Search results for "Measurements of"

showing 10 items of 159 documents

New Acoustic Test Chambers at the University of Palermo

2008

Acoustic test chambers at the University of Palermo have been completed after a design optimization of existent building structures. A unique building houses five reverberation chambers, differently coupled each other in order to achieve a large flexibility on testing procedures, and offices for the staff. Main measurements offered to national and international standards include determination of sound power, sound insulation and sound absorption. Reverberation chambers present peculiar geometries in order to achieve the desidered sound fields. Chambers structure and layout within the whole building, housing all the acoustic facilities, has been designed in order to achieve strong sound insu…

Flexibility (engineering)geographyAbsorption (acoustics)Reverberationgeography.geographical_feature_categorySettore ING-IND/11 - Fisica Tecnica AmbientaleAcoustics and UltrasonicsComputer scienceAcousticsSound powerTest (assessment)SoundproofingArts and Humanities (miscellaneous)Reverberation room design: theory applications to measurements of sound absorption transmission loss sound powerSound (geography)
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Observation of Electron Neutrino Appearance in a Muon Neutrino Beam

2014

The T2K experiment has observed electron neutrino appearance in a muon neutrino beam produced 295 km from the Super-Kamiokande detector with a peak energy of 0.6 GeV. A total of 28 electron neutrino events were detected with an energy distribution consistent with an appearance signal, corresponding to a significance of 7.3$\sigma$ when compared to 4.92 $\pm$ 0.55 expected background events. In the PMNS mixing model, the electron neutrino appearance signal depends on several parameters including three mixing angles $\theta_{12}$, $\theta_{23}$, $\theta_{13}$, a mass difference $\Delta m^2_{32}$ and a CP violating phase $\delta_{\mathrm{CP}}$. In this neutrino oscillation scenario, assuming $…

General PhysicsParticle physicsSolar neutrinoPhysics MultidisciplinaryFOS: Physical sciencesGeneral Physics and Astronomy7. Clean energy09 EngineeringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Tau neutrino[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Neutrino oscillation01 Mathematical SciencesPhysicsScience & Technology02 Physical Scienceshep-exPhysicsHigh Energy Physics::PhenomenologyT2K experimentFísicaSolar neutrino problemNeutrino detectorT2K CollaborationPhysical SciencesMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino
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High energy neutrino telescopes in the Northern Hemisphere

2012

We review the status and results of the high energy neutrino telescopes in the Northern Hemisphere, namely ANTARES and Baikal (NT200+).

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsNuclear and High Energy PhysicsPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaDark matterAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesAstronomyFísicaAstrophysicsSolar neutrino problemPhysics::GeophysicsNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaNeutrino oscillationInstrumentationAstrophysics::Galaxy Astrophysics
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Production of keV sterile neutrinos in supernovae: New constraints and gamma-ray observables

2019

We study the production of sterile neutrinos in supernovae, focusing in particular on the keV--MeV mass range, which is the most interesting range if sterile neutrinos are to account for the dark matter in the Universe. Focusing on the simplest scenario in which sterile neutrinos mixes only with muon or tau neutrino, we argue that the production of keV--MeV sterile neutrinos can be strongly enhanced by a Mikheyev--Smirnov--Wolfenstein (MSW) resonance, so that a substantial flux is expected to emerge from a supernova, even if vacuum mixing angles between active and sterile neutrinos are tiny. Using energetics arguments, this yields limits on the sterile neutrino parameter space that reach do…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSterile neutrinoParticle physicsPhysics::Instrumentation and Detectors010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoHigh Energy Physics::PhenomenologyFOS: Physical sciencesSolar neutrino problemComputer Science::Digital Libraries7. Clean energy01 natural sciencesCosmic neutrino backgroundHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Neutrino detector0103 physical sciencesMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical Phenomena010303 astronomy & astrophysicsPhysical Review D
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Sterile neutrinos and B–L symmetry

2017

We revisit the relation between the neutrino masses and the spontaneous breaking of the B-L gauge symmetry. We discuss the main scenarios for Dirac and Majorana neutrinos and point out two simple mechanisms for neutrino masses. In this context the neutrino masses can be generated either at tree level or at quantum level and one predicts the existence of very light sterile neutrinos with masses below the eV scale. The predictions for lepton number violating processes such as mu to e and mu to e gamma are discussed in detail. The impact from the cosmological constraints on the effective number of relativistic degree of freedom is investigated.

