Search results for "Bilin"

showing 10 items of 377 documents

Neutralino phenomenology at LEP2 in supersymmetry with bilinear breaking of R-parity

2000

We discuss the phenomenology of the lightest neutralino in models where an effective bilinear term in the superpotential parametrizes the explicit breaking of R-parity. We consider supergravity scenarios where the lightest supersymmetric particle (LSP) is the lightest neutralino and which can be explored at LEP2. We present a detailed study of the LSP decay properties and general features of the corresponding signals expected at LEP2. We also contrast our model with gauge mediated supersymmetry breaking.

PhysicsFenomenología del NeutralinoNuclear and High Energy PhysicsParticle physicsParidad RSupergravityHigh Energy Physics::LatticeSuperpotentialHigh Energy Physics::PhenomenologyFOS: Physical sciencesFísicaSupersymmetryLightest Supersymmetric ParticleSupersymmetry breakingLEP2High Energy Physics - PhenomenologyHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)SupersimetríaR-parityNeutralinoHigh Energy Physics::ExperimentPhenomenology (particle physics)Ruptura bilineal
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Bright and dark optical solitons in fiber media with higher-order effects

2002

We consider N-coupled higher-order nonlinear Schrodinger (N-CHNLS) equations which govern the simultaneous propagation of N optical fields in fiber media with higher-order effects. Bright and dark soliton solutions are derived using Hirota bilinear method for the general cross-coupling ratio between the parameters of self-phase modulation and cross-phase modulation effects. By means of coupled amplitude-phase formulation also, similar kind of dark soliton solutions are obtained. It is found that the parametric conditions for the simultaneous propagation of N dark solitons from both the methods are the same.

PhysicsGeneral MathematicsApplied MathematicsGeneral Physics and AstronomyBilinear interpolationStatistical and Nonlinear PhysicsNonlinear systemsymbols.namesakeNonlinear Sciences::Exactly Solvable and Integrable SystemsTransmission (telecommunications)ModulationQuantum mechanicssymbolsSolitonFiberNonlinear Sciences::Pattern Formation and SolitonsSchrödinger's catParametric statisticsChaos, Solitons & Fractals
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Superfield commutators for D = 4 chiral multiplets and their apppications

1987

The superfield commutators and their corresponding equal-time limits are derived in a covariant way for the D=4 free massive chiral multiplet. For interesting chiral multiplets, the general KAllen-Lehmann representation is also introduced. As applications of the free superfield commutators, the general solution of the Cauchy problem for chiral superfields is given, and an analysis of the closure of the bilinear products of superfields which desrcibe the extension of the internal currents for free supersymmetric chiral matter is performed.

PhysicsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyClosure (topology)General Physics and AstronomyBilinear interpolationSuperfieldHigh Energy Physics::TheoryNonlinear Sciences::Exactly Solvable and Integrable SystemsChiral superfieldQuantum electrodynamicsInitial value problemCovariant transformationRepresentation (mathematics)MultipletMathematical physicsCzechoslovak Journal of Physics B
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Testing the mechanism of R-parity breaking with slepton LSP decays

2003

In supersymmetric models R-parity can be violated through either bilinear or trilinear terms in the superpotential, or both. If charged scalar leptons are the lightest supersymmetric particles, their decay properties can be used to obtain information about the relative importance of these couplings. We show that in some specific scenarios it is even possible to decide whether bilinear or trilinear terms give the dominant contribution to the neutrino mass matrix.

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsScalar (mathematics)SuperpotentialHigh Energy Physics::PhenomenologyFOS: Physical sciencesBilinear interpolationFísicaSupersymmetry01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)Nonlinear Sciences::Exactly Solvable and Integrable SystemsR-parity0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsNeutrino oscillationLepton
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Solar Neutrino Masses and Mixing from Bilinear R-Parity Broken Supersymmetry: Analytical versus Numerical Results

2003

We give an analytical calculation of solar neutrino masses and mixing at one-loop order within bilinear R-parity breaking supersymmetry, and compare our results to the exact numerical calculation. Our method is based on a systematic perturbative expansion of R-parity violating vertices to leading order. We find in general quite good agreement between approximate and full numerical calculation, but the approximate expressions are much simpler to implement. Our formalism works especially well for the case of the large mixing angle MSW solution (LMA-MSW), now strongly favoured by the recent KamLAND reactor neutrino data.

