Search results for "Majorana"

showing 10 items of 174 documents

Unstable massive tau-neutrinos and primordial nucleosynthesis

1998

The impact of unstable Majorana tau neutrinos on primordial nucleosynthesis is considered. The mass and lifetime of nu_tau are taken in the intervals 0.1-20 MeV and 0.001-400 sec respectively. The studied decay modes are nu_tau -> nu_mu + phi and nu_tau -> nu_e + phi, where phi is a massless (or light) scalar. Integro-differential kinetic equations are solved numerically without any simplifying assumptions. Our results deviate rather strongly from earlier calculations. Depending on mass, lifetime, and decay channels of the nu_tau, the number of effective neutrino species (found from He4), in addition to the 3 standard ones, varies from -2 to +2.5. The abundances of H2 and Li7 are also…

PhysicsNuclear and High Energy PhysicsParticle physicsScalar (mathematics)FOS: Physical sciencesFísicaMassless particleHigh Energy Physics - PhenomenologyMAJORANAHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesisKinetic equationsHigh Energy Physics::ExperimentNeutrinoNuclear Physics B
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A potential test of the CP properties and Majorana nature of neutrinos

1999

The scattering of solar neutrinos on electrons may reveal their CP properties, which are particularly sensitive to their Majorana nature. The cross section is sensitive to the neutrino dipole moments through an interference of electro-magnetic and weak amplitudes. We show how future solar neutrino experiments with good angular resolution and low energy threshold, such as Hellaz, can be sensitive to the resulting azimuthal asymmetries in event number, and could therefore provide valuable information on the CP properties and the nature of the neutrinos, provided the solar magnetic field direction is fixed.

PhysicsNuclear and High Energy PhysicsParticle physicsScatteringSolar neutrinoHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)FísicaFOS: Physical sciencesElectronAstrophysicsAtomic and Molecular Physics and OpticsMagnetic fieldDipoleMAJORANAHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics::ExperimentNeutrinoEvent (particle physics)
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Bilinear R-parity violating SUSY: Neutrinoless double beta decay in the light of solar and atmospheric neutrino data

2000

Neutrinoless double beta ($\znbb$) decay is considered within bilinear R-parity breaking supersymmetry, including the full one-loop corrections to the neutrino-neutralino mass matrix. Expected rates for $\znbb$ decay in this model are discussed in light of recent atmospheric and solar neutrino data. We conclude that (a) tree-level calculations for $\znbb$ decay within the bilinear model are not reliable in the range of parameters preferred by current solar and atmospheric neutrino problems. And (b) if the solar and atmospheric neutrino problems are to be solved within bilinear R-parity violating SUSY the expected rates for $\znbb$ decay are very low; the effective Majorana neutrino mass at …

PhysicsNuclear and High Energy PhysicsParticle physicsSolar neutrinoHigh Energy Physics::PhenomenologyFOS: Physical sciencesBilinear interpolationFísicaSupersymmetryMass matrixMAJORANAHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Double beta decayR-parityHigh Energy Physics::ExperimentNeutrino
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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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Symmetrical Parametrizations of the Lepton Mixing Matrix

2011

Advantages of the original symmetrical form of the parametrization of the lepton mixing matrix are discussed. It provides a conceptually more transparent description of neutrino oscillations and lepton number violating processes like neutrinoless double beta decay, clarifying the significance of Dirac and Majorana phases. It is also ideal for parametrizing scenarios with light sterile neutrinos.

PhysicsNuclear and High Energy PhysicsParticle physicsSterile neutrino010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyPontecorvo–Maki–Nakagawa–Sakata matrixFísicaFOS: Physical sciences01 natural sciencesLepton numberHigh Energy Physics - ExperimentMAJORANAHigh Energy Physics - PhenomenologyHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciencesCP violationHigh Energy Physics::Experiment010306 general physicsNeutrino oscillationLepton
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Building the full Pontecorvo-Maki-Nakagawa-Sakata matrix from six independent Majorana-type phases

2009

In the framework of three light Majorana neutrinos, we show how to reconstruct, through the use of 3 x 3 unitarity, the full PMNS matrix from six independent Majorana-type phases. In particular, we express the strength of Dirac-type CP violation in terms of these Majorana-type phases by writing the area of the unitarity triangles in terms of these phases. We also study how these six Majorana phases appear in CP-odd weak-basis invariants as well as in leptonic asymmetries relevant for flavored leptogenesis.

