Search results for "MINOS"

showing 10 items of 739 documents

Measurement of Solar pp-neutrino flux with Borexino: results and implications

2015

International audience; Measurement of the Solar pp-neutrino flux completed the measurement of Solar neutrino fluxes from the pp-chain of reactions in Borexino experiment. The result is in agreement with the prediction of the Standard Solar Model and the MSW/LMA oscillation scenario. A comparison of the total neutrino flux from the Sun with Solar luminosity in photons provides a test of the stability of the Sun on the 10(5) years time scale, and sets a strong limit on the power production by the unknown energy sources in the Sun.

model: solarHistoryneutrino: solarSolar neutrinoAstrophysics::High Energy Astrophysical Phenomenaluminosity: solarSolar luminosity[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyneutrino: fluxEducationLuminosityNuclear physicsPhysics and Astronomy (all)SEARCH0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Astrophysics::Solar and Stellar Astrophysicsddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsDETECTORBorexinoMSW effectPhysicsStandard solar modelSolar energetic particles010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyphotonAstronomySolar neutrino problemstabilityoscillationComputer Science Applicationsp p13. Climate actionPhysics::Space PhysicsBorexinoAstrophysics::Earth and Planetary AstrophysicsNeutrinoexperimental results
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El fenómeno senderista en España. Análisis por un panel de expertos

2014

El fenómeno senderista en España. Análisis por un panel de expertos. El senderismo se ha convertido en una de las actividades físico-recreativas más importantes de nuestra sociedad. Los enfoques de práctica superan las motivaciones deportivas para incorporar objetivos turísticos, de calidad de vida, de movilidad no motorizada o del desarrollo rural, por citar algunos ejemplos. Por otra parte, el senderismo admite actividades afines (excursionismo, caminata, trekking, paseo,…) y coexiste perfectamente con otras prácticas complementarias (carreras de montaña, vías ferratas, Btt, equitación,…) que le convierten en un verdadero fenómeno social. Frente una actividad de tal envergadura y transcen…

movilidad no motorizadacaminos naturalesgestión deportivaclub de montañaespacios naturalesUNESCO::CIENCIAS ECONÓMICAS::Organización y dirección de empresasmontañismoalojamientosUNESCO::SOCIOLOGÍAVías verdesmovilidad pedrestre:PEDAGOGÍA::Organización y planificación de la educación [UNESCO]fenómeno socialocio y deportemovilidad urbanaturismo de montañaexcursionismo:CIENCIAS ECONÓMICAS::Organización y dirección de empresas ::Marketing [UNESCO]trekking:SOCIOLOGÍA [UNESCO]tiempo libreUNESCO::PEDAGOGÍA::Organización y planificación de la educaciónUNESCO::CIENCIAS ECONÓMICAS::Organización y dirección de empresas ::Marketingsenderismoturismoturismo deportivo:CIENCIAS ECONÓMICAS::Organización y dirección de empresas [UNESCO]
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Pràctica 1. Mètodes psicofísics de mesura

2018

El document forma part dels materials docents programats mitjançant l'ajut del Servei de Política Lingüística de la Universitat de València. Pràctica 1 de l'assignatura de psicofísica de la visió on l'objectiu és aprendre a emprar alguns dels mètodes que s’usen més habitualment als experiments de psicofísica: el mètode d’ajust, el mètode dels límits clàssic, un mètode adaptatiu per cerca binària i el mètode dels estímuls constants

mètode de l'ajustmètodes dels límitsfisicamètode de cerca binàriamètode de l'estímul constantluminositat
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Práctica de Métodos Psicofísicos de Medida: Igualación de luminosidades

2016

Material para realizar una práctica sobre métodos psicofísicos de medida, a partir de un experimento de igualación asimétrica de luminosidades, que incluye guiones, tablas de resultados y un programa de instalación del programa de generación y control de los estímulos. El usuario debe implementar manualmente los distintos métodos sugeridos en el guión de la práctica.

métodos psicofísicos de medidaluminanciaUNESCO::FÍSICA::Óptica ::Física de la visiónluminosidad
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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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New orbital ephemerides for the dipping source 4U 1323-619: Constraining the distance to the source

2016

4U 1323-619 is a low mass X-ray binary system that shows type I X-ray bursts and dips. The most accurate estimation of the orbital period is 2.941923(36) hrs and a distance from the source that is lower than 11 kpc has been proposed. We aim to obtain the orbital ephemeris, the orbital period of the system, as well as its derivative to compare the observed luminosity with that predicted by the theory of secular evolution. We took the advantage of about 26 years of X-ray data and grouped the selected observations when close in time. We folded the light curves and used the timing technique, obtaining 12 dip arrival times. We fit the delays of the dip arrival times both with a linear and a quad…

neutron X-rays: binaries X-rays: stars ephemerides stars: individual: 4U 1323-619 [stars]010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsEphemeris01 natural sciencesLuminositySettore FIS/05 - Astronomia E Astrofisica0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)stars: neutron X-rays: binaries X-rays: stars ephemerides stars: individual: 4U 1323-619Astronomy and AstrophysicsLight curveOrbital periodGalaxyNeutron starSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsLow MassAstrophysics - High Energy Astrophysical Phenomena
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Timing an Accreting Millisecond Pulsar: Measuring the Accretion Torque in IGR J00291+5934