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsSolar neutrinoHigh Energy Physics::PhenomenologyFOS: Physical sciencesBilinear interpolationFeynman graphSupersymmetry01 natural sciencesFormalism (philosophy of mathematics)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)R-parity0103 physical sciencesBibliographyReactor neutrino010306 general physics
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Neutrinoless double beta decay in supersymmetry with bilinear R-parity breaking

1998

We reanalyze the contributions to neutrinoless double beta ($\znbb$) decay from supersymmetry with explicit breaking of R-parity. Although we keep both bilinear and trilinear terms, our emphasis is put on bilinear R-parity breaking terms, because these mimic more closely the models where the breaking of R-parity is spontaneous. Comparing the relevant Feynman diagrams we conclude that the usual mass mechanism of double beta decay is the dominant one. From the non-observation of $\znbb$ decay we set limits on the bilinear R-parity breaking parameters of typically a (few) 100 $keV$. Despite such stringent bounds, we stress that the magnitude of R-parity violating phenomena that can be expected…

PhysicsNuclear and High Energy PhysicsParticle physicsFOS: Physical sciencesBilinear interpolationFísicaSupersymmetryFirst generationThird generationHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Double beta decayR-paritysymbolsFeynman diagramBeta (velocity)High Energy Physics::Experiment
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On the classification of accidental symmetries of the two Higgs doublet model potential

2011

Recently, it has been shown [arXiv:1106.3482] that the two-Higgs-doublet-model potential may exhibit a maximum of 13 distinct accidental symmetries. Such a classification is based on a six-dimensional bilinear scalar field formalism realizing the SO(1,5) symmetry group. This note presents the transformation relations for each of the 13 symmetries in the original scalar field space and their one-to-one correspondence to the space of scalar bilinears, thereby providing firm support for the completeness of the classification.

PhysicsNuclear and High Energy PhysicsParticle physicsScalar (mathematics)FOS: Physical sciencesBilinear interpolationSymmetry groupHigh Energy Physics - PhenomenologyTheoretical physicsTwo-Higgs-doublet modelHiggs fieldHigh Energy Physics - Phenomenology (hep-ph)Homogeneous spaceHiggs bosonScalar fieldPhysics Letters B
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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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R-parity violating sneutrino decays

2004

R-parity can be violated through either bilinear and/or trilinear terms in the superpotential. The decay properties of sneutrinos can be used to obtain information about the relative importance of these couplings provided sneutrinos are the lightest supersymmetric particles. We show that in some specific scenarios it is even possible to decide whether bilinear or trilinear terms give the dominant contribution to the neutrino mass matrix.

PhysicsNuclear and High Energy PhysicsParticle physicsSuperpotentialHigh Energy Physics::PhenomenologyBilinear interpolationFOS: Physical sciencesFísicaMass matrixHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Nonlinear Sciences::Exactly Solvable and Integrable SystemsR-parityHigh Energy Physics::ExperimentNeutrino
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Charged Higgs mass bounds from b → sγ in a bilinear R-parity violating model

1998

The experimental measurement of $B(b \to s\gamma)$ imposes important constraints on the charged Higgs boson mass in the MSSM. If squarks are in the few TeV range, the charged Higgs boson mass in the MSSM must satisfy $m_{H^{\pm}} \gsim 440$ GeV. For lighter squarks, then light charged Higgs bosons can be reconciled with $B(b \to s\gamma)$ only if there is also a light chargino. In the MSSM if we impose $m_{\chi^{\pm}_1}>90$ GeV then we need $m_{H^{\pm}} \gsim 110$ GeV. We show that by adding bilinear R--Parity violation (BRpV) in the tau sector, these bounds are relaxed. The bound on $m_{H^{\pm}}$ in the MSSM--BRpV model is $\gsim 340$ GeV for the the heavy squark case and $m_{H^{\pm}} \gsi…

PhysicsNuclear and High Energy PhysicsRange (particle radiation)Particle physicsHigh Energy Physics::PhenomenologyFísicaBilinear interpolationObservableHigh Energy Physics - PhenomenologyCharginoR-parityHiggs bosonRelaxation (physics)High Energy Physics::ExperimentBosonNuclear Physics B
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