Search results for "waves"

showing 10 items of 1766 documents

VLBA polarimetric monitoring of 3C 111

2018

Context. While studies of large samples of jets of active galactic nuclei (AGN) are important in order to establish a global picture, dedicated single-source studies are an invaluable tool for probing crucial processes within jets on parsec scales. These processes involve in particular the formation and geometry of the jet magnetic field as well as the flow itself. Aims. We aim to better understand the dynamics within relativistic magneto-hydrodynamical flows in the extreme environment and close vicinity of supermassive black holes. Methods. We analyze the peculiar radio galaxy 3C 111, for which long-Term polarimetric observations are available. We make use of the high spatial resolution of…

active [Galaxies]Radio galaxyAstrophysics::High Energy Astrophysical PhenomenaeducationFOS: Physical sciencesAstrophysicsgalaxies [Radio continuum]Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio continuum: galaxiesgalaxies: individual: 3C 111Coincident0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsSupermassive black holepolarizationGalaxies: magnetic fields010308 nuclear & particles physicsmagnetic fields [Galaxies]Astronomy and AstrophysicsGalaxies: activePolarization (waves)Astrophysics - Astrophysics of GalaxiesMonitoring programMagnetic fieldTransverse planeindividual: 3C 111 [galaxies]Space and Planetary ScienceGalaxies: jetsBrightness temperatureAstrophysics of Galaxies (astro-ph.GA)jets [Galaxies]
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Física por un tubo. Mide la velocidad del sonido en el aire y diviértete con los tubos sonoros

2011

En este trabajo damos las claves para disenar un conjunto de tubos sonoros de PVC que permiten realizar una ejecucion musical en grupo con la participacion de un gran numero de personas sin cultura musical previa. Proponemos ademas la utilizacion de los tubos para el estudio cuantitativo de los fenomenos fisicos involucrados en la generacion del sonido con instrumentos de viento. Se describe la utilizacion de los tubos sonoros, en combinacion con un ordenador y un programa de analisis de sonido, para el analisis de ondas estacionarias y la determinacion de la velocidad de propagacion del sonido en el aire mediante distintos procedimientos.Palabras clave: Acustica; Ondas estacionarias; Veloc…

acústicaSocial Sciencesanálisis de fourierondas estacionariasFourier analysisEducationHanálisis de Fouriervelocity of soundrecreational sciencestationary wavesciencia recreativaacousticsvelocidad del sonidoRevista Eureka sobre Enseñanza y Divulgación de las Ciencias
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Searching for signatures around 1920 MeV of a N-* state of three hadron nature

2009

We provide a series of arguments which support the idea that the peak seen in the gamma p -> K+ Lambda reaction around 1920 MeV should correspond to the recently predicted state of J(P) = 1/2(+) as a bound state of K(K) over bar N with a mixture of alpha(0)(980)N and f(0)(980)N components. At the same time we propose polarization experiments in that reaction as a further test of the prediction, as well as a study of the total cross-section for gamma p -> K(+)K(-)p at energies close to threshold and of d sigma/dM(inv) for invariant masses close to the two-kaon threshold.

associated production [K+]Nuclear and High Energy PhysicsParticle physicsNuclear TheoryHadronFOS: Physical sciences01 natural sciencesNuclear Theory (nucl-th)photon p --> Sigma0 K+0103 physical sciencesBound stateddc:530angular distributionbound state [K]010306 general physicstotal cross section(nucleon K anti-K) [bound state]Physicspolarizationhadroproduction [Lambda]intermediate state [f0(980)]photon p --> p K+ K-010308 nuclear & particles physicsFísica(1920) [nucleon resonance]Sigmaintermediate state [a0(980)]Polarization (waves)exclusive reaction [photon p]interpretation of experimentsproposed experimentphoton p --> Lambda K+
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Contribution of observed multi frequency spectrum of Alfvén waves to coronal heating

