Search results for "Domain Wall"

showing 10 items of 102 documents

A class of invisible axion models with FCNCs at tree level

2014

We build a class of invisible axion models with tree-level Flavor Changing Neutral Currents completely controlled by the fermion mixing matrices. The scalar sector of these models contains three-Higgs doublets and a complex scalar gauge singlet, with the same fermionic content than the Standard Model. A horizontal Peccei-Quinn symmetry provides a solution to the strong CP problem and predicts the existence of a very light and weakly coupled pseudo-Goldstone boson, the invisible axion or familon. A phenomenological analysis is performed taking into account familon searches in rare kaon and muon decays, astrophysical considerations and axion searches via axion-photon conversion. Drastic diffe…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsCabibbo–Kobayashi–Maskawa matrixScalar (mathematics)High Energy Physics::PhenomenologyFOS: Physical sciences01 natural sciencesSymmetry (physics)Standard ModelDomain wall (string theory)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesStrong CP problem010306 general physicsAxionBoson
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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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Domain-wall excitations in the two-dimensional Ising spin glass

2018

The Ising spin glass in two dimensions exhibits rich behavior with subtle differences in the scaling for different coupling distributions. We use recently developed mappings to graph-theoretic problems together with highly efficient implementations of combinatorial optimization algorithms to determine exact ground states for systems on square lattices with up to $10\,000\times 10\,000$ spins. While these mappings only work for planar graphs, for example for systems with periodic boundary conditions in at most one direction, we suggest here an iterative windowing technique that allows one to determine ground states for fully periodic samples up to sizes similar to those for the open-periodic…

PhysicsQuantum PhysicsSpin glassStatistical Mechanics (cond-mat.stat-mech)SpinsPhase (waves)FOS: Physical sciencesDisordered Systems and Neural Networks (cond-mat.dis-nn)Condensed Matter - Disordered Systems and Neural NetworksComputational Physics (physics.comp-ph)01 natural sciences010305 fluids & plasmasTheoretical physicsDomain wall (magnetism)Spin wave0103 physical sciencesCombinatorial optimizationIsing spinQuantum Physics (quant-ph)010306 general physicsPhysics - Computational PhysicsCritical exponentCondensed Matter - Statistical MechanicsPhysical Review B
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Fluctuations and lack of self-averaging in the kinetics of domain growth

1986

The fluctuations occurring when an initially disordered system is quenched at timet=0 to a state, where in equilibrium it is ordered, are studied with a scaling theory. Both the mean-sizel(t)d of thed-dimensional ordered domains and their fluctuations in size are found to increase with the same power of the time; their relative size fluctuations are independent of the total volumeLd of the system. This lack of self-averaging is tested for both the Ising model and the φ4 model on the square lattice. Both models exhibit the same lawl(t)=(Rt)x withx=1/2, although the φ4 model has “soft walls”. However, spurious results withx≷1/2 are obtained if “bad” pseudorandom numbers are used, and if the n…

PhysicsSelf-averagingSingularityDomain wall (magnetism)Monte Carlo methodExponentGeneral Materials ScienceIsing modelStatistical physicsCondensed Matter PhysicsSpurious relationshipSquare latticeElectronic Optical and Magnetic MaterialsZeitschrift für Physik B Condensed Matter
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Light majoron cold dark matter from topological defects and the formation of boson stars

2019

We show that for a relatively light majoron ($\ll 100 $ eV) non-thermal production from topological defects is an efficient production mechanism. Taking the type I seesaw as benchmark scheme, we estimate the primordial majoron abundance and determine the required parameter choices where it can account for the observed cosmological dark matter. The latter is consistent with the scale of unification. Possible direct detection of light majorons with future experiments such as PTOLEMY and the formation of boson stars from the majoron dark matter are also discussed.

PhysicsmonopolesParticle physicsCold dark matterCosmology and Nongalactic Astrophysics (astro-ph.CO)cosmological neutrinosdomain wallsCosmic stringsDark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCosmology of Theories beyond the SMTopological defectCosmic stringStarsHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Seesaw molecular geometryparticle physics – cosmology connectionMajoronBosonAstrophysics - Cosmology and Nongalactic Astrophysics
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Geometrical control of pure spin current induced domain wall depinning.

2017

[EN] We investigate the pure spin-current assisted depinning of magnetic domain walls in half ring based Py/Al lateral spin valve structures. Our optimized geometry incorporating a patterned notch in the detector electrode, directly below the Al spin conduit, provides a tailored pinning potential for a transverse domain wall and allows for a precise control over the magnetization configuration and as a result the domain wall pinning. Due to the patterned notch, we are able to study the depinning field as a function of the applied external field for certain applied current densities and observe a clear asymmetry for the two opposite field directions. Micromagnetic simulations show that this …

Pure spin currentField (physics)Magnetic domainGeometrical constrictions in nanostructuresSpin valve02 engineering and technology01 natural sciencesMagnetization0103 physical sciencesComputational physicsGeneral Materials Science[PHYS.COND]Physics [physics]/Condensed Matter [cond-mat]010306 general physicsComputingMilieux_MISCELLANEOUSSpin-½PhysicsCondensed matter physicsMagnetismSpin-transfer torque021001 nanoscience & nanotechnologyCondensed Matter PhysicsDomain wall motionDomain wall (magnetism)Spin Hall effect0210 nano-technologyJournal of physics. Condensed matter : an Institute of Physics journal
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Cosmic implications of a low-scale solution to the axion domain wall problem

2019

The post-inflationary breaking of Peccei-Quinn (PQ) symmetry can lead to the cosmic domain wall catastrophe. In this Letter we show how to avoid domain walls implementing the Instanton Interference Effect (IIE) with a new interaction which itself breaks PQ symmetry and confines at an energy scale smaller than $\Lambda_{QCD}$. We give a general description of the mechanism and consider its cosmological implications and constraints within a minimal model. Contrary to other mechanisms we do not require an inverse phase transition neither fine-tuned bias terms. Incidentally, the mechanism leads to the introduction of new self-interacting dark matter candidates and the possibility of producing g…

Quantum chromodynamicsPhysicsInstantonParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)010308 nuclear & particles physicsDark matterHigh Energy Physics::PhenomenologyFOS: Physical sciencesInverse01 natural sciencesHidden sectorDomain wall (string theory)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsAxionEnergy (signal processing)Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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Perturbative chiral violations for domain-wall QCD with improved gauge actions

2006

We investigate, in the framework of perturbation theory at finite $N_s$, the effectiveness of improved gauge actions in suppressing the chiral violations of domain-wall fermions. Our calculations show substantial reductions of the residual mass when it is compared at the same value of the gauge coupling, the largest suppression being obtained when the DBW2 action is used. Similar effects can also be observed for a power-divergent mixing coefficient which is chirally suppressed. No significant reduction instead can be seen in the case of the difference between the vector and axial-vector renormalization constants when improved gauge actions are used in place of the plaquette action. We also …

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyHigh Energy Physics - Lattice (hep-lat)FOS: Physical sciencesFermionGauge (firearms)01 natural sciencesRenormalizationDomain wall (string theory)High Energy Physics - LatticeLattice gauge theory0103 physical sciencesPerturbation theory (quantum mechanics)010306 general physicsMixing (physics)
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