Search results for "particle source"

showing 10 items of 17 documents

IceCube search for neutrinos coincident with compact binary mergers from LIGO-Virgo's first gravitational-wave transient catalog

2020

Using the IceCube Neutrino Observatory, we search for high-energy neutrino emission coincident with compact binary mergers observed by the LIGO and Virgo gravitational-wave (GW) detectors during their first and second observing runs. We present results from two searches targeting emission coincident with the sky localization of each GW event within a 1000 s time window centered around the reported merger time. One search uses a model-independent unbinned maximum-likelihood analysis, which uses neutrino data from IceCube to search for pointlike neutrino sources consistent with the sky localization of GW events. The other uses the Low-Latency Algorithm for Multi-messenger Astrophysics, which …

010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsBayesian7. Clean energy01 natural sciencesNeutrino astronomy; High energy astrophysics; Gravitational waveslocalizationIceCubeIceCube Neutrino ObservatoryGravitational wavesparticle source [neutrino]0103 physical sciencesLIGO010303 astronomy & astrophysics0105 earth and related environmental sciencesastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsGravitational wavegravitational radiationAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsLIGOobservatorymessengerMassless particleVIRGONeutrino detector13. Climate actionSpace and Planetary ScienceNeutrino astronomycompact [binary]Physique des particules élémentairesddc:520High Energy Physics::ExperimentNeutrino astronomyNeutrinoAstrophysics - High Energy Astrophysical PhenomenaHigh energy astrophysicsLepton
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Search for Extraterrestrial Point Sources of Neutrinos with AMANDA-II

2003

We present the results of a search for point sources of high energy neutrinos in the northern hemisphere using AMANDA-II data collected in the year 2000. Included are flux limits on several AGN blazars, microquasars, magnetars and other candidate neutrino sources. A search for excesses above a random background of cosmic-ray-induced atmospheric neutrinos and misreconstructed downgoing cosmic-ray muons reveals no statistically significant neutrino point sources. We show that AMANDA-II has achieved the sensitivity required to probe known TeV gamma-ray sources such as the blazar Markarian 501 in its 1997 flaring state at a level where neutrino and gamma-ray fluxes are equal.

AMANDAcosmic radiation [neutrino]Solar neutrinoAstrophysics::High Energy Astrophysical Phenomenaparticle source [cosmic radiation]General Physics and AstronomyFOS: Physical sciencesAstrophysicsmagnetic [matter]Astrophysicsnumerical methodsddc:550quasarBlazarAstroparticle physicsPhysicsphotomultipliercosmic radiation [muon]water [Cherenkov counter]Astrophysics (astro-ph)AstronomySolar neutrino problemCosmic neutrino backgroundNeutrino detectorMeasurements of neutrino speedHigh Energy Physics::Experimentflux [cosmic radiation]blazar [AGN]data managementNeutrinoupper limitexperimental results
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Correlation of the highest-energy cosmic rays with nearby extragalactic objects.

2007

Using data collected at the Pierre Auger Observatory during the past 3.7 years, we demonstrated a correlation between the arrival directions of cosmic rays with energy above ~ 6x10^{19} electron volts and the positions of active galactic nuclei (AGN) lying within ~ 75 megaparsecs. We rejected the hypothesis of an isotropic distribution of these cosmic rays with at least a 99% confidence level from a prescribed a priori test. The correlation we observed is compatible with the hypothesis that the highest energy particles originate from nearby extragalactic sources whose flux has not been substantially reduced by interaction with the cosmic background radiation. AGN or objects having a similar…

Active galactic nucleus[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomyAstrophysics::High Energy Astrophysical Phenomenaparticle source [cosmic radiation]Cosmic background radiationFOS: Physical sciencesFluxOsservatorio Pierre AugerCosmic rayanisotropyAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Raggi cosmici0103 physical sciencesUltra-high-energy cosmic ray010303 astronomy & astrophysicsBackground radiationNuclei galattivi attiviPhysicsPierre Auger ObservatorySPECTRUMMultidisciplinary[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsMedicine (all); MultidisciplinaryMedicine (all)Settore FIS/01 - Fisica SperimentaleAstrophysics (astro-ph)angular dependence [cosmic radiation]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaEnergia ultra altaExperimental High Energy Physicsddc:500Energy (signal processing)experimental 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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The $^{144}$Ce source for SOX

