Search results for "Instability"

showing 10 items of 724 documents

On reliability of systems with moving material subjected to fracture and instability

2015

Abstract The reliability of systems with moving cracked elastic and isotropic material is considered. The material is modeled as a moving plate which continually has a crack on the edge. The plate is subjected to homogeneous tension acting in the traveling direction and the tension varies temporally around a constant value, the set tension. The tension and the length of the crack are modeled by an Ornstein–Uhlenbeck process and an exponential Ornstein–Uhlenbeck process, respectively. Failure is regarded as the state at which the plate becomes unstable or fractures (or both) and a lower bound for the reliability of the system is derived. Considering reliability of the system leads to first p…

Aerospace EngineeringBoundary (topology)Ocean EngineeringInstabilityOrnstein–Uhlenbeck processfirst passage timerandom parametersCivil and Structural EngineeringMathematicsta214Tension (physics)business.industryMechanical EngineeringIsotropyStatistical and Nonlinear PhysicsOrnstein–Uhlenbeck processStructural engineeringMechanicsstabilitymoving plateCondensed Matter PhysicsNuclear Energy and EngineeringfractureFracture (geology)First-hitting-time modelConstant (mathematics)businessProbabilistic Engineering Mechanics
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Stochastic analysis of the critical velocity of an axially moving cracked elastic plate

2014

In this study, a probabilistic analysis of the critical velocity for an axially moving cracked elastic and isotropic plate is presented. Axially moving materials are commonly used in modelling of manufacturing processes, like paper making and plastic forming. In such systems, the most serious threats to runnability are instability and material fracture, and finding the critical value of velocity is essential for efficiency. In this paper, a formula for the critical velocity is derived under constraints for the probabilities of instability and fracture. The significance of randomness in different model parameters is investigated for parameter ranges typical of paper material and paper machin…

Aerospace EngineeringOcean EngineeringInstabilityRandomnessCivil and Structural EngineeringPhysicsta113Tension (physics)business.industryMechanical EngineeringplateIsotropypaperiStatistical and Nonlinear PhysicsMechanicsStructural engineeringmoving materialstabilityCondensed Matter PhysicsCritical valueCritical ionization velocityepävarmuusNuclear Energy and EngineeringfractureFracture (geology)businessAxial symmetryProbabilistic engineering mechanics
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Stabilizing lateral ankle instability by suture tape - a cadaver study.

2019

Abstract Background Suture tape is a recent development to augment a Brostrom repair at least during the healing phase of the native tissues used for stabilization of the lateral ankle ligaments. The purpose of this study was to evaluate whether suture tape is an effective mechanical stabilizer against anterior talar drawer in a cadaver experiment when tested with a validated arthrometer. Methods Different stability conditions were created in 14 cadaveric foot and leg specimens. Following anterior talofibular ligament (ATFL) dissection, isolated suture tape ATFL reconstruction was compared to the unaltered specimens, to the condition with ATFL cut, to the ATFL plus calcaneofibular ligament …

Aged 80 and overJoint InstabilityMaleSuture anchorlcsh:Diseases of the musculoskeletal systemArthrometry ArticularSuturesAugmentationLateral ankle instabilitylcsh:RD701-811Suture tapelcsh:Orthopedic surgerySuture AnchorsCadaverHumansCadaver studyFemalelcsh:RC925-935AnkleAgedResearch ArticleJournal of orthopaedic surgery and research
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On the enhancement of diffusion by chaos, escape rates and stochastic instability

1999

We consider stochastic perturbations of expanding maps of the interval where the noise can project the trajectory outside the interval. We estimate the escape rate as a function of the amplitude of the noise and compare it with the purely diffusive case. This is done under a technical hypothesis which corresponds to stability of the absolutely continuous invariant measure against small perturbations of the map. We also discuss in detail a case of instability and show how stability can be recovered by considering another invariant measure.

AmplitudeApplied MathematicsGeneral MathematicsCalculusTrajectoryInvariant measureInterval (mathematics)Statistical physicsAbsolute continuityNoise (electronics)Stability (probability)InstabilityMathematicsTransactions of the American Mathematical Society
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Dynamics of thick discs around Schwarzschild-de Sitter black holes

2003

We consider the effects of a cosmological constant on the dynamics of constant angular momentum discs orbiting Schwarzschild-de Sitter black holes. The motivation behind this study is to investigate whether the presence of a radial force contrasting the black hole's gravitational attraction can influence the occurrence of the runaway instability, a robust feature of the dynamics of constant angular momentum tori in Schwarzschild and Kerr spacetimes. In addition to the inner cusp near the black hole horizon through which matter can accrete onto the black hole, in fact, a positive cosmological constant introduces also an outer cusp through which matter can leave the torus without accreting on…

Angular momentumAstrophysics::High Energy Astrophysical PhenomenaAccretion discs ; Black holes ; Relativity ; Hydrodynamics ; Cosmological constantFOS: Physical sciencesCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)UNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsInstabilityGeneral Relativity and Quantum CosmologyRelativityGravitationGeneral Relativity and Quantum CosmologyDe Sitter universeCosmological constantPhysicsBlack holesHorizonAstrophysics (astro-ph)Astronomy and AstrophysicsTorus:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Classical mechanicsSpace and Planetary ScienceHydrodynamicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaSchwarzschild radiusAccretion discs:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Early induction of genetic instability and apoptosis by arsenic in cultured Chinese hamster cells