2006

We performed a timing analysis of the fastest accreting millisecond pulsar IGR J00291+5934 using RXTE data taken during the outburst of December 2004. We corrected the arrival times of all the events for the orbital (Doppler) effects and performed a timing analysis of the resulting phase delays. In this way we have the possibility to study, for the first time in this class of sources, the spin-up of a millisecond pulsar as a consequence of accretion torques during the X-ray outburst. The accretion torque gives us for the first time an independent estimate of the mass accretion rate onto the neutron star, which can be compared with the observed X-ray luminosity. We also report a revised valu…

neutron; stars : magnetic fields; pulsars : general; pulsars : individual : IGR J00291+5934; X-ray : binaries [accretion accretion disks; stars]X-rays : binariesAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesAstrophysicsaccretion accretion diskAstrophysicsX-ray : binariesBinary pulsarLuminositypulsars : individual : IGR J00291+5934symbols.namesakePulsarMillisecond pulsarAstrophysics::Solar and Stellar Astrophysicspulsars : individual (IGR J00291+5934)PhysicsAccretion (meteorology)general; pulsars : individual (IGR J00291+5934); stars : magnetic fields; stars : neutron; X-rays : binaries [pulsars]Astrophysics (astro-ph)pulsars : generalStatic timing analysisAstronomystars : magnetic fieldAstronomy and Astrophysicsstars : neutronNeutron starSpace and Planetary SciencesymbolsAstrophysics::Earth and Planetary AstrophysicsDoppler effectX-ray pulsar
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Near‐IR Radiation‐Induced Attenuation of Aluminosilicate Optical Fibers

2021

The X-ray radiation-induced attenuation (RIA) growth kinetics are studied online in different single-mode aluminosilicate optical fibers in the near-IR (NIR) domain to evaluate their potential in terms of dosimetry. The optical fibers differ by Al contents, core sizes, drawing parameters, and also by a preform deposition process. The data show no dependence of the RIA on all these parameters, a positive result for the design of point or distributed radiation detectors exploiting RIA to monitor the dose. The RIA growth rate is unchanged for dose rates changing from 0.073 to 6.25 Gy(SiO2) s−1, and the RIA linearly increases with the dose up to 2 kGy(SiO2). Small but noticeable RIA changes are…

optical fibersMaterials scienceOptical fiberRadiation induced02 engineering and technology01 natural scienceslaw.inventionX-ray irradiations[SPI]Engineering Sciences [physics]020210 optoelectronics & photonicsAluminosilicatelaw0103 physical sciences0202 electrical engineering electronic engineering information engineeringMaterials Chemistryradiation-induced attenuationElectrical and Electronic EngineeringComposite materialComputingMilieux_MISCELLANEOUS010308 nuclear & particles physicsAttenuationSurfaces and InterfacesCondensed Matter PhysicsSurfaces Coatings and FilmsElectronic Optical and Magnetic Materialsaluminosilicate glassesradiation effectsphysica status solidi (a)
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Sorption and mechanism studies of Cu2+, Sr2+ and Pb2+ ions on mesoporous aluminosilicates/zeolite composite sorbents

2020

The research aimed to develop a novel mesoporous aluminosilicate/zeolite composite by the template co-precipitation method. The effect of aluminosilicate (AlSi) and zeolite (NaY) on the basic properties and adsorption capacity of the resultant composite was conducted at different mass ratios of AlSi/NaY (i.e., 5/90, 10/80, 15/85, 20/80, and 50/50). The adsorption characteristics of such composite and its feedstock materials (i.e., aluminosilicates and zeolite) towards radioactive Sr2+ ions and toxic metals (Cu2+ and Pb2+ ions) in aqueous solutions was investigated. Results indicated that BET surface area (SBET), total pore volume (VTotal), and mesopore volume (VMeso) of prepared materials f…

radioactive ionraskasmetallitzeoliititmesoporous aluminosilicatesilikaatitadsorptiontextural propoertyheavy metalzeolitevedenkäsittelyadsorptiokomposiitit
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Hard Two-Photon Contribution to Elastic Lepton-Proton Scattering Determined by the OLYMPUS Experiment

2017

The OLYMPUS collaboration reports on a precision measurement of the positron-proton to electron-proton elastic cross section ratio, $R_{2\gamma}$, a direct measure of the contribution of hard two-photon exchange to the elastic cross section. In the OLYMPUS measurement, 2.01~GeV electron and positron beams were directed through a hydrogen gas target internal to the DORIS storage ring at DESY. A toroidal magnetic spectrometer instrumented with drift chambers and time-of-flight scintillators detected elastically scattered leptons in coincidence with recoiling protons over a scattering angle range of $\approx 20\degree$ to $80\degree$. The relative luminosity between the two beam species was mo…

ratioPhysics::Instrumentation and DetectorsHadronFOS: Physical sciencesSocio-culturaleGeneral Physics and AstronomyElectron01 natural sciencestransfersNuclear physicsEconomica0103 physical sciencesddc:550electromagnetic form factorsNuclear Experiment (nucl-ex)010306 general physicselectromagnetic form factors transfers ratioNuclear ExperimentPhysicsLuminosity (scattering theory)010308 nuclear & particles physicsScatteringGenerator (category theory)Form factor (quantum field theory)BremsstrahlungHigh Energy Physics::ExperimentLeptonPhysical Review Letters
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