Search results for "fields"

showing 10 items of 575 documents

Calibration of advanced Virgo and reconstruction of the gravitational wave signal h(t) during the observing run O2

2018

In August 2017, Advanced Virgo joined Advanced LIGO for the end of the O2 run, leading to the first gravitational waves detections with the three-detector network. This paper describes the Advanced Virgo calibration and the gravitational wave strain h(t) reconstruction during O2. The methods are the same as the ones developed for the initial Virgo detector and have already been described in previous publications, this paper summarizes the differences and emphasis is put on estimating systematic uncertainties. Three versions of the h(t) signal have been computed for the Virgo O2 run, an online version and two post-run reprocessed versions with improved detector calibration and reconstruction…

O2 observation runPhysics and Astronomy (miscellaneous)AstronomyAstrophysicsdetector: networkVIRGO: calibration01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsHigh Energy Physics::Theorydetector: calibrationLIGOmirrorgravitational wavePhysicsQuantum Science & TechnologyPhysicsDetectorphotonAstrophysics::Instrumentation and Methods for AstrophysicsReconstruction algorithmMassless particleAmplitudeCalibration Advanced Virgo O2Physical SciencesCalibration[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Advanced VirgoAstrophysics - Instrumentation and Methods for Astrophysicson-linereconstructioninterferometergravitational wave calibration reconstruction photon calibrator Virgo O2 observation runPhysics MultidisciplinaryFOS: Physical sciencesO2General Relativity and Quantum Cosmology (gr-qc)Astronomy & Astrophysicsgravitational radiation: direct detectionParticle detectorGeneral Relativity and Quantum Cosmology0103 physical sciencesCalibrationcalibration; gravitational wave; O2 observation run; photon calibrator; reconstruction; Virgo; Physics and Astronomy (miscellaneous)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Science & Technology010308 nuclear & particles physicsGravitational waveVirgogravitational radiationcalibration; gravitational wave; O2 observation run; photon calibrator; reconstruction; Virgocalibrationphoton calibratorLIGOgravitational radiation detectordetector: sensitivity* Automatic Keywords *network
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A Pooled Analysis of Extremely Low-Frequency Magnetic Fields and Childhood Brain Tumors

2010

Pooled analyses may provide etiologic insight about associations between exposure and disease. In contrast to childhood leukemia, no pooled analyses of childhood brain tumors and exposure to extremely low-frequency magnetic fields (ELF-MFs) have been conducted. The authors carried out a pooled analysis based on primary data (1960–2001) from 10 studies of ELF-MF exposure and childhood brain tumors to assess whether the combined results, adjusted for potential confounding, indicated an association. The odds ratios for childhood brain tumors in ELF-MF exposure categories of 0.1–<0.2 μT, 0.2–<0.4 μT, and ≥0.4 μT were 0.95 (95% confidence interval: 0.65, 1.41), 0.70 (95% CI: 0.40, 1.22), and 1.1…

Oncologymedicine.medical_specialtyNeoplasms Radiation-InducedChildhood leukemiaEpidemiologyBrain tumorGlobal HealthCentral nervous system diseaseElectromagnetic FieldsRisk FactorsInternal medicineEpidemiologymedicineHumansChildBrain Neoplasmsbusiness.industryIncidenceConfoundingOdds ratiomedicine.diseaseConfidence intervalSurgeryMeta-analysisbusinessSystematic Reviews and Meta- and Pooled AnalysesAmerican Journal of Epidemiology
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Planar metamaterial analogue of electromagnetically induced transparency for plasmonic sensing.

2009

We experimentally demonstrate a planar metamaterial analogue of electromagnetically induced transparency at optical frequencies. The structure consists of an optically bright dipole antenna and an optically dark quadrupole antenna, which are cut-out structures in a thin gold film. A pronounced coupling-induced reflectance peak is observed within a broad resonance spectrum. A metamaterial sensor based on these coupling effects is experimentally demonstrated and yields a sensitivity of 588 nm/RIU and a figure of merit of 3.8.

Optics and PhotonicsMaterials scienceElectromagnetically induced transparencySurface PropertiesPhysics::OpticsBioengineeringlaw.inventionPlanarOpticsElectromagnetic FieldslawFigure of meritNanotechnologyGeneral Materials ScienceDipole antennaParticle SizePlasmonbusiness.industryMechanical EngineeringMetamaterialResonanceMembranes ArtificialGeneral ChemistryEquipment DesignCondensed Matter PhysicsRefractometryOptoelectronicsGoldAntenna (radio)businessNano letters
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Spin up and phase fluctuations in the timing of the accreting millisecond pulsar XTE J1807-294

2007

We performed a timing analysis of the 2003 outburst of the accreting X-ray millisecond pulsar XTE J1807-294 observed by RXTE. Using recently refined orbital parameters we report for the first time a precise estimate of the spin frequency and of the spin frequency derivative. The phase delays of the pulse profile show a strong erratic behavior superposed to what appears as a global spin-up trend. The erratic behavior of the pulse phases is strongly related to rapid variations of the light curve, making it very difficult to fit these phase delays with a simple law. As in previous cases, we have therefore analyzed separately the phase delays of the first harmonic and of the second harmonic of …