High Energy Physics - TheoryNuclear and High Energy PhysicsSterile neutrinoParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)Computer Science::Digital Libraries01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsNeutrino oscillationGauge symmetryPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyLepton numberlcsh:QC1-999High Energy Physics - PhenomenologyMAJORANAHigh Energy Physics - Theory (hep-th)Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrinolcsh:PhysicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysics Letters B
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Light sterile neutrino from extra dimensions and four-neutrino solutions to neutrino anomalies

1999

We propose a four-neutrino model which can reconcile the existing data coming from underground experiments in terms of neutrino oscillations, together with the hint from the LSND experiment and a possible neutrino contribution to the hot dark matter of the Universe. It applies the idea that extra compact dimensions, probed only by gravity and possibly gauge-singlet fields, can lower the fundamental scales such as the Planck, string or unification scales. Our fourth light neutrino $\nu_s$ ($s$ for sterile) is identified with the zero mode of the Kaluza-Klein states. To first approximation \nu_sterile combines with the nu_mu in order to form a Dirac neutrino with mass in the eV range leaving …

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsParticle physicsSterile neutrinoHot dark matterSolar neutrinoHigh Energy Physics::PhenomenologyFísicaFOS: Physical sciencesMassless particleHigh Energy Physics - PhenomenologyExtra dimensionsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Measurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino oscillationPhysical Review D
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High significance measurement of the terrestrial neutrino flux with the Borexino detector

2015

International audience; We review the geoneutrino measurement with Borexino from 2056 days of data taking.

HistoryParticle physicsSolar neutrinoFlux010502 geochemistry & geophysics01 natural sciencesneutrino: fluxNOEducationNuclear physicstalk: Torino 2015/09/07Physics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530Borexino0105 earth and related environmental sciencesPhysics010308 nuclear & particles physicsDetectorComputer Science ApplicationsNeutrino detectorMeasurements of neutrino speedBorexinoneutrino: geophysicsNeutrinoexperimental results
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SOX: search for short baseline neutrino oscillations with Borexino

2015

International audience; The Borexino detector has convincingly shown its outstanding performances in the low energy regime through its accomplishments in the observation and study of the solar and geo neutrinos. It is then an ideal tool to perform a state of the art source-based experiment for testing the longstanding hypothesis of a fourth sterile neutrino with ~ eV(2) mass, as suggested by several anomalies accumulated over the past three decades in source, reactor, and accelerator-based experiments. The SOX project aims at successively deploying two intense radioactive sources, made of Cerium (antineutrino) and Chromium (neutrino), respectively, in a dedicated pit located beneath the det…

HistoryParticle physicsSterile neutrinochromium: nuclidePhysics::Instrumentation and DetectorsSolar neutrino[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyEducationNuclear physicsPhysics and Astronomy (all)0103 physical sciencesddc:530[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationBorexinoactivity reportPhysics010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyneutrino: particle sourceSolar neutrino problemneutrino: sterilesensitivityComputer Science ApplicationsNeutrino detector13. Climate actioncerium: nuclideMeasurements of neutrino speedHigh Energy Physics::ExperimentBorexinoneutrino: oscillationNeutrinoantineutrino: particle source
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Low-energy Neutrino Astronomy in LENA

2015

LENA (Low Energy Neutrino Astronomy) is a proposed next-generation neutrino detector based on 50 kilotons of liquid scintillator. The low detection threshold, good energy resolution and excellent background rejection inherent to the liquid-scintillator detectors make LENA a versatile observatory for low-energy neutrinos from astrophysical and terrestrial sources. In the framework of the European LAGUNA-LBNO design study, LENA is also considered as far detector for a very-long baseline neutrino beam from CERN to Pyhasalmi ¨ (Finland). The present contribution gives an overview LENA’s broad research program, highlighting the unique capabilities of liquid scintillator for the detection of low-…

LENAPhysicsParticle physicsta114Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologySolar neutrino problemPhysics and Astronomy(all)astroparticle physics. underground physicsNuclear physicslow-energy neutrino astronomyNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoNeutrino oscillationElectron neutrinoPhysics Procedia
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Magnetic Field Gradiometer with Sub-Micron Spatial Resolution Based on Caesium Vapour in an Extremely Thin Cell

2015

Abstract In this paper we present a device for measuring the magnetic field and its gradient with a spatial resolution of several hundred nanometres. This device is based on caesium metal vapour confined to an extremely thin cell (ETC). To measure magnetic signals, we use absorption and very low laser powers, which might be appealing for modern fabrication techniques. A portable, fully automated device was constructed.

Materials sciencebusiness.industryMagnetometerGeneral EngineeringGeneral Physics and Astronomychemistry.chemical_elementGradiometerlcsh:QC1-999Magnetic fieldlaw.inventionmeasurements of magnetic field gradientOpticschemistrylawCaesiummagnetometermagneto-optical resonancesextremely thin cellbusinessImage resolutionlcsh:PhysicsLatvian Journal of Physics and Technical Sciences
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