Search results for " Detectors"

showing 10 items of 2027 documents

Search for low-energy neutrinos from astrophysical sources with Borexino

2019

We report on searches for neutrinos and antineutrinos from astrophysical sources performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. Electron antineutrinos ($\bar{\nu}_e$) are detected in an organic liquid scintillator through the inverse $\beta$-decay reaction. In the present work we set model-independent upper limits in the energy range 1.8-16.8 MeV on neutrino fluxes from unknown sources that improve our previous results, on average, by a factor 2.5. Using the same data set, we first obtain experimental constraints on the diffuse supernova $\bar{\nu}_e$ fluxes in the previously unexplored region below 8 MeV. A search for $\bar{\nu}_e$ in the solar ne…

antineutrinosPhysics - Instrumentation and Detectorssolar flaresmagnetic field: highneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoscintillation counter: liquidelastic scatteringantineutrino/e: particle identification01 natural sciences7. Clean energyneutrino: fluxlaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: supernova26.65.+t010303 astronomy & astrophysicsBorexinoElastic scatteringPhysicsSolar flareSupernova Relic Neutrinosneutrino: energy spectrumS067EB8neutrinosInstrumentation and Detectors (physics.ins-det)neutrino: magnetic momentDiffuse Supernova Neutrino Background3. Good healthSupernovaHomestakeddc:540neutrino: flavorAntineutrinoBorexinoNeutrino97.60.BwHomestake experimentFlareantineutrino/e: fluxAntineutrinos13.15.+G; 26.65.+T; 29.40.Mc; 97.60.Bw; Antineutrinos; Diffuse supernova neutrino background; Neutrinos; Solar flares; Supernova relic neutrinosAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSupernova relic neutrinosupernova relic neutrinosNONuclear physics13.15.+gPE2_2Antineutrinos; Neutrinos; Diffuse supernova neutrino background; Supernova relic neutrinos; Solar flares0103 physical sciencesNeutrino[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinosdiffuse supernova neutrino background010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and Astrophysicsneutrino: particle source29.40.McGran SassoSolar flareSolar Flares13. Climate actionspectralHigh Energy Physics::Experimentexperimental results
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Borexino’s search for low-energy neutrino and antineutrino signals correlated with gamma-ray bursts

2017

International audience; A search for neutrino and antineutrino events correlated with 2350 gamma-ray bursts (GRBs) is performed with Borexino data collected between December 2007 and November 2015. No statistically significant excess over background is observed. We look for electron antineutrinos ( ν¯e ) that inverse beta decay on protons with energies from 1.8  MeV to 15  MeV and set the best limit on the neutrino fluence from GRBs below 8  MeV. The signals from neutrinos and antineutrinos from GRBs that scatter on electrons are also searched for, a detection channel made possible by the particularly radio-pure scintillator of Borexino. We obtain currently the best limits on the neutrino f…

antineutrinoselectronAntineutrinosneutrino: solarPhysics::Instrumentation and Detectorsdata acquisitionSolar neutrino[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical Phenomenalow energy/MeV neutrinosElectrongamma ray: burst01 natural sciencesNuclear physicsLow energy/MeV neutrino0103 physical sciencesNeutrinoLow energy/MeV neutrinosNeutrinosNuclear Experiment010303 astronomy & astrophysicsGamma-ray burstBorexinoscintillation counterPhysicsflavor010308 nuclear & particles physicsbackgroundgamma-ray burstsneutrinosAntineutrinos; Gamma-ray bursts; Low energy/MeV neutrinos; Neutrinos; Astronomy and AstrophysicsAstronomy and Astrophysicssemileptonic decayantineutrinocorrelation: timeNeutrino detectorInverse beta decayddc:540Scintillation counterreadoutHigh Energy Physics::ExperimentBorexinoGamma-ray burstsNeutrinoGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Estimates for Divergence Velocities of Axially Moving Orthotropic Thin Plates

