Search results for "binary [neutron star]"

showing 10 items of 544 documents

Epistemic, interpersonal, and moral stances in the construction of us and them in Christian metal lyrics

2011

Abstract Religious groupings and subcultures both tend to have well-articulated interests, aims, and values that unite certain people but also alienate those who do not share their interests. The case is then made for the construction of difference between ‘us’ and ‘them’. This paper examines the construction of such a group boundary in the previously little studied context of the Christian metal (CM) music subculture. The focus of analysis is on the kinds of stances that are taken and attributed to ‘us’ and ‘them’ in the English lyrics of Finnish CM groups. The particular types of stance are related to questions of epistemology, interpersonality, and morality. The paper shows that the bord…

Cultural StudiesLinguistics and LanguageBinary oppositionCommunicationmedia_common.quotation_subjectta6122Context (language use)ta6121MoralityLyricsWorshipObject (philosophy)EpistemologyDivinityHeavenSociologymedia_commonJournal of Multicultural Discourses
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Phase Behavior of Active Swimmers in Depletants: Molecular Dynamics and Integral Equation Theory

2013

We study the structure and phase behavior of a binary mixture where one of the components is self-propelling in nature. The inter-particle interactions in the system were taken from the Asakura-Oosawa model, for colloid-polymer mixtures, for which the phase diagram is known. In the current model version the colloid particles were made active using the Vicsek model for self-propelling particles. The resultant active system was studied by molecular dynamics methods and integral equation theory. Both methods produce results consistent with each other and demonstrate that the Vicsek model based activity facilitates phase separation, thus broadening the coexistence region.

Current (mathematics)PolymersMovementFOS: Physical sciencesGeneral Physics and AstronomyBinary numberCondensed Matter - Soft Condensed MatterMolecular Dynamics SimulationModels BiologicalDiffusionMolecular dynamicsColloidPhase (matter)ColloidsStatistical physicsCondensed Matter - Statistical MechanicsPhase diagramPhysicsStatistical Mechanics (cond-mat.stat-mech)Active systemsModels TheoreticalIntegral equationCondensed Matter::Soft Condensed MatterKineticsClassical mechanicsModels ChemicalSoft Condensed Matter (cond-mat.soft)Physical Review Letters
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Residual Stresses Induced by Cold Expansion of Adjacent and Cut-Out Holes

2012

Fatigue life of fastener holes can be enhanced via a cold-expansion process to introduce a compressive residual stress field around the hole edge and to reduce crack growth propagation. Considering that aerospace components contain multiple rows of holes, the present investigation focuses on the evaluation of the three-dimensional residual stress distribution in adjacent cold-expanded (CE) holes. The redistribution of residual stresses caused by a cut introduced between two adjacent holes was also investigated. Finite element (FE) analysis and experimental technique were used to assess the residual stress distribution in a 6082-T6 aluminum plate with two adjacent holes expanded sequentially…

Cut-out holebusiness.product_categoryMaterials scienceMechanical EngineeringSettore ING-IND/34 - Bioingegneria IndustrialeCold-expansion of holesAerospace Engineeringchemistry.chemical_elementEdge (geometry)Binary encoded light stripe projectionFastenerFinite element methodFatigue crack propagationFinite elementchemistryMechanics of MaterialsResidual stressAluminiumSolid mechanicsForensic engineeringCold-expansion of holeCut-out holesComposite materialbusinessExperimental Mechanics
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Facial geometry and speech analysis for depression detection.

2017

Depression is one of the most prevalent mental disorders, burdening many people world-wide. A system with the potential of serving as a decision support system is proposed, based on novel features extracted from facial expression geometry and speech, by interpreting non-verbal manifestations of depression. The proposed system has been tested both in gender independent and gender based modes, and with different fusion methods. The algorithms were evaluated for several combinations of parameters and classification schemes, on the dataset provided by the Audio/Visual Emotion Challenge of 2013 and 2014. The proposed framework achieved a precision of 94.8% for detecting persons achieving high sc…

Decision support systemFacial expressionDepressive DisorderDepressionSpeech recognition05 social sciencesNearest neighbourClassification scheme02 engineering and technologyFacial geometryBinary operationFace0502 economics and business0202 electrical engineering electronic engineering information engineeringDecision fusionHumansSpeech020201 artificial intelligence & image processingPsychologyClassifier (UML)050203 business & managementAlgorithmsAnnual International Conference of the IEEE Engineering in Medicine and Biology Society. IEEE Engineering in Medicine and Biology Society. Annual International Conference
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GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences

2018

The LIGO Scientific and Virgo Collaborations have announced the first detection of gravitational waves from the coalescence of two neutron stars. The merger rate of binary neutron stars estimated from this event suggests that distant, unresolvable binary neutron stars create a significant astrophysical stochastic gravitational-wave background. The binary neutron star background will add to the background from binary black holes, increasing the amplitude of the total astrophysical background relative to previous expectations. In the Advanced LIGO-Virgo frequency band most sensitive to stochastic backgrounds (near 25 Hz), we predict a total astrophysical background with amplitude $\Omega_{\rm…