PhysicsNuclear and High Energy PhysicsParticle physicsUnitarity010308 nuclear & particles physicsmedia_common.quotation_subjectHigh Energy Physics::Phenomenology01 natural sciencesAsymmetryPhysics::History of PhysicsMassless particleMAJORANADouble beta decayLeptogenesis0103 physical sciencesCP violationHigh Energy Physics::ExperimentNeutrino010306 general physicsParticle Physics - Phenomenologymedia_common
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On the CP asymmetries in Majorana neutrino decays

1997

We study the CP asymmetries in lepton number violating two body scattering processes and show explicitly how they vanish, in agreement with unitarity constraints. We relate these cross section asymmetries to the CP decay rate asymmetries of the intermediate massive neutrinos and show how the inclusion of the Universe expansion via Boltzmann equations is the key ingredient to allow the production of a non-vanishing asymmetry in spite of the unitarity constraint on the cross sections. We then show that the absorptive parts of both the one loop vertex and self energy corrections do contribute to the CP decay asymmetries.

PhysicsNuclear and High Energy PhysicsParticle physicsUnitarityScatteringmedia_common.quotation_subjectHigh Energy Physics::PhenomenologyFOS: Physical sciencesLepton numberAsymmetryHigh Energy Physics - Phenomenologysymbols.namesakeMAJORANAHigh Energy Physics - Phenomenology (hep-ph)Self-energyBoltzmann constantsymbolsHigh Energy Physics::ExperimentNeutrinomedia_common
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Bounds on Neutrino Transition Magnetic Moments in Random Magnetic Fields

1995

We consider the conversions of active to sterile Majorana neutrinos $\nu_{a}$ and $\nu_{s}$, due to neutrino transition magnetic moments in the presence of random magnetic fields (r.m.f.) generated at the electroweak phase transition. From a simple Schr\"{o}dinger-type evolution equation, we derive a stringent constraint on the corresponding transition magnetic moments and display it as a function of the domain size and field geometry. For typical parameter choices one gets limits much stronger than usually derived from stellar energy loss considerations. These bounds are consistent with the hypothesis of seeding of galactic magnetic fields by primordial fields surviving past the re-combina…

PhysicsNuclear and High Energy PhysicsPhase transitionParticle physicsField (physics)Magnetic momentElectroweak interactionHigh Energy Physics::PhenomenologyFísicaFOS: Physical sciencesMagnetic fieldHigh Energy Physics - PhenomenologyMAJORANASupernovaHigh Energy Physics - Phenomenology (hep-ph)Neutrino
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Oscillations of Dirac and Majorana neutrinos in matter and a magnetic field

2008

We study the evolution of massive mixed Dirac and Majorana neutrinos in matter under the influence of a transversal magnetic field. The analysis is based on relativistic quantum mechanics. We solve exactly the evolution equation for relativistic neutrinos, find the neutrino wave functions, and calculate the transition probability for spin-flavor oscillations. We analyze the dependence of the transition probability on the external fields and compare the cases of Dirac and Majorana neutrinos. The evolution of Majorana particles in vacuum is also studied and correction terms to the standard oscillation formula are derived and discussed. As a possible application of our results we discuss the s…

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physics010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyDirac (software)FOS: Physical sciencesRelativistic quantum mechanics01 natural sciencesHigh Energy Physics - PhenomenologyMAJORANAsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Dirac fermionQuantum electrodynamics0103 physical sciencessymbolsHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationMajorana equationPhysical Review D
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Minimal models with light sterile neutrinos

2011

We study the constraints imposed by neutrino oscillation experiments on the minimal extensions of the Standard Model (SM) with $n_R$ gauge singlet fermions ("right-handed neutrinos"), that can account for neutrino masses. We consider the most general coupling to SM fields of the new fields, in particular those that break lepton number and we do not assume any a priori hierarchy in the mass parameters. We proceed to analyze these models starting from the lowest level of complexity, defined by the number of extra fermionic degrees of freedom. The simplest choice that has enough free parameters in principle (i.e. two mass differences and two angles) to explain the confirmed solar and atmospher…

PhysicsNuclear and High Energy PhysicsSterile neutrinoParticle physics010308 nuclear & particles physicsFOS: Physical sciencesFísica01 natural sciences7. Clean energyLepton numberStandard ModelMiniBooNEHigh Energy Physics - PhenomenologyMAJORANAHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometry13. Climate action0103 physical sciencesNeutrino010306 general physicsNeutrino oscillation
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