2014

Some models for axially moving orthotropic thin plates are investigated analytically via methods of complex analysis to derive estimates for critical plate velocities. Linearised Kirchhoff plate theory is used, and the energy forms of steady-state models are considered with homogeneous and inhomogeneous tension profiles in the cross direction of the plate. With the help of the energy forms, some limits for the divergence velocity of the plate are found analytically. In numerical examples, the derived lower limits for the divergence velocity are analysed for plates with small flexural rigidity. peerReviewed

axially movingPhysics::Instrumentation and DetectorsGeneral MathematicsAerospace EngineeringOcean EngineeringGeometry02 engineering and technologyOrthotropic material01 natural sciencesPhysics::Fluid Dynamics0203 mechanical engineering0103 physical sciencesorthotropicta216Divergence (statistics)010301 acousticsCivil and Structural EngineeringMathematicsTension (physics)Mechanical Engineeringkalvot (biologia)Flexural rigidityMechanicsstabilityPhysics::Classical PhysicsCondensed Matter Physicslautaset (astiat)020303 mechanical engineering & transportsplatesmembranesMechanics of MaterialsHomogeneousAutomotive EngineeringPlate theoryAxial symmetryMechanics Based Design of Structures and Machines
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Search for Axionlike Dark Matter through Nuclear Spin Precession in Electric and Magnetic Fields

2017

We report on a search for ultralow-mass axionlike dark matter by analyzing the ratio of the spinprecession frequencies of stored ultracold neutrons and 199Hg atoms for an axion-induced oscillating electric dipole moment of the neutron and an axion-wind spin-precession effect. No signal consistent with dark matter is observed for the axion mass range 10−24 ≤ ma ≤ 10−17 eV. Our null result sets the first laboratory constraints on the coupling of axion dark matter to gluons, which improve on astrophysical limits by up to 3 orders of magnitude, and also improves on previous laboratory constraints on the axion coupling to nucleons by up to a factor of 40. ispartof: Physical Review X vol:7 issue:…

axionsCosmology and Nongalactic Astrophysics (astro-ph.CO)[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]Nuclear TheoryAtomic Physics (physics.atom-ph)Physics::Instrumentation and Detectors[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]QC1-999FOS: Physical sciencesmagnetic field[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]dark matterPhysics - Atomic PhysicsNuclear Theory (nucl-th)High Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph][ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]axion: couplingNuclear Experiment (nucl-ex)gluon: couplingNuclear Experiment[ PHYS.NUCL ] Physics [physics]/Nuclear Theory [nucl-th]spin: precessionaxion: dark mattern: electric momentnucleus: spinatomPhysicsHigh Energy Physics::Phenomenologyspin precessionoscillation[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]neutron electric dipole momentelectric fieldHigh Energy Physics - PhenomenologyS029IAN[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph][ PHYS.HPHE ] Physics [physics]/High Energy Physics - Phenomenology [hep-ph]axion: mass[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]experimental resultsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review X
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Detecting the stimulated decay of axions at radio frequencies

2018

Assuming axion-like particles account for the entirety of the dark matter in the Universe, we study the possibility of detecting their decay into photons at radio frequencies. We discuss different astrophysical targets, such as dwarf spheroidal galaxies, the Galactic Center and halo, and galaxy clusters. The presence of an ambient radiation field leads to a stimulated enhancement of the decay rate; depending on the environment and the mass of the axion, the effect of stimulated emission may amplify the photon flux by serval orders of magnitude. For axion-photon couplings allowed by astrophysical and laboratory constraints(and possibly favored by stellar cooling), we find the signal to be wi…

axionsPhotonAstrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio telescopeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesStimulated emissionAxionGalaxy clusterAstrophysics::Galaxy AstrophysicsPhysicsdark matter detectorsdark matter theory010308 nuclear & particles physicsGalactic CenterAstronomy and AstrophysicsAstrophysics - Astrophysics of Galaxiesdwarfs galaxiesGalaxy3. Good healthHigh Energy Physics - Phenomenologyaxions; dark matter detectors; dark matter theory; dwarfs galaxiesAstrophysics of Galaxies (astro-ph.GA)Journal of Cosmology and Astroparticle Physics
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Conceptual design and simulation of a water Cherenkov muon veto for the XENON1T experiment

