Search results for "SAW"

showing 10 items of 204 documents

Soft masses in supersymmetric SO(10) GUTs with low intermediate scales

2011

The specific shape of the squark, slepton and gaugino mass spectra, if measured with sufficient accuracy, can provide invaluable information not only about the dynamics underpinning their origin at some very high scale such as the unification scale ${M}_{G}$, but also about the intermediate scale physics encountered throughout their renormalization group equations evolution down to the energy scale accessible for the LHC. In this work, we study general features of the TeV scale soft supersymmetry breaking parameters stemming from a generic mSugra configuration within certain classes of supersymmetry $SO(10)$ GUTs with different intermediate symmetries below ${M}_{G}$. We show that particula…

PhysicsNuclear and High Energy PhysicsParticle physicsScale (ratio)010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGauginoFísicaSupersymmetryRenormalization group01 natural sciencesSupersymmetry breakingSeesaw molecular geometry0103 physical sciencesHomogeneous spaceHigh Energy Physics::ExperimentSO(10)010306 general physicsPhysical Review D
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3-Neutrino Mass Spectrum from Combining Seesaw and Radiative Neutrino Mass Mechanisms

1999

We extend the Standard Model by adding a second Higgs doublet and a right-handed neutrino singlet with a heavy Majorana mass term. In this model, there are one heavy and three light Majorana neutrinos with a mass hierarchy m_3 >> m_2 >> m_1 such that that only m_3 is non-zero at the tree level and light because of the seesaw mechanism, m_2 is generated at the one-loop and m_1 at the two-loop level. We show that the atmospheric neutrino oscillations and large mixing MSW solar neutrino transitions with $��m^2_\mathrm{atm} \simeq m_3^2$ and $��m^2_\mathrm{solar} \simeq m_2^2$, respectively, are naturally accommodated in this model without employing any symmetry.

PhysicsNuclear and High Energy PhysicsParticle physicsSolar neutrinoHigh Energy Physics::PhenomenologyFOS: Physical sciencesStandard ModelMAJORANAHigh Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryMass spectrumHiggs bosonNeutrino
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Enhanced lepton flavor violation in the supersymmetric inverse seesaw model

2004

We discuss a supersymmetric inverse seesaw model in which lepton flavour violating decays can be enhanced either by flavour violating slepton contributions or by the non-unitarity of the charged current mixing matrix. As an example we calculate Br(mu -> e gamma) taking into account both heavy lepton exchange as well as supersymmetric diagrams in a minimal supergravity framework. We find that the for the same parameters the rate can be enhanced with respect to seesaw model expectations, with or without supersymmetry.

PhysicsNuclear and High Energy PhysicsParticle physicsSolar neutrinoSupergravityHigh Energy Physics::PhenomenologyFlavourFOS: Physical sciencesFísicaSupersymmetryRenormalization groupHigh Energy Physics - PhenomenologyHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryHigh Energy Physics::ExperimentCharged currentLeptonPhysical Review D
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Leptogenesis with Single Right-Handed Neutrino Dominance

2001

We make an analytic and numerical study of leptogenesis in the framework of the (Supersymmetric) Standard Model plus the see-saw mechanism with a U(1) family symmetry and single right-handed neutrino dominance. In presenting our analytic and numerical results we make a clear distinction between the theoretically clean asymmetry parameter $\epsilon_1$ and the baryon asymmetry $Y_B$. In calculating $Y_B$ we propose and use a fit to the solutions to the Boltzmann equations which gives substantially more reliable results than parametrisations previously used in the literature. Our results show that there is a decoupling between the low energy neutrino observables and the leptogenesis prediction…

PhysicsNuclear and High Energy PhysicsParticle physicsSolar neutrinomedia_common.quotation_subjectHigh Energy Physics::PhenomenologyFísicaFOS: Physical sciencesDecoupling (cosmology)AsymmetryHigh Energy Physics - PhenomenologyBaryon asymmetrySeesaw mechanismHigh Energy Physics - Phenomenology (hep-ph)LeptogenesisNeutrinoNeutrino oscillationmedia_common
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Flavour-symmetric type-II Dirac neutrino seesaw mechanism

2018

We propose a Standard Model extension with underlying A4 flavour symmetry where small Dirac neutrino masses arise from a Type-II seesaw mechanism. The model predicts the "golden" flavour-dependent bottom-tau mass relation, requires an inverted neutrino mass ordering and non-maximal atmospheric mixing angle. Using the latest neutrino oscillation global fit we derive restrictions on the oscillation parameters, such as a correlation between Dirac CP phase and the lightest neutrino mass.

