Search results for "Wave"

showing 10 items of 6009 documents

Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO-Virgo Run O3a

2022

Abbott, R., et al. (LIGO and VIRGO Collaboration)

neutron star: binaryGravitational waves(678)ELECTROMAGNETIC COUNTERPARTSBinary numberAstrophysics01 natural sciencesLIGOHigh-Energy Phenomena and Fundamental PhysicsQCSUPERNOVAQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01education.field_of_study[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Black holesSettore FIS/0506 humanities and the artsGRBEnergy InjectionSearch for gravitational wave transients associated to GRBs - Fermi and Swift satellitesAFTERGLOWPhysical SciencesRELATIVISTIC JETSAstrophysics - High Energy Astrophysical PhenomenaSwiftGravitational waveBlack-Hole330Evolutiongr-qcGamma Ray Burst LIGO Virgo Gravitational WavesAstrophysics::High Energy Astrophysical PhenomenaGeneral Relativity and Quantum Cosmology (gr-qc)0603 philosophy ethics and religionGravitational-wave astronomyNeutron starsENERGY INJECTIONCORE-COLLAPSEeducationGamma-ray burstScience & TechnologyCore-CollapseVirgoRCUKAstronomy and AstrophysicstriggerLuminosity FunctionDewey Decimal Classification::500 | Naturwissenschaften::520 | Astronomie KartographieGamma Ray BurstSpace and Planetary ScienceBLACK-HOLEddc:520gravitational wave astronomyGravitational wave astronomyGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]LIGO(920)Fermi Gamma-ray Space TelescopeAstronomyAstrophysicsGeneral Relativity and Quantum Cosmologyneutron starsENERGYGravitational wave detectorsGamma-ray bursts(629)Neutron Stars Mergers Gravitational Waves010303 astronomy & astrophysicsgravitational waves; gamma ray bursts; LIGO; Virgo; Fermi; SwiftCompact binary stars(283)astro-ph.HEPhysicscompact binary starsgamma-ray burstsgamma-ray bursts ; gravitational waves; LIGO; Virgogravitational waves060302 philosophy[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]PRECURSOR ACTIVITYGravitational wave astronomy(675)Gamma-ray burstsGW_HIGHLIGHT[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PopulationCompact binary starssatelliteFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & Astrophysicsgamma ray: burstMASS1STGLASTGamma-ray bursts; Gravitational wave astronomy; Gravitational waves; Gravitational wave detectors0103 physical sciencesSTFCFermigravitational waves; gamma-ray bursts; LIGO; Virgo; Fermi; SwiftGravitational wavegravitational radiationgamma ray burstsgamma-ray burts--black holesLIGOEVOLUTIONOBSERVING RUNNeutron stars(1108)Neutron starPhysics and Astronomy[SDU]Sciences of the Universe [physics]LUMINOSITY FUNCTIONBlack holes(162)INJECTIONEMISSION
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The advanced Virgo longitudinal control system for the O2 observing run

2020

Following a successful period of data-taking between 2006 and 2011, the Virgo gravitational-wave detector was taken offline for a major upgrade. The changes made to the instrument significantly increased the complexity of the control systems and meant that an extended period of commissioning was required to reach a sensitivity appropriate for science data-taking. This commissioning period was completed in July of 2017 and the second-generation Advanced Virgo detector went on to join the Advanced LIGO detectors in the O2 science run in August of the same year. The upgraded detector was approximately twice as sensitive to binary neutron star mergers as the first-generation instrument. During …