Design sensitivityneutron star: binarygravitational radiation: stochasticAstronomyX-ray binaryGeneral Physics and AstronomyAstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologylocalizationGravitational wave backgroundGravitational Waves Neutron Stars Stochastic Background Virgo LIGOblack holeLIGOstochastic modelQCQBPhysicsGAMMA-RAY BURSTSSignal to noise ratioStochastic systemsBlack holesGravitational effectsarticleAstrophysics::Instrumentation and Methods for AstrophysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSING[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sources Experimental studies of gravity Gravitational WavesGravitationBinary neutron starsX-ray bursterBinsAstrophysics::High Energy Astrophysical PhenomenaMERGERSFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesgravitational radiation: direct detectionBinary pulsarNeutron starsSTAR-FORMATIONPhysics and Astronomy (all)General Relativity and Quantum CosmologyBinary black holebinary: coalescence0103 physical sciencesFrequency bandsddc:530RATESINTERFEROMETERS010306 general physicsAstrophysics::Galaxy AstrophysicsNeutronsGravitational Waves010308 nuclear & particles physicsGravitational waveVirgogravitational radiation: backgroundgravitational radiationAstronomyNeutron Stars530 Physikbinary: compactsensitivityStarsLIGObackground: stochasticEVOLUTIONsignal noise ratioVIRGOPhysics and Astronomyblack hole: binarygravitational radiation: emissionStellar black holeStochastic BackgroundDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikHIGH-REDSHIFTneutron star: coalescencePhysical Review Letters
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Search for Subsolar-Mass Ultracompact Binaries in Advanced LIGO's First Observing Run

2018

We present the first Advanced LIGO and Advanced Virgo search for ultracompact binary systems with component masses between 0.2 $M_\odot$ - 1.0 $M_\odot$ using data taken between September 12, 2015 and January 19, 2016. We find no viable gravitational wave candidates. Our null result constrains the coalescence rate of monochromatic (delta function) distributions of non-spinning (0.2 $M_\odot$, 0.2 $M_\odot$) ultracompact binaries to be less than $1.0 \times 10^6 \text{Gpc}^{-3} \text{yr}^{-1}$ and the coalescence rate of a similar distribution of (1.0 $M_\odot$, 1.0 $M_\odot$) ultracompact binaries to be less than $1.9 \times 10^4 \text{Gpc}^{-3} \text{yr}^{-1}$ (at 90 percent confidence). N…

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftendensity: fluctuationMACHOAstronomyGeneral Physics and AstronomyPrimordial black holeAstrophysicsCoalescence01 natural sciencesGeneral Relativity and Quantum CosmologylocalizationLIMITSddc:550Massive compact halo objectLIGOneutron starQCQBPhysicseducation.field_of_studyPhysicsDensity fluctuationBinary systemsgravitational wavesPhysical SciencesSearch enginesastro-ph.COblack hole: primordialAstrophysics - Cosmology and Nongalactic AstrophysicsGravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)gr-qcBinary formationAstrophysics::High Energy Astrophysical PhenomenaPopulationDark matterPhysics MultidisciplinaryEarly universeFOS: Physical sciencesPrimordial black holesGeneral Relativity and Quantum Cosmology (gr-qc)dark matter: densityAstrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesCoalescence rateGravitation and AstrophysicsPhysics and Astronomy (all)General Relativity and Quantum Cosmologybinary: coalescence0103 physical sciencesddc:530Delta functions010306 general physicseducationSTFCAstrophysics::Galaxy AstrophysicsScience & Technologymass: solar010308 nuclear & particles physicsGravitational waveStellar evolutionsbinary: formationgravitational radiationRCUKblack hole: massGalaxiesStarsGalaxyLIGOBlack holeVIRGOPhysics and Astronomyblack hole: binarygravitational radiation: emissionDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikMicro-lensing[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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GW170817: Measurements of Neutron Star Radii and Equation of State

2018

On 17 August 2017, the LIGO and Virgo observatories made the first direct detection of gravitational waves from the coalescence of a neutron star binary system. The detection of this gravitational-wave signal, GW170817, offers a novel opportunity to directly probe the properties of matter at the extreme conditions found in the interior of these stars. The initial, minimal-assumption analysis of the LIGO and Virgo data placed constraints on the tidal effects of the coalescing bodies, which were then translated to constraints on neutron star radii. Here, we expand upon previous analyses by working under the hypothesis that both bodies were neutron stars that are described by the same equation…

