Search results for "LIMIT"

showing 10 items of 2826 documents

Design of the friction stir welding tool using the continuum based FEM model

2006

In friction stir welding (FSW), the welding tool geometry plays a fundamental role in obtaining desirable microstructures in the weld and the heat-affected zones, and consequently improving strength and fatigue resistance of the joint. In this paper, a FSW process with varying pin geometries (cylindrical and conical) and advancing speeds is numerically modeled, and a thermo-mechanically coupled, rigid-viscoplastic, fully 3D FEM analysis able to predict the process variables as well as the material flow pattern and the grain size in the welded joints is performed. The obtained results allow finding optimal tool geometry and advancing speed for improving nugget integrity of aluminum alloys.

Heat-affected zoneMaterials scienceViscoplasticitybusiness.industryMechanical EngineeringWeldingStructural engineeringConical surfaceCondensed Matter PhysicsFatigue limitFinite element methodStatistics::Computationlaw.inventionMaterial flowMechanics of MaterialslawFriction stir weldingGeneral Materials SciencebusinessMaterials Science and Engineering: A
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Analysis of cannabinoids by liquid chromatography–mass spectrometry in milk, liver and hemp seed to ensure food safety

2017

A method for determining cannabinoids, Δ9-tetrahidrocannabinol (THC), 11-nor-9-carboxy-Δ9-THC (THC-COOH) and 11-hidroxy-Δ9-THC (THC-OH) in milk, liver and hemp seeds based on liquid chromatography tandem mass spectrometry has been optimized and validated. Analytes were extracted with methanol and the extracts cleaned-up by solid-phase extraction using Oasis HLB (60 mg). The developed method was validated according to the Commission Decision 2002/657/EC. The decision limit (CCα) and detection capability (CCβ) ranged from 3.10–10.5 ng g−1 and 3.52–11.5 ng g−1, the recoveries were 76–118% and matrix effect ranged from −17.8% to 19.9% in the three matrices studied. The method was applied to foo…

Hemp seedFood Safety010501 environmental sciences01 natural sciencesMass SpectrometryAnalytical ChemistryFood safetyLC–MS/MSLiquid chromatography–mass spectrometryLc ms msAnimalsSolid phase extraction0105 earth and related environmental sciencesSolid-phase extractionChromatographyChemistrybusiness.industryCannabinoidsSolid Phase Extraction010401 analytical chemistryExtraction (chemistry)General MedicineFood safety0104 chemical sciencesMilkLiverSeedsbusinessDecision limitChromatography LiquidFood ScienceFood of animal origin
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The dyon charge in noncommutative gauge theories

2007

We present an explicit classical dyon solution for the noncommutative version of the Yang-Mills-Higgs model (in the Prasad-Sommerfield limit) with a tehta term. We show that the relation between classical electric and magnetic charges also holds in noncommutative space. Extending the Noether approach to the case of a noncommutative gauge theory, we analyze the effect of CP violation at the quantum level, induced both by the theta term and by noncommutativity and we prove that the Witten effect formula for the dyon charge remains the same as in ordinary space.

High Energy Physics - TheoryComputer Science::Machine LearningCiencias FísicasGeneral Physics and AstronomyFOS: Physical sciencesSpace (mathematics)Computer Science::Digital LibrariesStatistics::Machine Learningsymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryMathematics::Quantum AlgebraGauge theoryLimit (mathematics)Ciencias ExactasMathematical physicsPhysicsnoncommutative gauge theoryMathematics::Operator AlgebrasHigh Energy Physics::PhenomenologyFísicaCharge (physics)Noncommutative geometryDyonHigh Energy Physics - Theory (hep-th)Computer Science::Mathematical SoftwaresymbolsCP violationNoether's theorem
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Implications for dark matter direct detection in the presence of LIGO-motivated primordial black holes

2019

We discuss formation of dark matter (DM) mini-halos around primordial black holes (PBHs) and its implication on DM direct detection experiments, including axion searches. Motivated by LIGO observations, we consider $f_{\textrm{DM}} \simeq 0.01$ as the fraction of DM in PBHs with masses $10 M_{\odot} - 70 M_{\odot}$. In this case, we expect the presence of dressed PBHs after Milky Way halo formation with mini-halo masses peaked around $M_{\textrm{halo}} \sim (50-55) M_{\textrm{PBH}}$. We analyze the effect of tidal forces acting on dressed PBHs within the Milky Way galaxy. In the solar neighborhood, the mini-halos are resistant against tidal disruption from the mean-field potential of the ga…

