Search results for "Instrument"

showing 10 items of 5652 documents

Muon neutrino charged current quasi-elastic interactions in the T2K off-axis near detector

2015

246 páginas. Tesis Doctoral del Departamento de Física Atómica, Molecular y Nuclear de la Universidad de Valencia y del Instituto de Física Corpuscular (IFIC).

neutrinoexperiment:FÍSICA [UNESCO]Physics::Instrumentation and DetectorsUNESCO::FÍSICAinteractionHigh Energy Physics::ExperimentFísica de Partículasquasi-elasticcharged current
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Deep Underground Neutrino Experiment (DUNE) Near Detector Conceptual Design Report

2021

The Deep Underground Neutrino Experiment (DUNE) is an international, world-class experiment aimed at exploring fundamental questions about the universe that are at the forefront of astrophysics and particle physics research. DUNE will study questions pertaining to the preponderance of matter over antimatter in the early universe, the dynamics of supernovae, the subtleties of neutrino interaction physics, and a number of beyond the Standard Model topics accessible in a powerful neutrino beam. A critical component of the DUNE physics program involves the study of changes in a powerful beam of neutrinos, i.e., neutrino oscillations, as the neutrinos propagate a long distance. The experiment co…

neutrinoneutriino-oskillaationeutrino oscillationsnear detectorDUNEPhysics::Instrumentation and DetectorsilmaisimettutkimuslaitteetneutriinotHigh Energy Physics::ExperimenthiukkasfysiikkaDeep Underground Neutrino Experiment
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Solar neutrino spectroscopy in Borexino

2018

International audience; In more than ten years of operation, Borexino has performed a precision measurement of the solar neutrino spectrum, resolving almost all spectral components originating from the proton-proton fusion chain. The presentation will review the results recently released for the second data taking phase 2012–2016 during which the detector excelled by its unprecedentedly low background levels. New results on the rate of pp, 7Be, pep and 8B neutrinos as well as their implications for solar neutrino oscillations and metallicity are discussed.

neutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoMetallicityNuclear physicsbackground: lowneutrino: spectrum[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino oscillationSpectroscopyBorexinoPhysicsProton–proton chain reactionpp-chainp p: fusionprecision measurementDetector* Automatic Keywords *13. Climate actionsolar neutrinosspectralHigh Energy Physics::ExperimentBorexinoneutrino: oscillationNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Increasing the Astrophysical Reach of the Advanced Virgo Detector via the Application of Squeezed Vacuum States of Light

2019

Current interferometric gravitational-wave detectors are limited by quantum noise over a wide range of their measurement bandwidth. One method to overcome the quantum limit is the injection of squeezed vacuum states of light into the interferometer's dark port. Here, we report on the successful application of this quantum technology to improve the shot noise limited sensitivity of the Advanced Virgo gravitational-wave detector. A sensitivity enhancement of up to 3.2±0.1 dB beyond the shot noise limit is achieved. This nonclassical improvement corresponds to a 5%-8% increase of the binary neutron star horizon. The squeezing injection was fully automated and over the first 5 months of the thi…

neutron star: binaryGravitational waves detectionGeneral Physics and Astronomy01 natural sciencesvacuum stateNOISEinterferometric detectorLIGOnoise: quantumgravitational waves; squeezing; vacuumSettore FIS/01PhysicsQuantum opticsPhysicsQuantum limitQuantum noiseDetectorPhysical Sciencesgravitational waves squeezed lightinterferometric detectorsGravitational waveSqueezed coherent statePhysics Multidisciplinarysqueezed stateGravitation and AstrophysicshorizonGravitational wavesGeneral Relativity and Quantum CosmologyOpticsSettore FIS/05 - Astronomia e Astrofisica0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]SDG 7 - Affordable and Clean Energy010306 general physicsenhancementAstrophysiqueScience & Technology/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energybusiness.industryShot noisegravitational radiationgravitational waves thermal noisesensitivityLIGOdetector: sensitivityQuantum technology* Automatic Keywords *VIRGOinjectionPhysics and Astronomygravitational radiation detector: interferometerGravitational waves; interferometric detectors; noiseWAVEbusiness[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]gravitational waves nonlinear optics quantum opticsPhysical Review Letters
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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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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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Modification of a commercial atomic force microscopy for low-noise, high-resolution frequency-modulation imaging in liquid environment.