2019

Context. Whilst there are observational indications that transverse magnetohydrodynamic (MHD) waves carry enough energy to maintain the thermal structure of the solar corona, it is not clear whether such energy can be efficiently and effectively converted into heating. Phase-mixing of Alfvén waves is considered a candidate mechanism, as it can develop transverse gradient where magnetic energy can be converted into thermal energy. However, phase-mixing is a process that crucially depends on the amplitude and period of the transverse oscillations, and only recently have we obtained a complete measurement of the power spectrum for transverse oscillations in the corona. Aims. We aim to investig…

atmosphere [Sun]Magnetohydrodynamics (MHD)corona [Sun]T-NDASContext (language use)Astrophysics01 natural sciences03 medical and health sciences0103 physical sciencesQB AstronomyAstrophysics::Solar and Stellar AstrophysicsQA MathematicsSun: oscillationsQASun: magnetic fields010303 astronomy & astrophysicsQCQB030304 developmental biologyPhysics0303 health sciencesMagnetic energySun: coronaoscillations [Sun]Spectral densityAstronomy and AstrophysicsTransverse waveCoronal loopComputational physicsTransverse planeQC PhysicsAmplitudemagnetic fields [Sun]Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary SciencePhysics::Space PhysicsWavesMagnetohydrodynamicsSun: atmosphereAstronomy & Astrophysics
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Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network

2019

Gravitational wave astronomy has been firmly established with the detection of gravitational waves from the merger of ten stellar mass binary black holes and a neutron star binary. This paper reports on the all-sky search for gravitational waves from intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network. The search uses three independent algorithms: two based on matched filtering of the data with waveform templates of gravitational wave signals from compact binaries, and a third, model-independent algorithm that employs no signal model for the incoming signal. No intermediate mass black hole binary event was detected in this sear…

binary: massneutron star: binaryAstronomybinary: angular momentumAstrophysicsdetector: network01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsLIMITSclustersLIGOgravitational waveGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCQBastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01black hole: spinPhysicsintermediate mass black hole binarieNumerical relativityGeneral relativitygravitational wavesgravitational waves; intermediate mass black hole binaries; Advanced LIGO and VirgoPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenastarsGeneral relativitygr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesalternative theories of gravitySTARS; CLUSTERS; LIMITSAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & Astrophysicsgravitational radiation: direct detectionGeneral Relativity and Quantum CosmologySettore FIS/05 - Astronomia e AstrofisicaBinary black hole0103 physical sciencesddc:530010306 general physicsAstrophysics::Galaxy AstrophysicsSTFCScience & Technology010308 nuclear & particles physicsGravitational waveAdvanced LIGO and Virgointermediate mass black hole binariesRCUKGravitational Wave Physicsblack hole: massMass ratiobinary: compact04.80.NnLIGOgravitational radiation detectorNeutron starVIRGOblack hole: binaryIntermediate-mass black holerelativity theorygravitational radiation: emission95.55.Ymmass ratioDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik07.05.Kflimits[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]CLUSTERSSTARSGravitational waves Black holes (astronomy) Gravitational self force
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All-sky search in early O3 LIGO data for continuous gravitational-wave signals from unknown neutron stars in binary systems

2021

Rapidly spinning neutron stars are promising sources of continuous gravitational waves. Detecting such a signal would allow probing of the physical properties of matter under extreme conditions. A significant fraction of the known pulsar population belongs to binary systems. Searching for unknown neutron stars in binary systems requires specialized algorithms to address unknown orbital frequency modulations. We present a search for continuous gravitational waves emitted by neutron stars in binary systems in early data from the third observing run of the Advanced LIGO and Advanced Virgo detectors using the semicoherent, GPU-accelerated, binaryskyhough pipeline. The search analyzes the most s…

binary: orbitneutron star: binaryPhysics and Astronomy (miscellaneous)Astronomybinary [neutron star]AstrophysicsGravitational Waves; LIGO (Observatory); Neutron Stars01 natural sciencesneutron starsGeneral Relativity and Quantum CosmologyMonte Carlo: Markov chainPhysics Particles & Fieldsbinary starsbinary systemsBinary SystemsLIGOgravitational waveQCQBpulsarastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicseducation.field_of_studySettore FIS/03Physicsorbit [binary]General relativityPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical Phenomenabinary stardata analysis methodsensitivity [detector]General relativitygr-qcfrequency [modulation]Populationneutron star: spinFOS: Physical sciencesalternative theories of gravityMarkov chain [Monte Carlo]General Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsGravitational Waves Neutron Stars Binary Systems LIGO VirgoLIGO (Observatory)emission [gravitational radiation]Pulsarbinary: coalescence0103 physical sciencesBinary starddc:530spin [neutron star]background [gravitational radiation]010306 general physicseducationSTFCOrbital elementsGravitational WavesScience & Technology010308 nuclear & particles physicsGravitational waveVirgogravitational radiation: backgroundmodulation: frequencyRCUKNeutron StarsLIGOgravitational radiation detectordetector: sensitivityNeutron starVIRGOgravitational radiation: emissionDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikcoalescence [binary][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]binary stars; neutron stars
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Stability and extraction of bioactive sulfur compounds from Allium genus processed by traditional and innovative technologies