High Energy Physics - TheoryDISRUPTIONHALO MODELSPrimordial black holeAstrophysicsDark mini-halosdark matter direct detectionkosmologia01 natural sciencesGeneral Relativity and Quantum CosmologyLIMITSHigh Energy Physics - Phenomenology (hep-ph)BulgePhysicsprimordial black holeslcsh:QC1-999High Energy Physics - PhenomenologyBULGEMILKY-WAYLIGO-Virgo collaborationHaloAstrophysics - Cosmology and Nongalactic Astrophysicsaxion dark matterNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Axion dark matterMilky WayDark mattermustat aukotFOS: Physical sciencesPrimordial black holesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsDark matter direct detection114 Physical sciencespimeä ainedark mini-halos0103 physical sciences010306 general physicsAxionCP CONSERVATIONAstrophysics::Galaxy Astrophysics010308 nuclear & particles physicsCONSTRAINTSAstrophysics - Astrophysics of GalaxiesLIGOGalaxyHigh Energy Physics - Theory (hep-th)Astrophysics of Galaxies (astro-ph.GA)lcsh:Physics
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Constraints on Cosmic Strings Using Data from the Third Advanced LIGO–Virgo Observing Run

2021

We search for gravitational-wave signals produced by cosmic strings in the Advanced LIGO and Virgo full O3 data set. Search results are presented for gravitational waves produced by cosmic string loop features such as cusps, kinks and, for the first time, kink-kink collisions.cA template-based search for short-duration transient signals does not yield a detection. We also use the stochastic gravitational-wave background energy density upper limits derived from the O3 data to constrain the cosmic string tension, $G\mu$, as a function of the number of kinks, or the number of cusps, for two cosmic string loop distribution models.cAdditionally, we develop and test a third model which interpolat…

High Energy Physics - TheoryDewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftengravitational radiation: stochasticAstronomyCosmic stringsWAVESGeneral Physics and Astronomy01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologyGravitation Cosmology & AstrophysicsGravitationLIMITSCosmic strings & domain wallCosmology & Astrophysicsddc:550Distribution modelsTransient signalenergy: densityLIGOQCstochastic modelLIGO Scientific CollaborationShort durationsCosmic strings & domain walls; Gravitational waves; Gravitation Cosmology & AstrophysicsQBPhysicsCosmic strings & domain wallskinkSettore FIS/03Stochastic systems[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thPhysicsGravitational effectsarticleGRAVITATIONAL-RADIATION; LIMITS; EVOLUTION; WAVEStensionGravitational-wave signalsCosmologyPhysical Sciencesastro-ph.COGrand unified theories[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational waveAstrophysics - Cosmology and Nongalactic AstrophysicsGravitational effects; Gravity waves; Stochastic models; Stochastic systems; Cosmic strings; Distribution models; Grand unified theories; Gravitational-wave signals; Orders of magnitude; Short durations; Template-based; Transient signalGravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)gr-qcPhysics MultidisciplinaryGRAVITATIONAL-RADIATIONO3FOS: Physical sciencesContext (language use)General Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsPhysics and Astronomy(all)Gravity wavesGravitation and AstrophysicsGravitational wavesTheoretical physicsGeneral Relativity and Quantum Cosmologystatistical analysis0103 physical sciencesTemplate-basedCosmic Strings O3 LIGO Virgoddc:530010306 general physicscosmic stringSTFCInflation (cosmology)Science & Technology010308 nuclear & particles physicsGravitational wavestring tensionVirgogravitational radiation: backgroundRCUKLIGOEVOLUTIONCosmic stringStochastic modelsOrders of magnitudeVIRGOHigh Energy Physics - Theory (hep-th)Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Stellar structure models in modified theories of gravity: Lessons and challenges

2019

The understanding of stellar structure represents the crossroads of our theories of the nuclear force and the gravitational interaction under the most extreme conditions observably accessible. It provides a powerful probe of the strong field regime of General Relativity, and opens fruitful avenues for the exploration of new gravitational physics. The latter can be captured via modified theories of gravity, which modify the Einstein-Hilbert action of General Relativity and/or some of its principles. These theories typically change the stellar structure equations, thus having a large impact on the astrophysical properties of the corresponding stars and opening a new window to constrain these …

High Energy Physics - TheoryFísica-Modelos matemáticosGeneral relativityFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsStellar classification01 natural sciencesGeneral Relativity and Quantum CosmologyGravitation0103 physical sciencesFísica matemáticaAstrophysics::Solar and Stellar AstrophysicsStellar structure010306 general physicsChandrasekhar limitSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsWhite dwarfStarsNeutron starHigh Energy Physics - Theory (hep-th)Astrophysics - Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsPhysics Reports
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Double collinear splitting amplitudes at next-to-leading order

2013

We compute the next-to-leading order (NLO) QCD corrections to the $1 \to 2$ splitting amplitudes in different dimensional regularization (DREG) schemes. Besides recovering previously known results, we explore new DREG schemes and analyze their consistency by comparing the divergent structure with the expected behavior predicted by Catani's formula. Through the introduction of scalar-gluons, we show the relation among splittings matrices computed using different schemes. Also, we extended this analysis to cover the double collinear limit of scattering amplitudes in the context of QCD+QED.

