Search results for "String Theory"

showing 10 items of 75 documents

Flavour-violating charged lepton decays in seesaw-type models

1994

Analytic expressions of lepton-flavour- and lepton-number-violating decays of charged leptons are derived in the context of general $SU(2)_L\otimes U(1)_Y$ seesaw scenarios that are motivated by grand unified theories (GUT's) or superstring models, in which left-handed and/or right-handed neutral singlets are present. Possible constraints imposed by cosmology and low-energy data are briefly discussed. The violation of the decoupling theorem in flavour-dependent graphs due to the presence of heavy neutral leptons of Dirac or Majorana nature is emphasized. Numerical estimates reveal that the decays $\tau^-\to e^-e^-e^+$ or $\tau^-\to e^-\mu^-\mu^+$ can be as large as $\sim 10^{-6}$, which may…

PhysicsNuclear and High Energy PhysicsParticle physicsDirac (video compression format)High Energy Physics::PhenomenologyFOS: Physical sciencesSuperstring theoryContext (language use)Lepton flavour violation ; seesaw ; singlet Majorana/Dirac neutrinosType (model theory)CosmologyHigh Energy Physics - PhenomenologyMAJORANAHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryHigh Energy Physics::ExperimentLepton
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Lepton physics versus neutrino mass

1990

Abstract The relationship between the strength of lepton flavour violating processes and the magnitude of the neutrino mass is rather model dependent. I review this question within different neutrino mixing models including superstring inspired models. Processes such as μ → e + γ , μ → 3 e , μ - e conversion in nuclei, etc. as well as lepton flavour violating Z ° decays can occur even if the physical neutrinos are strictly massless. As a result, the corresponding rates are unconstrained by bounds on the neutrino mass that follow from laboratory, astrophysics and cosmology and can therefore be large. Leptonic CP violation may also occur even when the physical neutrinos are strictly massless.

PhysicsNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::PhenomenologySuperstring theoryAtomic and Molecular Physics and OpticsCosmologyNuclear physicsMassless particleCP violationMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationLeptonNuclear Physics B - Proceedings Supplements
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Production mechanisms and signatures of isosinglet neutral heavy leptons in Z0 decays

1990

Abstract Neutral Heavy Leptons (NHLs) arise in many extensions of the standard electroweak theory such as superstring inspired models. The possibility of gauge singlets NHLs is especially attractive because it gives an explanation for the observed smallness of the neutrino mass. Existing limits on the possible existence of such particles are still fairly poor. We have investigated isosinglet NHL production and decays within different models. The dominant production cross section is single production (i.e. Z 0 → N + ν or Z 0 → N + ν ) as a result of mixing with the standard doublet neutrinos. Subsequent NHL decays lead to striking signatures. Taking into account the expected luminosities and…

PhysicsNuclear and High Energy PhysicsParticle physicsNeutral currentHigh Energy Physics::PhenomenologyElectroweak interactionFísicaSuperstring theoryGauge (firearms)Nuclear physicsHigh Energy Physics::ExperimentNeutrinoMixing (physics)Charged currentParticle Physics - PhenomenologyLeptonNuclear Physics B
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NON-PERTURBATIVE VACUUM WAVE-FUNCTIONAL AND CLOSED STRING EQUATIONS OF MOTION

1989

The anomalous conformal dependence of the vacuum wave-functional is studied in the non-perturbative regime of the closed bosonic string theory. It is shown that the vanishing of the vacuum expectation value of the stress-energy tensor trace leads to the implementation of a suitable variational condition on the wave-functional, provided that the dilaton condensate be taken as a conformal compensator for the graviton condensate of the embedding space.

PhysicsNuclear and High Energy PhysicsQED vacuumBosonic string theoryGravitonGeneral Physics and AstronomyAstronomy and AstrophysicsString field theoryGeneral Relativity and Quantum CosmologyNon-critical string theoryClassical mechanicsString cosmologyDilatonVacuum expectation valueModern Physics Letters A
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Analysis method for detecting topological defect dark matter with a global magnetometer network

2019

Abstract The Global Network of Optical Magnetometers for Exotic physics searches (GNOME) is a network of time-synchronized, geographically separated, optically pumped atomic magnetometers that is being used to search for correlated transient signals heralding exotic physics. GNOME is sensitive to exotic couplings of atomic spins to certain classes of dark matter candidates, such as axions. This work presents a data analysis procedure to search for axion dark matter in the form of topological defects: specifically, walls separating domains of discrete degenerate vacua in the axion field. An axion domain wall crossing the Earth creates a distinctive signal pattern in the network that can be d…

