weinberg operator at the one-loop level. We identify three different categories of neutrino mass generation: (1) finite irreducible diagrams; (2) finite extensions of the usual seesaw mechanisms at one-loop and (3) divergent loop realizations of the seesaws. All radiative one-loop neutrino mass models must fall into one of these classes. Case (1) gives the leading contribution to neutrino mass naturally and a classic example of this class is the Zee model. We demonstrate that in order to prevent that a tree level contribution dominates in case (2), Majorana fermions running in the loop and an additional $\mathbb{Z}_2$ symmetry are needed for a genu…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsOperator (physics)Mass generationHigh Energy Physics::PhenomenologyFísicaFOS: Physical sciencesCoupling (probability)01 natural sciencesLepton numberLoop (topology)MAJORANATheoretical physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesNeutrino010306 general physics
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A(4)-based neutrino masses with Majoron decaying dark matter

2010

We propose an A(4) flavor-symmetric SU(3) circle times SU(2) circle times U(1) seesaw model where lepton number is broken spontaneously. A consistent two-zero texture pattern of neutrino masses and mixing emerges from the interplay of type-I and type-II seesaw contributions, with important phenomenological predictions. We show that, if the Majoron becomes massive, such seesaw scenario provides a viable candidate for decaying dark matter, consistent with cosmic microwave background lifetime constraints that follow from current WMAP observations. We also calculate the subleading one-loop-induced decay into photons which leads to a monoenergetic emission line that may be observed in future x-r…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsPhysics beyond the Standard ModelCosmic microwave backgroundDark matterHigh Energy Physics::PhenomenologyCosmic background radiationFísicaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energyLepton numberHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesNeutrino010306 general physicsMajoronParticle Physics - Phenomenology
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The simplest scoto-seesaw model: WIMP dark matter phenomenology and Higgs vacuum stability

2021

We analyze the consistency of electroweak breaking, neutrino and dark matter phenomenology within the simplest scoto-seesaw model. By adding the minimal dark sector to the simplest "missing partner" type-I seesaw one has a physical picture for the neutrino oscillation lengths: the "atmospheric" mass scale arises from the tree-level seesaw, while the "solar" scale is induced radiatively, mediated by the dark sector. We identify parameter regions consistent with theoretical constraints, as well as dark matter relic abundance and direct detection searches. Using two-loop renormalization group equations we explore the stability of the vacuum and the consistency of the underlying dark parity sym…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsPhysicsQC1-999Dark matterElectroweak interactionHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryDouble beta decay0103 physical sciencesHiggs bosonNeutrino010306 general physicsNeutrino oscillationPhenomenology (particle physics)Physics Letters B
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The minimal adjoint-SU (5) x Z(4) GUT model

2013

An extension of the adjoint SU (5) model with a flavour symmetry based on the Z(4) group is investigated. The Z(4) symmetry is introduced with the aim of leading the up-and down-quark mass matrices to the Nearest-Neighbour-Interaction form. As a consequence of the discrete symmetry embedded in the SU (5) gauge group, the charged lepton mass matrix also gets the same form. Within this model, light neutrinos get their masses through type-I, type-III and one-loop radiative seesaw mechanisms, implemented, respectively, via a singlet, a triplet and an octet from the adjoint fermionic 24 fields. It is demonstrated that the neutrino phenomenology forces the introduction of at least three 24 fermio…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsProton decayHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísica01 natural sciencesSymmetry (physics)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryGauge group0103 physical sciencesHiggs bosonDiscrete and Finite SymmetriesHigh Energy Physics::ExperimentNeutrino PhysicsGUTNeutrino010306 general physicsLeptonDiscrete symmetry
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Dark Matter and the elusive $\mathbf{Z'}$ in a dynamical Inverse Seesaw scenario

2017

The Inverse Seesaw naturally explains the smallness of neutrino masses via an approximate $B-L$ symmetry broken only by a correspondingly small parameter. In this work the possible dynamical generation of the Inverse Seesaw neutrino mass mechanism from the spontaneous breaking of a gauged $U(1)$ $B-L$ symmetry is investigated. Interestingly, the Inverse Seesaw pattern requires a chiral content such that anomaly cancellation predicts the existence of extra fermions belonging to a dark sector with large, non-trivial, charges under the $U(1)$ $B-L$. We investigate the phenomenology associated to these new states and find that one of them is a viable dark matter candidate with mass around the T…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsSpontaneous symmetry breakingDark matterHigh Energy Physics::PhenomenologyInverseFOS: Physical sciencesFermion16. Peace & justice01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry0103 physical sciencesBeyond Standard Modellcsh:QC770-798Neutrino Physicslcsh:Nuclear and particle physics. Atomic energy. RadioactivityNeutrino010306 general physicsPhenomenology (particle physics)Boson
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Dark matter in minimal supergravity with type-II seesaw mechanism

2009

We calculate the relic density of the lightest neutralino in a supersymmetric seesaw type-II (``triplet seesaw'') model with minimal supergravity boundary conditions at the grand unified theory (GUT) scale. The presence of a triplet below the GUT scale, required to explain measured neutrino data in this setup, leads to a characteristic deformation of the sparticle spectrum with respect to the pure minimal supergravity (mSUGRA) expectations, affecting the calculated relic dark matter (DM) density. We discuss how the DM allowed regions in the $({m}_{0},{M}_{1/2})$ plane change as a function of the (type-II) seesaw scale. We also compare the constraints imposed on the models parameter space fo…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsSupergravityDark matterHigh Energy Physics::PhenomenologyFísicaSupersymmetry01 natural sciencesSeesaw mechanismSeesaw molecular geometry0103 physical sciencesNeutralinoGrand Unified TheoryHigh Energy Physics::ExperimentNeutrino010306 general physics
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