neutron star: binaryPhysics::Instrumentation and DetectorsAstronomycavity: opticalSuspended optical cavities01 natural sciencesGravitational wave detectorsoff-lineGravitational wave detectors; Interferometer; Suspended optical cavities; Control loopsControl loopSuspended optical cavitieLIGOInterferometer010303 astronomy & astrophysicsdetectorsSettore FIS/01Physics[PHYS]Physics [physics]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsGravitational wave detectors Interferometer Suspended optical cavities Control loopsGravitational wave detectorUpgrade[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]upgradecontrol systemGravitational wavelongitudinalAstrophysics::High Energy Astrophysical PhenomenainterferometerAstrophysics::Cosmology and Extragalactic Astrophysicscontrol loops; gravitational wave detectors; interferometer; suspended optical cavitiesgravitational radiation: direct detectionGeneral Relativity and Quantum CosmologySettore FIS/05 - Astronomia e AstrofisicaBinary black holebinary: coalescence0103 physical sciencesControl loops[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010308 nuclear & particles physicsGravitational wavegravitational radiationAstronomyAstronomy and AstrophysicssensitivityLIGOgravitational radiation detectordetector: sensitivityNeutron star* Automatic Keywords *VIRGOblack hole: binaryControl systemgravitational radiation: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

2017

On August 17, 2017 at 12-41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per 8.0×104 years. We infer the component masses of the binary to be between 0.86 and 2.26 M, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60 M, with the total mass of the system 2.74-0.01+0.04M. The source was localized within a sky region of 28 deg2 (90% probabili…

neutron star: binary[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]X-ray binaryADVANCED LIGOAstrophysicsKilonovagravitational waves; LIGO; binary neutron star inspiralspin01 natural sciencesLIGOGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Electromagnetic observationsGravitational-wave signals3100 General Physics and AstronomyPoint MassesAstrophysics - High Energy Astrophysical PhenomenaBlack-Hole MergersBinary neutron starsBlack HolesX-ray bursterCoalescing BinariesAstrophysics::High Energy Astrophysical Phenomena10192 Physics InstituteGeneral Relativity and Quantum Cosmology (gr-qc)Gravity wavesGravitational wavesNeutron starsPhysics and Astronomy (all)ddc:530Electromagnetic spectraNeutrons010308 nuclear & particles physicsVirgoGamma raysAstronomyRCUKVIRGOelectromagneticgravitational radiation: emissionStellar black holeGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Compact Binariesbinary: masscosmological modelAstronomyGeneral Physics and AstronomyAstrophysicsneutron starsGamma ray burstsGeneral Relativity and Quantum CosmologyGravitational wave detectorsUniverseDENSE MATTER010303 astronomy & astrophysicsastro-ph.HEPhysicsSignal to noise ratioSettore FIS/01 - Fisica SperimentaleGravitational effectsFalse alarm rateEQUATION-OF-STATEMergers and acquisitionsgravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]530 PhysicsMERGERSGeneral Relativity and Quantum Cosmology; General Relativity and Quantum Cosmology; astro-ph.HEFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstgravitational radiation: direct detectionMerging[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]GAMMA-RAY BURSTLIGO (Observatory)binary: coalescenceGravitational waves neutron stars gamma-ray burst LIGO Virgo0103 physical sciencesGW151226MASSESSTFCAstrophysics::Galaxy AstrophysicsPhysiqueGravitational wavegravitational radiationPULSARgravitational radiation detectorNeutron starPhysics and AstronomygravitationRADIATIONDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikbinary neutron star inspiralSignal detectionPHYS REV LETT PHYSICAL REVIEW LETTERS
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Zinātniskās fantastikas ilustrāciju vizuālā stilistika

2015

Diplomdarbā tika pētītas zinātniskās fantastikas ilustrācijas, to attīstības vēsture un vizuālā stilistika. Darba teorētiskajā daļā tika noskaidrots zinātniskās fantastikas jēdziens un tā vēsturiskā izcelšanās un pazīmes, kas norāda piederību šim žanram. Tika apskatīti tādi zinātniskās fantastikas apakšžanri kā: space opera, new wave, cyberpunk un steampunk. Kā arī tiem piemītošās stilistiskās īpatnības. Attiecīgi katram attīstības posmam apzināti tā perioda ilustratori. Darba empīriskajā daļā tika apzinātas un analizētas zinātniskās fantastikas ilustrācijas, sagrupējot tās pa četriem laika periodiem. Tika apskatītas ilustrācijas līdz 19.gs., tad atsevišķi izdalot 19.gs. un 20.gs ilustrācij…

new waveMākslas zinātnespace operazinātniskā fantastikailustrācijacyberpunk
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Quantum Motion of Chemisorbed Hydrogen on Ni Surfaces

