Search results for "Dirac fermion"

showing 10 items of 18 documents

Spin-1 Heisenberg chain and the one-dimensional fermion gas.

1989

The composite-spin representation of the spin-1 Heisenberg chain is used to transform it through the Jordan-Wigner transformation to the one-dimensional fermion gas. To properly include the xy couplings between spins, we also consider the bosonized version of the fermion model. Phase diagrams deduced from the two versions of the fermion model are compared against numerical results for finite Heisenberg chains. One of the symmetries of the spin model is lost in the fermionization, and this leads to a topologically incorrect phase diagram in at least one part of the parameter space. There are clear indications of significant coupling of spin and charge degrees of freedom in the fermion model …

Coupling constantPhysicsFermion doublingHelical Dirac fermionHeisenberg modelHigh Energy Physics::LatticeFermionRenormalizationsymbols.namesakeDirac fermionQuantum mechanicssymbolsSpin modelCondensed Matter::Strongly Correlated ElectronsPhysical review. B, Condensed matter
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Exactly solvable relativistic model with the anomalous interaction

2010

A special class of Dirac-Pauli equations with time-like vector potentials of an external field is investigated. An exactly solvable relativistic model describing the anomalous interaction of a neutral Dirac fermion with a cylindrically symmetric external electromagnetic field is presented. The related external field is a superposition of the electric field generated by a charged infinite filament and the magnetic field generated by a straight line current. In the nonrelativistic approximation the considered model is reduced to the integrable Pron'ko-Stroganov model.

Electromagnetic fieldPhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciMeccanica QuantisticaFermionRelativitàAtomic and Molecular Physics and OpticsSymmetry (physics)Settore FIS/03 - Fisica Della MateriaMagnetic fieldSuperposition principlesymbols.namesakeDirac fermionQuantum electrodynamicsElectric fieldsymbolsRelativistic wave equations
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Electromagnetic Duality Anomaly in Curved Spacetimes

2016

The source-free Maxwell action is invariant under electric-magnetic duality rotations in arbitrary spacetimes. This leads to a conserved classical Noether charge. We show that this conservation law is broken at the quantum level in presence of a background classical gravitational field with a non-trivial Chern-Pontryagin invariant, in a parallel way to the chiral anomaly for massless Dirac fermions. Among the physical consequences, the net polarization of the quantum electromagnetic field is not conserved.

High Energy Physics - TheoryElectromagnetic fieldFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakeGravitational field0103 physical sciences010306 general physicsQuantumMathematical PhysicsMathematical physicsPhysicsChiral anomalyQuantum PhysicsConservation law010308 nuclear & particles physicsMathematical Physics (math-ph)Invariant (physics)Classical mechanicsHigh Energy Physics - Theory (hep-th)Dirac fermionsymbolsNoether's theoremQuantum Physics (quant-ph)Physical Review Letters
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Adiabatic regularization and particle creation for spin one-half fields

2013

The extension of the adiabatic regularization method to spin-$1/2$ fields requires a self-consistent adiabatic expansion of the field modes. We provide here the details of such expansion, which differs from the WKB ansatz that works well for scalars, to firmly establish the generalization of the adiabatic renormalization scheme to spin-$1/2$ fields. We focus on the computation of particle production in de Sitter spacetime and obtain an analytic expression of the renormalized stress-energy tensor for Dirac fermions.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Quantum field theory in curved spacetimeFOS: Physical sciencesFísicaGeneral Relativity and Quantum Cosmology (gr-qc)Mathematical Physics (math-ph)Adiabatic quantum computationGeneral Relativity and Quantum CosmologyWKB approximationRenormalizationsymbols.namesakeGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Dirac fermionRegularization (physics)symbolsAdiabatic processMathematical PhysicsAstrophysics - Cosmology and Nongalactic AstrophysicsMathematical physicsAnsatz
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Impact of nitrogen doping on the band structure and the charge carrier scattering in monolayer graphene

2021

The addition of nitrogen as a dopant in monolayer graphene is a flexible approach to tune the electronic properties of graphene as required for applications. Here, we investigate the impact of the doping process that adds N dopants and defects on the key electronic properties, such as the mobility, the effective mass, the Berry phase, and the scattering times of the charge carriers. Measurements at low temperatures and magnetic fields up to 9 T show a decrease of the mobility with increasing defect density due to elastic, short-range scattering. At low magnetic fields weak localization indicates an inelastic contribution depending on both defects and dopants. Analysis of the effective mass …

Materials sciencePhysics and Astronomy (miscellaneous)DopantCondensed matter physics530 PhysicsScatteringGrapheneDoping530 Physiklaw.inventionWeak localizationCondensed Matter::Materials Sciencesymbols.namesakeEffective mass (solid-state physics)Dirac fermionlawPhysics::Atomic and Molecular ClusterssymbolsGeneral Materials ScienceCharge carrierPhysical Review Materials
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Can one ever prove that neutrinos are Dirac particles?