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Field (physics)Spins010308 nuclear & particles physicsMagnetometerDark matterFOS: Physical sciencesAstronomy and Astrophysics01 natural sciencesTopological defectlaw.inventionDomain wall (string theory)Space and Planetary Sciencelaw0103 physical sciencesAstrophysics - Instrumentation and Methods for Astrophysics010303 astronomy & astrophysicsAxionInstrumentation and Methods for Astrophysics (astro-ph.IM)GnomeAstrophysics - Cosmology and Nongalactic Astrophysics
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Spontaneous Breaking of Lepton Number and Cosmological Domain Wall Problem

2019

We show that if global lepton number symmetry is spontaneously broken in a post inflation epoch, then it can lead to the formation of cosmological domain walls. This happens in the well-known "Majoron paradigm" for neutrino mass generation. We propose some realistic examples which allow spontaneous lepton number breaking to be safe from such domain walls.

PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Mass generationHigh Energy Physics::PhenomenologyGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesLepton numberSymmetry (physics)High Energy Physics - PhenomenologyDomain wall (string theory)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesDomain (ring theory)High Energy Physics::ExperimentNeutrino010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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An invisible axion model with controlled FCNCs at tree level

2015

We derive the necessary conditions to build a class of invisible axion models with Flavor Changing Neutral Currents at tree-level controlled by the fermion mixing matrices and present an explicit model implementation. A horizontal Peccei-Quinn symmetry provides a solution to the strong CP problem via the Peccei-Quinn mechanism and predicts a cold dark mater candidate, the invisible axion or familon. The smallness of active neutrino masses can be explained via a type I seesaw mechanism, providing a dynamical origin for the heavy seesaw scale. The possibility to avoid the domain wall problem stands as one of the most interesting features of the type of models considered. Experimental limits r…

PhysicsParticle physicsNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsDark matterHigh Energy Physics::PhenomenologyFOS: Physical scienceslcsh:QC1-999Domain wall (string theory)High Energy Physics - PhenomenologySeesaw mechanismHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryStrong CP problemNeutrinoAxionMixing (physics)lcsh:PhysicsPhysics Letters B
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Deforming D-brane models on T6/(Z2×Z2M) orbifolds

2016

We review the stabilisation of complex structure moduli in Type IIA orientifolds, especially on with discrete torsion, via deformations of orbifold singularities. While D6-branes in SO(2N) and USp(2N) models always preserve supersymmetry and thus give rise to flat directions, in an exemplary Pati-Salam model with only U(N) gauge groups ten out of the 15 deformation moduli can be stabilised at the orbifold point.

PhysicsPati–Salam model010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGeneral Physics and AstronomySupersymmetryString theory01 natural sciencesModuliHigh Energy Physics::TheoryTheoretical physicsClassical mechanicsOrientifold0103 physical sciencesGravitational singularityD-brane010306 general physicsMathematics::Symplectic GeometryOrbifoldFortschritte der Physik
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The Einstein field equation in a multidimensional universe

1988

String theory [4] predicts that the universe has 10 or 26 dimensions. A salient problem is how the Einstein field equation should be written in terms of these revivified Kaluza-Klein cosmologies. The answer is by now well-known, yet nobody seems to have rewritten the seminal computation in [6] where an unnecessarily involved Euler-Lagrange variational method is employed and, curiously enough, no allusion to the Gauss-Bonnet-Chern theorem is made. We provide a more straightforward argument, which has been inspired by Hilbert's original derivation of the Einstein field equation [5].

PhysicsPhysics and Astronomy (miscellaneous)media_common.quotation_subjectComputationString theorynobodyUniverseHigh Energy Physics::TheoryGeneral Relativity and Quantum Cosmologysymbols.namesakeVariational methodDifferential geometryAllusionsymbolsEinsteinmedia_commonMathematical physicsGeneral Relativity and Gravitation
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Spectrum of the QCD flux tube in 3d SU(2) lattice gauge theory

2009

Abstract Evidence from the lattice suggests that formation of a flux tube between a q q ¯ pair in the QCD vacuum leads to quark confinement. For large separations between the quarks, it is conjectured that the flux tube has a behavior similar to an oscillating bosonic string, supported by lattice data for the groundstate q q ¯ potential. We measure the excited states of the flux tube in 3d SU ( 2 ) gauge theory with three different couplings inside the scaling region. We compare our results to predictions of effective string theories.

PhysicsQuantum chromodynamicsNuclear and High Energy PhysicsParticle physicsFlux tubeHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyQCD vacuumLattice field theoryLattice QCDNon-critical string theoryHamiltonian lattice gauge theoryLattice gauge theoryQuantum electrodynamicsPhysics Letters B
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