PhysicsNuclear and High Energy PhysicsParticle physicsSterile neutrino010308 nuclear & particles physicsOscillationDirac (video compression format)High Energy Physics::LatticeHigh Energy Physics::PhenomenologyFOS: Physical sciences01 natural sciencesSymmetry (physics)lcsh:QC1-999High Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Phenomenology (hep-ph)Standard-Model Extension0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationlcsh:PhysicsPhysics Letters B
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New neutrino mass sum rule from the inverse seesaw mechanism

2012

A class of discrete flavor-symmetry-based models predicts constrained neutrino mass matrix schemes that lead to specific neutrino mass sum rules. One of these implies a lower bound on the effective neutrinoless double beta mass parameter, even for normal hierarchy neutrinos. Here we propose a new model based on the ${S}_{4}$ flavor symmetry that leads to the new neutrino mass sum rule and discuss how to generate a nonzero value for the reactor angle ${\ensuremath{\theta}}_{13}$ indicated by recent experiments, and the resulting correlation with the solar angle ${\ensuremath{\theta}}_{12}$.

PhysicsNuclear and High Energy PhysicsParticle physicsSterile neutrino010308 nuclear & particles physicsSolar neutrinoHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemMass matrix01 natural sciencesSeesaw mechanism0103 physical sciencesHigh Energy Physics::ExperimentSum rule in quantum mechanicsNeutrino010306 general physicsNeutrino oscillation
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Neff versus the lightest neutrino mass

2016

AbstractWithin the framework of low-scale Type I seesaw models with two and three extra sterile neutrinos we evaluate the production of the sterile states in the Early Universe. We explore the full parameter space and find that in the model with two extra states both of them reach thermal equilibrium with the primordial plasma. In the model with three sterile neutrinos, if the lightest active neutrino mass is below O(10−3eV) one sterile neutrino might not thermalize, while the other two always reach thermalization. Applying constrains from both extra radiation at BBN and CMB, and the dark matter allowed abundance, we show that the spectra of heavier states are severely restricted in the mas…

PhysicsNuclear and High Energy PhysicsParticle physicsSterile neutrino010308 nuclear & particles physicsSolar neutrinoHigh Energy Physics::PhenomenologyNeutrino decouplingSolar neutrino problem01 natural sciencesseesaw modelCosmic neutrino backgroundNuclear physicssterile neutrinos0103 physical sciencesMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationNuclear and Particle Physics Proceedings
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N_eff in low-scale seesaw models versus the lightest neutrino mass

2014

We evaluate the contribution to $N_{\rm eff}$ of the extra sterile states in low-scale Type I seesaw models (with three extra sterile states). We explore the full parameter space and find that at least two of the heavy states always reach thermalisation in the Early Universe, while the third one might not thermalise provided the lightest neutrino mass is below ${\mathcal O}(10^{-3}$eV). Constraints from cosmology therefore severely restrict the spectra of heavy states in the range 1eV- 100 MeV. The implications for neutrinoless double beta decay are also discussed.

PhysicsNuclear and High Energy PhysicsParticle physicsSterile neutrinoCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics beyond the Standard Modelmedia_common.quotation_subjectFOS: Physical sciencesFísicaUniverseNuclear physicsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryDouble beta decayMeasurements of neutrino speedNeutrinoNeutrino oscillationmedia_commonAstrophysics - Cosmology and Nongalactic Astrophysics
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Inflation and majoron dark matter in the neutrino seesaw mechanism

2014

We propose that inflation and dark matter have a common origin, connected to the neutrino mass generation scheme. As a model we consider spontaneous breaking of global lepton number within the seesaw mechanism. We show that it provides an acceptable inflationary scenario consistent with the recent cosmic microwave background B-mode observation by the BICEP2 experiment. The scheme may also account for the baryon asymmetry of the Universe through leptogenesis for reasonable parameter choices.

PhysicsNuclear and High Energy PhysicsParticle physicsSterile neutrinoDark matterHigh Energy Physics::PhenomenologyFísicaAstrophysics::Cosmology and Extragalactic AstrophysicsLepton numberSeesaw mechanismBaryon asymmetryLeptogenesisddc:530NeutrinoMajoron
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Fair scans of the seesaw. Consequences for predictions on LFV processes

2011

22 páginas, 5 figuras.-- El Pdf es la versión pre-print: arXiv:1010.5751v1

PhysicsNuclear and High Energy PhysicsParticle physicsSupersymmetric Standard Model010308 nuclear & particles physicsBranching fractionYukawa potentialFOS: Physical sciencesFísicaValue (computer science)Space (mathematics)01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Cover (topology)Seesaw molecular geometryLeptogenesis0103 physical sciencesNeutrino Physics010306 general physicsSimple (philosophy)Journal of High Energy Physics
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