2017

Abstract Since ancient times, species from the Allium genus have been used in both culinary and medicinal applications. The health promoting properties, with well documented “evidence-based” studies, were attributed to the genus’ high content of bioactive organosulfur compounds. For these reasons, the organosulfur compounds have attracted interest in both food and pharmaceutical industries to be used as additives or supplements. Therefore, improvement in the extraction and stability during processing and storage of these molecules is crucial. The presented review documents the effects of traditional and innovative processing techniques on the extraction and stability of organosulfur compoun…

biologyChemistry010401 analytical chemistryExtraction (chemistry)chemistry.chemical_element04 agricultural and veterinary sciencesbiology.organism_classification040401 food science01 natural sciencesSulfur0104 chemical sciencesWhole systems0404 agricultural biotechnologyEnzymatic hydrolysisAllium ; Bioactive sulfur compounds ; Thermal processing ; High pressure processing ; Ultrasound ; Microwaves ; Supercritical fluids ; Food analysis ; Food compositionOrganic chemistryAlliumOrganosulfur compoundsFood ScienceJournal of Food Composition and Analysis
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Phaenocompsopogon pustulatus n.gen.n. sp., a calcareous alga from the lacustrine rotliegend of the Saar-Nahe Basin (SW-Germany)

1992

Phaenocompsopogon pustulatus n. gen. n. sp. is a calcareous freshwater alga, probably of rhodophycean affinity. The fossils are mainly known from one locality in the Lower Permian of the Saar-Nahe Basin. The algal remains form a packstone in the Reckweilerhof-Bank of the Altenglan Formation. The simple thallus branches irregularly y-shaped and is covered with abundant pustules. An axial canal is characteristic, as are distinct cell features of an inner and outer cortex surrounding a structureless medulla. Most fossils are silicified and often three-dimensionally preserved. The algae lived in a wave-dominated environment, probably in offshore shallow water. The limited occurrence suggests sp…

biologyPermianStratigraphyPaleontologyGeologyStructural basinbiology.organism_classificationThallusWaves and shallow waterPaleontologyAlgaeSaar–Nahe BasinSedimentologyCalcareousGeologyFacies
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Dynamics of boson stars and fermion-boson stars: a numerical-relativity panorama

2022

Los albores de la astronomía de ondas gravitacionales, actualmente liderada por la Colaboración LIGO-Virgo-KAGRA, abren un nuevo canal para inspeccionar la verdadera naturaleza de los objetos compactos oscuros. Los miembros más convincentes de esta categoría son los agujeros negros, de los que se cree ampliamente que están bien descritos por la métrica de Kerr cerca del equilibrio. Se han propuesto varias posibilidades teóricas más exóticas, denominadas imitadores de agujeros negros, ya que sus propiedades y dinámica se parecen en ciertos aspectos a las de los agujeros negros. Entre esos objetos compactos oscuros alternativos, las estrellas bosónicas, descritas por un campo escalar o vector…

boson starsgravitational wavesfermion-boson starsgeneral relativitynumerical relativityUNESCO::ASTRONOMÍA Y ASTROFÍSICA
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Refractive index of GaTe under high pressure

2000

In this paper we describe two experiments, in the near- and mid-infrared, designed to investigate the evolution under pressure of the GaTe refractive index for polarization parallel and perpendicular to the crystallographic c-axis (in the layer plane). The refractive index dispersion for both light polarizations has been determined up to 5.5 GPa. It is found that the refractive index increases faster in the direction perpendicular to the c-axis than along the c-axis. To find out the origin of such a difference we used a Phillips-Van Vechten model and arrived at the conclusion that it is due to the different pressure behaviour of the Penn gap for each polarization.

business.industryBand gapChemistryInfraredCondensed Matter PhysicsPolarization (waves)Electronic Optical and Magnetic MaterialsOpticsHigh pressureDispersion relationMaterials ChemistryPerpendicularElectrical and Electronic EngineeringbusinessStep-index profileRefractive indexSemiconductor Science and Technology
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