2017

According to the "Black Box" theorem the experimental confirmation of neutrinoless double beta decay ($0 \nu 2 \beta$) would imply that at least one of the neutrinos is a Majorana particle. However, a null $0 \nu 2 \beta$ signal cannot decide the nature of neutrinos, as it can be suppressed even for Majorana neutrinos. In this letter we argue that if the null $0 \nu 2 \beta$ decay signal is accompanied by a $0 \nu 4 \beta$ quadruple beta decay signal, then at least one neutrino should be a Dirac particle. This argument holds irrespective of the underlying processes leading to such decays.

Nuclear and High Energy PhysicsParticle physicsNuclear TheoryAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentNuclear Theory (nucl-th)symbols.namesakeHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Double beta decay0103 physical sciencesNuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentPhysics010308 nuclear & particles physicsDirac (video compression format)Null (mathematics)High Energy Physics::PhenomenologyBeta decaylcsh:QC1-999MAJORANAHigh Energy Physics - PhenomenologyDirac fermionsymbolsHigh Energy Physics::ExperimentNeutrinolcsh:Physics
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Dirac neutrinos from flavor symmetry

2013

We present a model where Majorana neutrino mass terms are forbidden by the flavor symmetry group Delta(27). Neutrinos are Dirac fermions and their masses arise in the same way as that of the charged fermions, due to very small Yukawa couplings. The model fits current neutrino oscillation data and correlates the octant of the atmospheric angle with the magnitude of the lightest neutrino mass, with maximal mixing excluded for any neutrino mass

Nuclear and High Energy PhysicsParticle physicsSterile neutrinoNeutrino theory of lightPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::LatticePontecorvo–Maki–Nakagawa–Sakata matrixFOS: Physical sciences7. Clean energy01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaSolar neutrino problemHigh Energy Physics - PhenomenologyDirac fermionsymbolsMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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Leptophobic dark matter and the baryon number violation scale

2019

We discuss the possible connection between the scale for baryon number violation and the cosmological bound on the dark matter relic density. A simple gauge theory for baryon number which predicts the existence of a leptophobic cold dark matter particle candidate is investigated. In this context, the dark matter candidate is a Dirac fermion with mass defined by the new symmetry breaking scale. Using the cosmological bounds on the dark matter relic density we find the upper bound on the symmetry breaking scale around 200 TeV. The properties of the leptophobic dark matter candidate are investigated in great detail and we show the prospects to test this theory at current and future experiments…

Particle physicsCold dark mattermedia_common.quotation_subjectDark matterFOS: Physical sciencesContext (language use)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAsymmetryPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)symbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesSymmetry breaking010306 general physicsmedia_commonPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHigh Energy Physics - PhenomenologyDirac fermionAntimattersymbolsBaryon numberPhysical Review
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Observational constraints on decoupled hidden sectors

2016

We consider an extension of the Standard Model with a singlet sector consisting of a real (pseudo)scalar and a Dirac fermion coupled with the Standard Model only via the scalar portal. We assume that the portal coupling is weak enough for the singlet sector not to thermalize with the Standard Model allowing the production of singlet particles via the freeze-in mechanism. If the singlet sector interacts with itself sufficiently strongly, it may thermalize within itself, resulting in dark matter abundance determined by the freeze-out mechanism operating within the singlet sector. We investigate this scenario in detail. In particular, we show that requiring the absence of inflationary isocurva…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterScalar (mathematics)FOS: Physical sciencesParameter space114 Physical sciences01 natural sciencesStandard Modeldecouplingsymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)ABELL 38270103 physical sciencesSinglet state010306 general physicsdark matter abundanceInflation (cosmology)PhysicsINTERACTING DARK-MATTERta114010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyextensions of the Standard ModelHidden sectorHigh Energy Physics - Phenomenologysinglet sectorCOSMOLOGICAL SIMULATIONSDirac fermionGALAXY CLUSTER 1E-0657-56symbols3.5 KEV LINEINTERACTION CROSS-SECTIONAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Topological insulators in filled skutterudites

2011

We propose new topological insulators in cerium filled skutterudite (FS) compounds based on ab initio calculations. We find that two compounds CeOs4As12 and CeOs4Sb12 are zero gap materials with band inversion between Os-d and Ce-f orbitals, which are thus parent compounds of two and three-dimensional topological insulators just like bulk HgTe. At low temperature, both compounds become topological Kondo insulators, which are Kondo insulators in the bulk, but have robust Dirac surface states on the boundary. This new family of topological insulators has two advantages compared to previous ones. First, they can have good proximity effect with other superconducting FS compounds to realize Maja…

PhysicsCondensed Matter - Materials ScienceCondensed matter physicsKondo insulatorLattice (group)Materials Science (cond-mat.mtrl-sci)FOS: Physical sciencesFermionCondensed Matter PhysicsElectronic Optical and Magnetic Materialssymbols.namesakeDirac fermionTopological insulatorProximity effect (superconductivity)symbolsTopological orderCondensed Matter::Strongly Correlated ElectronsCharge transfer insulatorsPhysical Review B
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