2011

A key issue for high-resolution frequency-modulation atomic force microscopy imaging in liquids is minimizing the frequency noise, which requires a detailed analysis of the corresponding noise contributions. In this paper, we present a detailed description for modifying a commercial atomic force microscope (Bruker MultiMode V with Nanoscope V controller), aiming at atomic-resolution frequency-modulation imaging in ambient and in liquid environment. Care was taken to maintain the AFMs original stability and ease of operation. The new system builds upon an optimized light source, a new photodiode and an entirely new amplifier. Moreover, we introduce a home-built liquid cell and sample holder …

noiseMaterials scienceoptical sensorsAtomic force acoustic microscopy530Noise (electronics)law.inventionOpticsphotodiodeslawInstrumentationAtomic de Broglie microscopeatomic force microscopycalcium compoundsbusiness.industrysample holdersAmplifierNoise spectral densityPhotodiodefrequency modulationmodulationfrequencyamplifiersbusinessNon-contact atomic force microscopyFrequency modulationimage resolutionThe Review of scientific instruments
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Latest Developments and Results of Radiation Tolerance CMOS Sensors with Small Collection Electrodes

2020

The development of radiation hard Depleted Monolithic Active Pixel Sensors (DMAPS) targets the replacement of hybrid pixel detectors to meet radiation hardness requirements of at least 1.5e16 1 MeV neq/cm2 for the HL-LHC and beyond. DMAPS were designed and tested in the TJ180 nm TowerJazz CMOS imaging technology with small electrodes pixel designs. This technology reduces costs and provides granularity of 36.4x36.4 um2 with low power operation (1 uW/pixel), low noise of ENC < 20 e-, a small collection electrode (3 um) and fast signal response within 25 ns bunch crossing. This contribution will present the latest developments after the MALTA and Mini-MALTA sensors. It will illustrate the imp…

noiseParticle tracking detectors ; Radiation-hard detectors ; Electronic detector readout concepts ; CMOS sensors ; Monolithic active pixel sensorsMaterials science010308 nuclear & particles physicsbusiness.industryintegrated circuitelectrode01 natural sciencesCMOSRadiation toleranceefficiency0103 physical sciencesElectrodeHardware_INTEGRATEDCIRCUITSelectronics: readoutOptoelectronicssemiconductor detector[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental Techniquescontrol system010306 general physicsbusiness
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Generalized Noise Study of Solid-State Nanopores at Low Frequencies.

2017

Nanopore technology has been extensively investigated for analysis of biomolecules, and a success story in this field concerns DNA sequencing using a nanopore chip featuring an array of hundreds of biological nanopores (BioNs). Solid-state nanopores (SSNs) have been explored to attain longer lifetime and higher integration density than what BioNs can offer, but SSNs are generally considered to generate higher noise whose origin remains to be confirmed. Here, we systematically study low-frequency (including thermal and flicker) noise characteristics of SSNs measuring 7 to 200 nm in diameter drilled through a 20-nm-thick SiNx membrane by focused ion milling. Both bulk and surface ionic curren…

noiseta221Analytical chemistryIonic bondingBioengineering02 engineering and technologyElectrolyte010402 general chemistry01 natural sciencesNoise (electronics)Flicker noiseInstrumentationFluid Flow and Transfer Processesta114ChemistryProcess Chemistry and TechnologyFlicker021001 nanoscience & nanotechnology0104 chemical sciencesNanoporenanopore technologyChemical physicssolid-state nanoporesIon milling machine0210 nano-technologyVoltageACS sensors
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Un estudio longitudinal de la reputación social no conformista y la violencia en adolescentes desde la perspectiva de género

2011

El objetivo del presente estudio fue analizar la relación existente entre la reputación social del adolescente -percibida e ideal-, y la violencia instrumental -manifiesta y relacional- en adolescentes desde una perspectiva de género. La muestra utilizada en este estudios fue de 1319 adolescentes -T1- de ambos sexos (53% chicas y 47% chicos) y de edades comprendidas entre los 11 y los 16 años (edad media 13.5; desviación típica 1.5), escolarizados en siete centros educativos de enseñanza secundaria y, de 554 estudiantes -T2- (54% chicas y 46% chicos). Los instrumentos utilizados fueron la Escala de Reputación Social no conformista de Carroll, Houghton, Hattie y Durkin (1999) y la Escala de …

non-conforming social reputationadolescencialcsh:Psychologylcsh:BF1-990adolescenceviolencia instrumentalinstrumental violencereputación social no conformistaPsychosocial Intervention
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