2002

In order to assess at what time from the beginning of exposure inorganic arsenic can give rise to genetic instability and trigger apoptosis, V79-C13 Chinese hamster cells were treated with 10 microM sodium arsenite for 24 h. Under these conditions, cell survival was >70% and cells showed neither an increase in chromosome aberration frequency nor a delay in cell cycle progression. Investigations, which were carried out every 6 h during the treatment, revealed an early appearance of genetically unstable cells, namely micronucleated, multinucleated and mononucleated 'giant' cells, as well as apoptotic cells. Indirect immunostaining using anti-beta-tubulin antibody showed severe alterations in …

ArsenitesCell SurvivalHealth Toxicology and MutagenesisPopulationMitosisHamsterApoptosisToxicologyChromosome aberrationChromosomesChinese hamsterCricetulusMultinucleateCricetinaeGeneticsAnimalseducationMitosisGenetics (clinical)Chromosome Aberrationseducation.field_of_studybiologyAneuploidybiology.organism_classificationSodium CompoundsMolecular biologyCell biologySettore BIO/18 - GeneticaCell cultureApoptosisCytogenetic AnalysisMutationarsenic genomic instability apoptosisFluorescein-5-isothiocyanate
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GW190521: A Binary Black Hole Merger with a Total Mass of 150  M⊙

2020

LIGO Scientific Collaboration and Virgo Collaboration: et al.

AstronomyGeneral Physics and Astronomydetector: networkAstrophysicsGravitational waves; Binary black holes Intermediate mass black holes01 natural sciencesGeneral Relativity and Quantum Cosmologygravitational waves; black holesGW190521 BBHIntermediate mass black holesLIGO10. No inequalityQCQBSettore FIS/01astro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPAIR-INSTABILITYSettore FIS/05Physicsstatistical analysis: BayesianSupernovaPhysical SciencesPhysique des particules élémentaires[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaGravitational wavedata analysis methodBinary black holes Intermediate mass black holesgr-qcPhysics MultidisciplinaryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Physics and Astronomy(all)Gravitation and AstrophysicsGravitational wavespair-instabilitySettore FIS/05 - Astronomia e AstrofisicaBinary black holeBinary black holesNeutron starsgravitational wavessupernova0103 physical sciences010306 general physicsLuminosity distanceSTFCGW190521Science & Technology9. Industry and infrastructureGravitational wavegravitational radiationRCUKblack hole: massgravitational waves black holegravitational radiation detectorLIGORedshiftBlack holewave: modelVIRGOblack hole: binaryIntermediate-mass black holegravitational radiation: emissionBBH[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Observation of Poincaré-Andronov-Hopf Bifurcation in Cyclotron Maser Emission from a Magnetic Plasma Trap.

2018

We report the first experimental evidence of a controlled transition from the generation of periodic bursts of electromagnetic radiation into the continuous-wave regime of a cyclotron maser formed in magnetically confined nonequilibrium plasma. The kinetic cyclotron instability of the extraordinary wave of weakly inhomogeneous magnetized plasma is driven by the anisotropic electron population resulting from electron cyclotron plasma heating in a MHD-stable minimum-$B$ open magnetic trap.

Astrophysics::High Energy Astrophysical PhenomenaCyclotronGeneral Physics and AstronomyElectronplasmafysiikka01 natural sciences7. Clean energyInstabilityElectromagnetic radiation010305 fluids & plasmaslaw.inventionsymbols.namesakePhysics::Plasma PhysicslawMagnetic trap0103 physical sciencesMaser010306 general physicsPhysicsHopf bifurcationta114plasma physicssyklotronitPlasmaPhysics::Space PhysicssymbolsAtomic physicscyclotronsPhysical review letters
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GRAVITATIONAL WAVE SIGNATURES IN BLACK HOLE FORMING CORE COLLAPSE

2013

We present numerical simulations in general relativity of collapsing stellar cores. Our initial model consists of a low metallicity rapidly-rotating progenitor which is evolved in axisymmetry with the latest version of our general relativistic code CoCoNuT, which allows for black hole formation and includes the effects of a microphysical equation of state (LS220) and a neutrino leakage scheme to account for radiative losses. The motivation of our study is to analyze in detail the emission of gravitational waves in the collapsar scenario of long gamma-ray bursts. Our simulations show that the phase during which the proto-neutron star (PNS) survives before ultimately collapsing to a black hol…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics01 natural sciencesInstabilityGeneral Relativity and Quantum Cosmology0103 physical sciencesRadiative transferAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsEinstein Telescope010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsVirgo ClusterBlack holeSupernovaNeutron starAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaThe Astrophysical Journal
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Stability analysis of relativistic jets from collapsars and its implications on the short-term variability of gamma-ray bursts

2002

We consider the transverse structure and stability properties of relativistic jets formed in the course of the collapse of a massive progenitor. Our numerical simulations show the presence of a strong shear in the bulk velocity of such jets. This shear can be responsible for a very rapid shear--driven instability that arises for any velocity profile. This conclusion has been confirmed both by numerical simulations and theoretical analysis. The instability leads to rapid fluctuations of the main hydrodynamical parameters (density, pressure, Lorentz factor, etc.). However, the perturbations of the density are effectively decoupled from those of the pressure because the beam of the jet is radi…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesgalaxies jetsAstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAInstabilitysymbols.namesakeAstrophysical jetISM jets and outflowsPhysicsBurstsGamma ray theoryTurbulenceAstrophysics (astro-ph)Magnetohydradynamics (MHD) : Gamma rays ; Bursts ; Gamma ray theory ; ISM jets and outflows ; galaxies jetsAstronomy and AstrophysicsMechanicsLight curve:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Transverse planeLorentz factorSpace and Planetary SciencesymbolsGamma rays [Magnetohydradynamics (MHD)]OutflowUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaGamma-ray burst:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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