2015

International audience; The SOX (Short distance neutrino Oscillations with BoreXino) project aims at testing the light sterile neutrino hypothesis. To do so, two artificials sources of antineutrinos and neutrinos respectively will be consecutively deployed at the Laboratori Nazionali del Gran Sasso (LNGS) in close vicinity to Borexino, a large liquid scintillator detector. This document reports on the source production and transportation. The source should exhibit a long lifetime and a high decay energy, a requirement fullfilled by the (144)Ce-(144)Pr pair at secular equilibrium. It will be produced at FSUE “Mayak” PA using spent nuclear fuel. It will then be shielded and packed according t…

HistorySterile neutrinoParticle physicsenergy: decay[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]Scintillator01 natural sciences7. Clean energyEducationNuclear physicsPhysics and Astronomy (all)0103 physical sciencesddc:530010306 general physicsNeutrino oscillationparticle sourceBorexinoPhysicslifetimenucleusSecular equilibriumneutrino: sterileantineutrinosensitivitySpent nuclear fuelComputer Science ApplicationsGran SassoceriumDecay energyradioactivityBorexinoneutrino: oscillationproductionNeutrino
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Solar neutrino detectors as sterile neutrino hunters

2016

International audience; The large size and the very low radioactive background of solar neutrino detectors such as Borexino at the Gran Sasso Laboratory in Italy offer a unique opportunity to probe the existence of neutrino oscillations into new sterile components by means of carefully designed and well calibrated anti-neutrino and neutrino artificial sources. In this paper we briefly summarise the key elements of the SOX experiment, a program for the search of sterile neutrinos (and other short distance effects) by means of a (144)Ce-(144)Pr anti-neutrino source and, possibly in the medium term future, with a (51)Cr neutrino source.

HistorySterile neutrinoParticle physicsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical Phenomena01 natural sciences7. Clean energyEducationPhysics and Astronomy (all)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex][PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationnuclideBorexinoPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemneutrino: sterileComputer Science ApplicationspraseodymiumGran Sassoneutrino: detectorNeutrino detectorcerium: nuclideHigh Energy Physics::Experimentneutrino: oscillationNeutrino astronomyNeutrinoantineutrino: particle source[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Effect of double frequency heating on the lead afterglow beam currents of an electron cyclotron resonance ion source

2017

International audience; The effect of double frequency heating on the performance of the CERN GTS-LHC 14.5 GHz ElectronCyclotron Resonance (ECR) ion source in afterglow mode is reported. The source of the secondary microwave frequency was operated both in pulsed and continuous wave (CW) modes within the range of 12–18 GHz. The results demonstrate that the addition of the secondary frequency can significantly impact the extracted beam currents and the temporal stability of the beam during the afterglow discharge. For example, up to a factor of 2.6 increase was achieved for 208Pb35+ and a factor of 3.1 for 208Pb37+ compared to single frequency afterglow currents. It is shown that these effect…

Nuclear and High Energy PhysicsMaterials scienceCERN LabPhysics and Astronomy (miscellaneous)Ion beam[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]Cyclotron resonancecyclotron: resonanceheating01 natural sciencesElectron cyclotron resonance010305 fluids & plasmasmicrowaves: frequencyplasma production0103 physical scienceslead: ionlcsh:Nuclear and particle physics. Atomic energy. Radioactivityparticle source010302 applied physicsta114beam: stabilityResonanceSurfaces and InterfacesAccelerators and Storage RingsIon sourceheavy ionAfterglowlcsh:QC770-798Atomic physicsMicrowaveIon cyclotron resonanceperformancePhysical Review Accelerators and Beams
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Atomic physics studies at the gamma factory at CERN