1983

Quantum mechanical energy levels and wave functions have been calculated for the motion of chemisorbed hydrogen atoms on Ni surfaces. The results show considerable quantum effects for the adatom in both the ground and the excited states. The description of the adparticles as being delocalized along the surface offers a novel interpretation of several phenomena, in particular the vibrational excitations. Peer reviewed

nickel surfacesMaterials scienceSolid-state physicsHydrogenwave functionsGeneral Physics and Astronomychemistry.chemical_element02 engineering and technology01 natural sciencesCondensed Matter::Materials ScienceDelocalized electron0103 physical sciencesPhysics::Atomic and Molecular Clustersenergy levels010306 general physicsWave functionQuantumMechanical energyPhysicshydrogen atoms021001 nanoscience & nanotechnologychemistryChemisorptionExcited stateAtomic physics0210 nano-technologyPhysical Review Letters
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Noiseless Quantum Measurement and Squeezing of Microwave Fields Utilizing Mechanical Vibrations

2017

A process which strongly amplifies both quadrature amplitudes of an oscillatory signal necessarily adds noise. Alternatively, if the information in one quadrature is lost in phase-sensitive amplification, it is possible to completely reconstruct the other quadrature. Here we demonstrate such a nearly perfect phase-sensitive measurement using a cavity optomechanical scheme, characterized by an extremely small noise less than 0.2 quanta. We also observe microwave radiation strongly squeezed by 8 dB below vacuum. A source of bright squeezed microwaves opens up applications in manipulations of quantum systems, and noiseless amplification can be used even at modest cryogenic temperatures.

noiseFOS: Physical sciencesGeneral Physics and AstronomyQuantum measurement02 engineering and technology01 natural sciencesOpticsMesoscale and Nanoscale Physics (cond-mat.mes-hall)0103 physical sciences010306 general physicsQuantumPhysicsQuantum PhysicsCondensed Matter - Mesoscale and Nanoscale Physicsta114business.industrymittausnoiseless amplifications021001 nanoscience & nanotechnologymeluQuadrature (astronomy)VibrationAmplitudequantum systemsmeasurementQuantum Physics (quant-ph)0210 nano-technologybusinesscryogenic temperaturesMicrowave
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Inference of proto-neutron star properties from gravitational-wave data in core-collapse supernovae

2021

The eventual detection of gravitational waves from core-collapse supernovae (CCSN) will help improve our current understanding of the explosion mechanism of massive stars. The stochastic nature of the late post-bounce gravitational wave signal due to the non-linear dynamics of the matter involved and the large number of degrees of freedom of the phenomenon make the source parameter inference problem very challenging. In this paper we take a step towards that goal and present a parameter estimation approach which is based on the gravitational waves associated with oscillations of proto-neutron stars (PNS). Numerical simulations of CCSN have shown that buoyancy-driven g-modes are responsible …

noiseGravitational-wave observatorygravitational radiation: stochasticAstrophysics::High Energy Astrophysical Phenomenaprotoneutron starDegrees of freedom (physics and chemistry)FOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciences7. Clean energyGeneral Relativity and Quantum CosmologyEinstein Telescopeeffect: nonlinearsupernova0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]LIGOnumerical calculations010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)equation of statePhysicsSolar massmass: solarEinstein Telescope010308 nuclear & particles physicsGravitational wavegravitational radiationoscillationgravitational radiation detectorLIGOgravitation: collapsedetector: sensitivitystar: massiveSupernovaStarswave: modelVIRGO13. Climate actiongravitational radiation: emission[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]galaxyAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics and astroparticle physics
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Electroencephalography as a Non-Invasive Biomarker of Alzheimer’s Disease: A Forgotten Candidate to Substitute CSF Molecules?