Orbital elementsPhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Phase (waves)Static timing analysisFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsLight curveAstrophysicsPulsars: General Stars: Pulsars: Individual: Alphanumeric: XTE J1807-294 Stars: Magnetic Fields Stars: Neutron X-Rays: Binaries [Stars]Pulse (physics)Settore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceMillisecond pulsarHarmonicStars: Pulsars: General Stars: Pulsars: Individual: Alphanumeric: XTE J1807-294 Stars: Magnetic Fields Stars: Neutron X-Rays: BinariesSpin-½
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Precise determination of orbital parameters in system with slowly drifting phases: application to the case of XTE J1807-294

2007

We describe a timing technique that allows to obtain precise orbital parameters of an accreting millisecond pulsar in those cases in which intrinsic variations of the phase delays (caused e.g. by proper variation of the spin frequency) with characteristic timescale longer than the orbital period do not allow to fit the orbital parameters over a long observation (tens of days). We show under which conditions this method can be applied and show the results obtained applying this method to the 2003 outburst observed by RXTE of the accreting millisecond pulsar XTE J1807-294 which shows in its phase delays a non-negligible erratic behavior. We refined the orbital parameters of XTE J1807-294 usin…

Orbital elementsPhysicspulsars : individualAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Phase (waves)pulsars : generalFOS: Physical sciencesstars : magnetic fieldAstronomy and AstrophysicsAstrophysicsOrbital periodAstrophysicsstars : neutronX-ray : binariesXTE J1807-294Space and Planetary ScienceMillisecond pulsarAstrophysics::Earth and Planetary AstrophysicsSpin (physics)Variation (astronomy)magnetic fields; stars : neutron; pulsars : general; pulsars : individual; XTE J1807-294; X-ray : binaries [stars]Order of magnitude
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Human brain organoids assemble functionally integrated bilateral optic vesicles

2021

During embryogenesis, optic vesicles develop from the diencephalon via a multistep process of organogenesis. Using induced pluripotent stem cell (iPSC)-derived human brain organoids, we attempted to simplify the complexities and demonstrate formation of forebrain-associated bilateral optic vesicles, cellular diversity, and functionality. Around day 30, brain organoids attempt to assemble optic vesicles, which develop progressively as visible structures within 60 days. These optic vesicle-containing brain organoids (OVB-organoids) constitute a developing optic vesicle's cellular components, including primitive corneal epithelial and lens-like cells, retinal pigment epithelia, retinal progeni…

OrganogenesisInduced Pluripotent Stem Cellsretinal pigment epitheliumiPSCsEmbryonic DevelopmentBiology03 medical and health sciencesDiencephalonchemistry.chemical_compoundProsencephalon0302 clinical medicineGeneticsOrganoidmedicineHumansInduced pluripotent stem cell030304 developmental biology0303 health sciencesforebrain organoidsRetinal pigment epitheliumbrain organoidsVesicleprimordial eye fieldsOVB-organoidsCell DifferentiationRetinalCell BiologyOptic vesicleHuman brainCell biologyOrganoidsmedicine.anatomical_structurenervous systemchemistryMolecular MedicineFOXG1; OVB-organoids; brain organoids; forebrain organoids; iPSCs; optic vesicles; primary cilium; primordial eye fields; retinal pigment epitheliumoptic vesiclesFOXG1030217 neurology & neurosurgeryprimary ciliumCell Stem Cell
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Measurement of the first ionization potential of astatine by laser ionization spectroscopy

2013

The radioactive element astatine exists only in trace amounts in nature. Its properties can therefore only be explored by study of the minute quantities of artificially produced isotopes or by performing theoretical calculations. One of the most important properties influencing the chemical behaviour is the energy required to remove one electron from the valence shell, referred to as the ionization potential. Here we use laser spectroscopy to probe the optical spectrum of astatine near the ionization threshold. The observed series of Rydberg states enabled the first determination of the ionization potential of the astatine atom, 9.31751(8) eV. New ab initio calculations are performed to sup…

Other Fields of PhysicsGeneral Physics and Astronomychemistry.chemical_element7. Clean energy01 natural sciencesGeneral Biochemistry Genetics and Molecular BiologyArticlePhysics in GeneralAb initio quantum chemistry methodsCHEMISTRYIonization0103 physical sciencesAtomPhysics::Atomic and Molecular ClustersFACILITYPhysics::Atomic Physics010306 general physicsAstatineSpectroscopyPhysicsMultidisciplinary010308 nuclear & particles physicsGeneral ChemistryION-SOURCEIon source3. Good healthchemistry13. Climate actionIonization energyAtomic physicsValence electronNature Communications
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Auditory and Cognitive Deficits Associated with Acquired Amusia after Stroke: A Magnetoencephalography and Neuropsychological Follow-Up Study