High Energy Physics - TheoryNLO COMPUTATIONSNuclear and High Energy PhysicsParticle physicsHADRONIC COLLIDERSCiencias FísicasFOS: Physical sciencesContext (language use)01 natural sciences//purl.org/becyt/ford/1 [https]Dimensional regularizationHigh Energy Physics - Phenomenology (hep-ph)Consistency (statistics)0103 physical sciencesLimit (mathematics)010306 general physicsMathematical physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísica//purl.org/becyt/ford/1.3 [https]Scattering amplitudeAstronomíaHigh Energy Physics - PhenomenologyAmplitudeHigh Energy Physics - Theory (hep-th)Cover (topology)CIENCIAS NATURALES Y EXACTASJournal of High Energy Physics
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High-energy evolution to three loops

2018

The Balitsky-Kovchegov equation describes the high-energy growth of gauge theory scattering amplitudes as well as nonlinear saturation effects which stop it. We obtain the three-loop corrections to this equation in planar $\mathcal{N}=4$ super Yang-Mills theory. Our method exploits a recently established equivalence with the physics of soft wide-angle radiation, so-called non-global logarithms, and thus yields at the same time the three-loop evolution equation for non-global logarithms. As a by-product of our analysis, we develop a Lorentz-covariant method to subtract infrared and collinear divergences in cross-section calculations in the planar limit. We compare our result in the linear re…

High Energy Physics - TheoryNuclear and High Energy PhysicsDifferential equationFOS: Physical sciencesYang–Mills theory01 natural sciences114 Physical sciencesperturbative QCDSupersymmetric Gauge TheoryPomeronHARMONIC POLYLOGARITHMSHigh Energy Physics - Phenomenology (hep-ph)supersymmetriaPerturbative QCD0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityGauge theoryLimit (mathematics)Scattering Amplitudes010306 general physicsQCD AMPLITUDESsupersymmetric gauge theoryMathematical physicsPhysicsPOMERONta114010308 nuclear & particles physicsMASS SINGULARITIESPerturbative QCDDIFFERENTIAL-EQUATIONSscattering amplitudesScattering amplitudeHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Supersymmetric gauge theoryresummationYANG-MILLS THEORYlcsh:QC770-798ResummationkvanttikenttäteoriaTO-LEADING ORDERGAUGE-THEORYAPPROXIMATIONJournal of High Energy Physics
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Optimal estimation of losses at the ultimate quantum limit with non-Gaussian states

2009

We address the estimation of the loss parameter of a bosonic channel probed by arbitrary signals. Unlike the optimal Gaussian probes, which can attain the ultimate bound on precision asymptotically either for very small or very large losses, we prove that Fock states at any fixed photon number saturate the bound unconditionally for any value of the loss. In the relevant regime of low-energy probes, we demonstrate that superpositions of the first low-lying Fock states yield an absolute improvement over any Gaussian probe. Such few-photon states can be recast quite generally as truncations of de-Gaussified photon-subtracted states.

High Energy Physics - TheoryPhotonPHOTON NUMBER STATES DETERMINISTIC GENERATION CIRCUIT CAVITY FIELDGaussianFOS: Physical sciencesValue (computer science)Fock spacePHOTON NUMBER STATESsymbols.namesakeQuantum mechanicsFIELDQuantum information scienceMathematical PhysicsPhysicsDETERMINISTIC GENERATIONQuantum PhysicsOptimal estimationPHOTON NUMBER STATES; DETERMINISTIC GENERATION; CIRCUIT; CAVITY; FIELDQuantum limitCIRCUITMathematical Physics (math-ph)Atomic and Molecular Physics and OpticsCondensed Matter - Other Condensed MatterHigh Energy Physics - Theory (hep-th)CAVITYsymbolsQuantum Physics (quant-ph)Other Condensed Matter (cond-mat.other)Optics (physics.optics)Communication channelPhysics - Optics
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Apparent universality of semiclassical gravity in the far field limit

2006

The universality of semiclassical gravity is investigated by considering the behavior of the quantities < ��^2 > and < {T^a}_b >, along with quantum corrections to the effective Newtonian potential in the far field limits of static spherically symmetric objects ranging from stars in the weak field Newtonian limit to black holes. For scalar fields it is shown that when differences occur they all result from the behavior of a single mode with zero frequency and angular momentum and are thus due to a combination of infrared and s-wave effects. An intriguing combination of similarities and differences between the extreme cases of a Schwarzschild black hole and a star in the weak fie…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsAngular momentumQuantum field theory in curved spacetimeNewtonian potentialFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Newtonian limitGeneral Relativity and Quantum CosmologyGravitationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum mechanicsSchwarzschild metricSemiclassical gravityQuantum field theory
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