2014

XENON is a direct detection dark matter project, consisting of a time projection chamber (TPC) that uses xenon in double phase as a sensitive detection medium. XENON100, located at the Laboratori Nazionali del Gran Sasso (LNGS) in Italy, is one of the most sensitive experiments of its field. During the operation of XENON100, the design and construction of the next generation detector (of ton-scale mass) of the XENON project, XENON1T, is taking place. XENON1T is being installed at LNGS as well. It has the goal to reduce the background by two orders of magnitude compared to XENON100, aiming at a sensitivity of $2 \cdot 10^{-47} \mathrm{cm}^{\mathrm{2}}$ for a WIMP mass of 50 GeV/c$^{2}$. With…

axionsPhysics - Instrumentation and Detectors[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Cherenkov and transition radiationCherenkov detectorPhysics::Instrumentation and DetectorsDark matterDetector modelling and simulations I (interaction of radiation with matterchemistry.chemical_elementFOS: Physical sciences01 natural scienceslaw.inventionNuclear physicsXenonWIMPlawCherenkov and transition radiation Detector modelling and simulations Cherenkov detectors Dark Matter detectorsetc.)0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentationInstrumentation and Methods for Astrophysics (astro-ph.IM)Dark Matter detectors (WIMPsMathematical PhysicsCherenkov radiationetc)PhysicsMuonTime projection chamber010308 nuclear & particles physicsCherenkov detectorsDetectorAstrophysics::Instrumentation and Methods for Astrophysicsinteraction of photons with matterInstrumentation and Detectors (physics.ins-det)Cherenkov and transition radiation; Cherenkov detectors; Dark Matter detectors (WIMPs axions etc.); Detector modelling and simulations I (interaction of radiation with matter; interaction of hadrons with matter etc); interaction of photons with matter[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]interaction of hadrons with matterchemistryHigh Energy Physics::ExperimentAstrophysics - Instrumentation and Methods for AstrophysicsJOURNAL OF INSTRUMENTATION
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Neutrinos below 100 TeV from the southern sky employing refined veto techniques to IceCube data

2020

Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos with a typical energy cutoff well below 100 TeV. For the IceCube Neutrino Observatory located at the South Pole, the southern sky, containing the inner part of the Galactic plane and the Galactic Center, is a particularly challenging region at these energies, because of the large background of atmospheric muons. In this paper, we present recent advancements in data selection strategies for track-like muon neutrino events with energies below 100 TeV from the southern sky. The strategies utilize the outer detector regions as veto and features of the signal pattern to reduce the background of atm…

background [atmosphere]Physics::Instrumentation and Detectorsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenapoleFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryIceCubecharged currentHigh Energy Physics - Experiment (hep-ex)Neutrinos; Point sources; Veto techniquesSEARCHTRACK RECONSTRUCTION0103 physical sciencessupernovaMuon neutrinoatmosphere [muon]Neutrinos010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsneutrino muonMuon010308 nuclear & particles physicsICEGalactic CenterHigh Energy Physics::PhenomenologyVeto techniquesAstronomyPoint sourcesAstronomy and Astrophysicsflux [neutrino]Galactic planeobservatorySupernovaPhysics and AstronomySkyenergy [neutrino]gamma rayddc:540spectralHigh Energy Physics::ExperimentgalaxyNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Comparison between simulated and observed LHC beam backgrounds in the ATLAS experiment at E beam =4 TeV

2018

Results of dedicated Monte Carlo simulations of beam-induced background (BIB) in the ATLAS experiment at the Large Hadron Collider (LHC) are presented and compared with data recorded in 2012. During normal physics operation this background arises mainly from scattering of the 4 TeV protons on residual gas in the beam pipe. Methods of reconstructing the BIB signals in the ATLAS detector, developed and implemented in the simulation chain based on the FLUKA Monte Carlo simulation package, are described. The interaction rates are determined from the residual gas pressure distribution in the LHC ring in order to set an absolute scale on the predicted rates of BIB so that they can be compared qua…