2010

Acquired amusia is a common disorder after damage to the middle cerebral artery (MCA) territory. However, its neurocognitive mechanisms, especially the relative contribution of perceptual and cognitive factors, are still unclear. We studied cognitive and auditory processing in the amusic brain by performing neuropsychological testing as well as magnetoencephalography (MEG) measurements of frequency and duration discrimination using magnetic mismatch negativity (MMNm) recordings. Fifty-three patients with a left (n = 24) or right (n = 29) hemisphere MCA stroke (MRI verified) were investigated 1 week, 3 months, and 6 months after the stroke. Amusia was evaluated using the Montreal Battery of …

PITCHMalemagnetoencephalographyMiddle Cerebral ArteryAnatomy and Physiologylcsh:MedicineMismatch negativity312 Clinical medicineNeuropsychological TestsAudiologymagnetic fieldsCardiovascularSocial and Behavioral SciencesBehavioral NeuroscienceLearning and MemoryCognition0302 clinical medicinePsychologyMedicinelcsh:Sciencemagnetoencephalography and neuropsychologicalClinical NeurophysiologyMultidisciplinarymedicine.diagnostic_testBRAIN RESPONSES05 social sciencesStroke RehabilitationCognitive flexibilityNeuropsychologyMagnetoencephalographyElectroencephalographyExperimental Psychologyfollow-up studyMiddle Aged3. Good healthElectrophysiologyStrokeHemorrhagic StrokeClinical PsychologyMemory Short-TermNeurologyMedicineSensory PerceptionFemaleMUSIC PERCEPTION DEFICITSResearch ArticleAdultCORTEXmedicine.medical_specialtyMISMATCH NEGATIVITY MMN515 PsychologyCognitive NeuroscienceCerebrovascular DiseasesNeuroimagingAmusiaAuditory cortex050105 experimental psychologyLateralization of brain functionPerceptual Disorders03 medical and health sciencesNeuropsychologyDiagnostic MedicineSPEECH INTONATIONHumans0501 psychology and cognitive sciencesBiologyMusic TherapyIschemic StrokeAuditory CortexCONGENITAL AMUSIAbusiness.industryMEMORYlcsh:R3112 NeurosciencesMagnetoencephalographymedicine.diseaseAuditory and cognitive deficits6131 Theatre dance music other performing artsNeuroanatomyDISCRIMINATIONBrain Injurieslcsh:QNEURAL-NETWORKSbusinessNeurocognitive030217 neurology & neurosurgeryNeuroscienceFollow-Up Studies
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Measurement of Upsilon production in collisions at root s=2.76 TeV

2014

The production of Υ(1S) , Υ(2S) and Υ(3S) mesons decaying into the dimuon final state is studied with the LHCb detector using a data sample corresponding to an integrated luminosity of 3.3pb-1 collected in proton–proton collisions at a centre-of-mass energy of s=2.76  TeV. The differential production cross-sections times dimuon branching fractions are measured as functions of the Υ transverse momentum and rapidity, over the ranges pT&lt;15 GeV/ c and 2.0&lt;y&lt;4.5 . The total cross-sections in this kinematic region, assuming unpolarised production, are measured to be σpp→Υ(1S)X×BΥ(1S)→μ+μ-=1.111±0.043±0.044nb,σpp→Υ(2S)X×BΥ(2S)→μ+μ-=0.264±0.023±0.011nb,σpp→Υ(3S)X×BΥ(3S)→μ+μ-=0.159±0.020±0.…

PP COLLISIONSScience & Technology530 PhysicsPhysicsPHYSICS PARTICLES & FIELDSOCTET QUARKONIA PRODUCTIONPhysics InstituteLHCb - Abteilung HofmannJ-PSIoctet quarkonia productin; PP collisions; J-PSI; hadronic production; decay; distributions; toolHigh Energy Physics - ExperimentSettore FIS/04 - Fisica Nucleare e SubnuclearePhysical SciencesDISTRIBUTIONSTOOLFísica nuclearDECAYParticle Physics - ExperimentHADRONIC PRODUCTION
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Next Generation Search for Axion and ALP Dark Matter with the International Axion Observatory

2018

International audience; More than 80 years after the postulation of dark matter, its nature remains one of the fundamental questions in cosmology. Axions are currently one of the leading candidates for the hypothetical, non-baryonic dark matter that is expected to account for about 25% of the energy density of the Universe. Especially in the light of the Large Hadron Collider at CERN slowly closing in on Weakly-Interacting Massive Particle (WIMP) searches, axions and axion-like particles (ALPs) provide a viable alternative approach to solving the dark matter problem. The fact that makes them particularly appealing is that they were initially introduced to solve a long-standing problem in qu…

Particle physicsCERN LabPhysics::Instrumentation and DetectorsDark matterObservatoriesaxion: detector7. Clean energy01 natural sciencesCosmologyHigh Energy Physics::TheoryPrimakoff effectSensitivityWIMP0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsAxionPrimakoff effectactivity reportPhysicsHelioscopeLarge Hadron Collider010308 nuclear & particles physicsPhysicsHigh Energy Physics::PhenomenologyToroidal magnetic fieldsDetectorsobservatory13. Climate actionCouplingsaxion-like particlesproposed experimentCERN Axion Solar Telescopeaxion: solarTelescopes
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