2021

Biomarkers for disease diagnosis and prognosis are crucial in clinical practice. They should be objective and quantifiable and respond to specific therapeutic interventions. Optimal biomarkers should reflect the underlying process (pathological or not), be reproducible, widely available, and allow measurements repeatedly over time. Ideally, biomarkers should also be non-invasive and cost-effective. This review aims to focus on the usefulness and limitations of electroencephalography (EEG) in the search for Alzheimer’s disease (AD) biomarkers. The main aim of this article is to review the evolution of the most used biomarkers in AD and the need for new peripheral and, ideally, non-invasive b…

non-invasive biomarkerscerebral rhythmsQH301-705.5ReviewDiseaseElectroencephalographyBioinformaticsCatalysisInorganic ChemistryAlzheimer DiseaseAlzheimer’s disease diagnosismedicineAnimalsHumansEEGBiology (General)Physical and Theoretical ChemistryQD1-999Molecular BiologySpectroscopyCerebrospinal Fluidmedicine.diagnostic_testbusiness.industryOrganic ChemistryNon invasive biomarkerssynchronyElectroencephalographyGeneral MedicineComputer Science ApplicationsClinical PracticeChemistrycomplexitybusinessBiomarkersalpha waveInternational Journal of Molecular Sciences
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Liver stiffness quantification in biopsy-proven nonalcoholic fatty liver disease patients using shear wave elastography in comparison with transient …

2021

Purpose: This study prospectively assessed the performance of liver stiffness measurements using point shear-wave elastography (p-SWE) in comparison with transient elastography (TE) in patients with biopsy-proven nonalcoholic fatty liver disease (NAFLD). Methods: Fifty-six consecutive adult patients with a histological diagnosis of NAFLD prospectively underwent TE and p-SWE on the same day. The median of 10 measurements (SWE-10), the first five (SWE-5), and the first three (SWE-3) measurements were analyzed for p-SWE. Liver biopsy was considered as the reference standard for liver fibrosis grade. Receiver operating characteristic (ROC) curves and areas under the ROC curves (AUROCs) were cal…

nonalcoholic fatty liver diseasemedicine.medical_specialtyGastroenterologySettore MED/01 - Statistica Medica030218 nuclear medicine & medical imaging03 medical and health sciences0302 clinical medicineLiver stiffnessInternal medicineStatistical significanceBiopsyNonalcoholic fatty liver diseaseMedical technologymedicineRadiology Nuclear Medicine and imagingnonalcoholic steatohepatitisR855-855.5shear wave elastographymedicine.diagnostic_testReceiver operating characteristicbusiness.industryNonalcoholic fatty liver disease Nonalcoholic steatohepatitis Shear wave elastography Transient elastography Liver stiffnessmedicine.diseasetransient elastographyliver stiffnessLiver biopsyOriginal Article030211 gastroenterology & hepatologyElastographySettore MED/36 - Diagnostica Per Immagini E RadioterapiabusinessTransient elastographyUltrasonography
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Phase-delayed laser diode array allows ultrasonic guided wave mode selection and tuning

2013

Selecting and tuning modes are useful in ultrasonic guided wave non-destructive testing (NDT) since certain modes at various center frequencies are sensitive to specific types of defects. Ideally one should be able to select both the mode and the center frequency of the launched waves. We demonstrated that an affordable laser diode array can selectively launch either the S0 or A0 ultrasonic wave mode at a chosen center frequency into a polymer plate. A fiber-coupled diode array (4 elements) illuminated a 2 mm thick acrylic plate. A predetermined time delay matching the selected mode and frequency was employed between the output of the elements. The generated ultrasound was detected by a 215…

nondestructive testingplates (structures)delayssemiconductor laser arraysacoustic receiversoptical fibre couplersacoustic waveguidesultrasonic wavespolymeeritlaser modeslaser tuning
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