2020

The Gamma Factory initiative proposes to develop novel research tools at CERN by producing, accelerating and storing highly relativistic, partially stripped ion beams in the SPS and LHC storage rings. By exciting the electronic degrees of freedom of the stored ions with lasers, high-energy narrow-band photon beams will be produced by properly collimating the secondary radiation that is peaked in the direction of ions' propagation. Their intensities, up to $10^{17}$ photons per second, will be several orders of magnitude higher than those of the presently operating light sources in the particularly interesting $\gamma$--ray energy domain reaching up to 400 MeV. This article reviews opportuni…

Photonradiation: secondaryAtomic Physics (physics.atom-ph)atomic spectroscopyGeneral Physics and Astronomy02 engineering and technology01 natural sciences7. Clean energyPhysics - Atomic PhysicsHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)propagation[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]particle sourcePhysicsLarge Hadron Collidercollimatorhep-phsecondary beam021001 nanoscience & nanotechnologyion: excited stateLHC storage ringsHigh Energy Physics - PhenomenologyCERN LHC CollSPS storage rings0210 nano-technologyParticle Physics - ExperimentAccelerator Physics (physics.acc-ph)CERN LabOrders of magnitude (temperature)[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]gamma–ray productionOther Fields of PhysicsFOS: Physical sciencesAtomic spectroscopyion: beamgamma ray: burstpartially stripped ionsphysics.atom-phIonNuclear physics0103 physical sciencesddc:530010306 general physicsSpectroscopyphoton: beamphysics.acc-phParticle Physics - PhenomenologyAccelerator physicsparticle source: proposedhep-exCERN SPSAccelerators and Storage Rings[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]laser* Automatic Keywords *ion: storage ringatomic physics[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Physics::Accelerator PhysicsPhysics - Accelerator PhysicsStorage ring
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Comparison of ultracold neutron sources for fundamental physics measurements

2016

Ultracold neutrons (UCNs) are key for precision studies of fundamental parameters of the neutron and in searches for new CP violating processes or exotic interactions beyond the Standard Model of particle physics. The most prominent example is the search for a permanent electric dipole moment of the neutron (nEDM). We have performed an experimental comparison of the leading UCN sources currently operating. We have used a 'standard' UCN storage bottle with a volume of 32 liters, comparable in size to nEDM experiments, which allows us to compare the UCN density available at a given beam port.

Physics - Instrumentation and DetectorsPhysics beyond the Standard ModelFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciencesNuclear physics25.40Fq0103 physical sciencesCP: violationNeutron[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det][ PHYS.NEXP ] Physics [physics]/Nuclear Experiment [nucl-ex]Nuclear Experiment (nucl-ex)010306 general physicsNuclear Experiment[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear ExperimentPhysicsn: densityn: electric moment010308 nuclear & particles physics29.25.Dzn: particle sourceInstrumentation and Detectors (physics.ins-det)31.30.jn28.20.Pr3. Good healthFundamental physicsMoment (physics)14.20.DhUltracold neutronsNeutron sourceBeam (structure)
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Design of the Magnet System of the Neutron Decay Facility PERC

2018

The PERC (Proton and Electron Radiation Channel) facility is currently under construction at the research reactor FRM II, Garching. It will serve as an intense and clean source of electrons and protons from neutron beta decay for precision studies. It aims to contribute to the determination of the Cabibbo-Kobayashi-Maskawa quark-mixing element $V_{ud}$ from neutron decay data and to search for new physics via new effective couplings. PERC's central component is a 12m long superconducting magnet system. It hosts an 8m long decay region in a uniform field. An additional high-field region selects the phase space of electrons and protons which can reach the detectors and largely improves system…

Physics - Instrumentation and Detectorsmagnet: designProtonQC1-999FOS: Physical sciencesSuperconducting magnetElectron[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]01 natural sciences7. Clean energyelectron: particle sourcep: particle sourceNuclear physics0103 physical sciencesResearch reactorNeutron[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Nuclear Experiment (nucl-ex)010306 general physicsNuclear ExperimentPhysicsn: semileptonic decay010308 nuclear & particles physicsPhysicsInstrumentation and Detectors (physics.ins-det)magnet: superconductivityMagnetic fieldbeam opticsMagnetPhase spaceHigh Energy Physics::Experiment
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