background [beam]background: inducedPhysics::Instrumentation and DetectorsCiencias FísicasMonte Carlo method01 natural sciencesHigh Energy Physics - ExperimentSubatomär fysik//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)beam lossesSubatomic Physicsscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]and programsInstrumentationQCMathematical PhysicsPhysicsLarge Hadron ColliderRadiation calculationsAtlas (topology)Accelerator modelling and simulations (multi-particle dynamics; single-particle dynamics)DetectorATLAS experimentSettore FIS/01 - Fisica SperimentaleSimulation methods and programBeams (radiation) Accelerator modelling and simulations (multi-particle dynamics;; single-particle dynamics); Radiation calculations; Simulation methods; and programs; DETECTOR; SEARCHObservableAccelerator modelling and simulations (multi-particle dynamicMonte Carlo [numerical calculations]ATLASNuclear & Particles PhysicsAccelerator modelling and simulationsCERN LHC Coll collimators beam: backgroundcolliding beams [p p]numerical calculations: Monte CarloCIENCIAS NATURALES Y EXACTASParticle Physics - Experimentp p: scatteringAccelerator modelling and simulations (multi-particle dynamics; Radiation calculations; Simulation methods and programs; single-particle dynamics); Instrumentation; Mathematical Physics530 PhysicsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesFísica de Partículas y CamposAccelerator Physics and InstrumentationNuclear physicsFLUKAsingle-particle dynamics)ATLAS LHC High Energy PhysicsHIGH ENERGY PHYSICSSEARCH0103 physical sciencesddc:610010306 general physicsAbsolute scaleDETECTORpressure [gas]Science & Technology010308 nuclear & particles physicsScatteringhep-exRadiation calculationscatteringAcceleratorfysik och instrumentering//purl.org/becyt/ford/1.3 [https]ghostAccelerator modelling and simulations (multi-particle dynamicsSimulation methodscorrelationinduced [background]Experimental High Energy Physicsgas: pressureSimulation methods and programsp p: colliding beamsexperimental results
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New high-sensitivity searches for neutrons converting into antineutrons and/or sterile neutrons at the HIBEAM/NNBAR experiment at the European Spalla…

2021

Abstract The violation of baryon number, B , is an essential ingredient for the preferential creation of matter over antimatter needed to account for the observed baryon asymmetry in the Universe. However, such a process has yet to be experimentally observed. The HIBEAM/NNBAR program is a proposed two-stage experiment at the European Spallation Source to search for baryon number violation. The program will include high-sensitivity searches for processes that violate baryon number by one or two units: free neutron–antineutron oscillation ( n → n ̄ ) via mixing, neutron–antineutron oscillation via regeneration from a sterile neutron state ( n → [ n ′ , n ̄ ′ ] → n ̄ ), and neutron disappearan…

baryon number violation; feebly interacting particles; European Spallation Source; baryogenesisPhysics beyond the Standard ModelNuclear TheoryEXPERIMENTAL LIMITfeebly interacting particlesbaryogenesisAntineutron01 natural sciencesSubatomär fysikANTIPROTON ANNIHILATIONn: oscillationSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentsterilePhysicsMIRROR MATTERnew physicsanti-nddc:Antimatterbaryon: asymmetryproposed experimentDAMA ANNUAL MODULATIONNuclear and High Energy PhysicsParticle physicsAccelerator Physics and Instrumentation114 Physical sciencesBaryon asymmetrynuclear physics0103 physical sciencesDARK-MATTERmixingNeutronSensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]TRANSITION OPERATORS010306 general physicsbaryon number: violationactivity report010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAcceleratorfysik och instrumenteringMAJORANA NEUTRINOSsensitivitybaryon number violationBaryogenesisregenerationEuropean Spallation SourceUNIFIED PICTUREB-L SYMMETRYBaryon numberBARYON-NUMBER NONCONSERVATION
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Study of supersymmetric signals with R-parity violation in ATLAS at LHC

2013

219 páginas. Tesis Doctoral del Departamento de Física Atómica, Molecular y Nuclear, de la Universidad de Valencia.

bilinear R-parity violation:FÍSICA::Física de altas energías [UNESCO]Physics::Instrumentation and DetectorsHigh Energy Physics::PhenomenologyUNESCO::FÍSICA::Física de altas energíasHigh Energy Physics::ExperimentLHCATLASsupersymmetryParticle Physics - Experiment
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