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftenneutron star: binaryAstronomyGeneral Physics and AstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGRAVITATIONAL-WAVESGW170817BINARIESddc:550DENSELIGODENSE MATTEREquation of State010303 astronomy & astrophysicsQCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysicsNeutron Star RadiusPhysicsGravitational effectsEquations of stateParametrizationsElectromagnetic observationsGravitational-wave signals3. Good healthQUADRUPOLE-MOMENTSMacroscopic propertiesPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sourceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaEquations of state of nuclear matterGravitational wavesaturation: densityBinary neutron starsNUCLEON MATTEREquations of state of nuclear matter; Gravitational wave sources; Gravitational waves; Nuclear matter in neutron starsGeneral relativitygr-qcAstrophysics::High Energy Astrophysical PhenomenaGW170817 Neutron Star Radius Equation of StatePhysics Multidisciplinaryneutron star: spinFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesgravitational radiation: direct detectionGravitation and AstrophysicsNuclear matter in neutron starsGravitational waveselectromagnetic field: productionPhysics and Astronomy (all)Pulsargalaxy: binary0103 physical sciencesddc:530NeutronMASSESSTFCequation of state: parametrizationAstrophysics::Galaxy AstrophysicsNeutronsExtreme conditionsGravitational wave sourcesEquation of stateScience & TechnologyNeutron Star Interior Composition Explorer010308 nuclear & particles physicsGravitational wavegravitational radiationRCUKFlocculationSaturation densityUNIVERSAL RELATIONSStarsLIGOgravitational radiation detectorNeutron starStarsVIRGOPhysics and Astronomygravitational radiation: emissionneutron star: binary: coalescenceDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]MATTER
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Tests of General Relativity with GW170817

2019

The recent discovery by Advanced LIGO and Advanced Virgo of a gravitational wave signal from a binary neutron star inspiral has enabled tests of general relativity (GR) with this new type of source. This source, for the first time, permits tests of strong-field dynamics of compact binaries in presence of matter. In this paper, we place constraints on the dipole radiation and possible deviations from GR in the post-Newtonian coefficients that govern the inspiral regime. Bounds on modified dispersion of gravitational waves are obtained; in combination with information from the observed electromagnetic counterpart we can also constrain effects due to large extra dimensions. Finally, the polari…

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftenneutron star: binaryAstronomyTestingGravitational WaveGeneral Physics and AstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmologystrong fieldddc:550general relativityLIGOQCSettore FIS/01PhysicsPhysicsGravitational effectsarticlePolarization (waves)Gravitational-wave signalsExtra dimensionsgravitational wavesPhysical SciencesExtra dimensions[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Large extra dimensiondispersionBinary neutron starsgravitational radiation: polarizationGeneral RelativityGeneral relativitygr-qcPhysics MultidisciplinaryGRAVITATIONAL-WAVE OBSERVATIONSFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)gravitational wavesblack holesGravity wavesMASSgravitational radiation: direct detectionGravitation and Astrophysicselectromagnetic field: productionRelativityGeneral Relativity and Quantum CosmologyDipole radiationsGRAVITYTests of general relativitygravitation: weak field0103 physical sciencesddc:530High Energy Physicscapture010306 general physicsGravitational Wave; General RelativitySTFCradiation: dipolepolarizationScience & TechnologyStrong fieldGravitational wavegravitational radiationRCUKbinary: compactgravitational radiation detectorLIGONeutron starVIRGODewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikNewtonianshigher-dimensional
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Phase equilibria and multiple azeotropy in the associating system methanol + diethylamine

1997

Vapor−liquid equilibrium has been measured for the binary system of methanol (1) + diethylamine (2) at 101.3 and 300 kPa. Both equilibrium isobars show strong deviations from ideal behavior and a single maximum boiling point azeotrope of practically constant composition x1 ≈ 0.76, corresponding to a temperature of 339.8 K at 101.3 kPa and 370.0 K at 300 kPa. The trend of the high-pressure isobar data is consistent with the formation of a second minimum boiling azeotrope, confirming the multiple azeotropic behavior found by others at a higher temperature (398.58 K). Furthermore, the excess Gibbs energy is negative and inflects markedly with composition with increased pressure. The equilibriu…

DiethylamineUNIQUACGeneral Chemical EngineeringThermodynamicsGeneral ChemistryGibbs free energychemistry.chemical_compoundBoiling pointsymbols.namesakechemistryAzeotropeBoilingIsobarsymbolsBinary system
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3D printed diffractive terahertz lenses

2016

[EN] A 3D printer was used to realize custom-made diffractive THz lenses. After testing several materials, phase binary lenses with periodic and aperiodic radial profiles were designed and constructed in polyamide material to work at 0.625 THz. The nonconventional focusing properties of such lenses were assessed by computing and measuring their axial point spread function (PSF). Our results demonstrate that inexpensive 3D printed THz diffractive lenses can be reliably used in focusing and imaging THz systems. Diffractive THz lenses with unprecedented features, such as extended depth of focus or bifocalization, have been demonstrated.

DiffractionPoint spread function3d printedMaterials scienceTerahertz radiationPhase (waves)Diffractive lensesBinary optics02 engineering and technologyDiffraction efficiency01 natural sciences010309 opticsDiffractive lensOpticsImage quality assessment0103 physical sciencesDiffractive opticsExtended depth of focusbusiness.industry021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsTerahertz imagingFISICA APLICADAOptical fabrication0210 nano-technologybusiness
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