Search results for "detectors"

showing 10 items of 2229 documents

Physics results from the Amanda neutrino detector

2001

In the winter season of 2000, the AMANDA (Antarctic Muon And Neutrino Detector Array) detector was completed to its final state. We report on major physics results obtained from the AMANDA-B10 detector, as well as initial results of the full AMANDA-II detector.

Astroparticle physicsPhysicsParticle physicsMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDetectorSolar neutrino problemNuclear physicsNeutrino detectorHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyNeutrino oscillationPhysics::Atmospheric and Oceanic PhysicsParticle Physics - Phenomenology
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Limits to the muon flux from neutralino annihilations in the Sun with the AMANDA detector

2005

A search for an excess of muon-neutrinos from neutralino annihilations in the Sun has been performed with the AMANDA-II neutrino detector using data collected in 143.7 days of live-time in 2001. No excess over the expected atmospheric neutrino background has been observed. An upper limit at 90% confidence level has been obtained on the annihilation rate of captured neutralinos in the Sun, as well as the corresponding muon flux limit at the Earth, both as functions of the neutralino mass in the range 100 GeV-5000 GeV.

Astroparticle physicsPhysicsParticle physicsRange (particle radiation)AMANDAMuonPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaDetectorDark matterHigh Energy Physics::PhenomenologyAstrophysics (astro-ph)NeutralinoFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAMANDA; Dark matter; Neutralino; Neutrino telescopesNuclear physicsNeutrino detectorNeutralinoMuon fluxDark matterHigh Energy Physics::ExperimentNeutrino telescopes
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Topological track reconstruction in unsegmented, large-volume liquid scintillator detectors

2018

Unsegmented, large-volume liquid scintillator (LS) neutrino detectors have proven to be a key technology for low-energy neutrino physics. The efficient rejection of radionuclide background induced by cosmic muon interactions is of paramount importance for their success in high-precision MeV neutrino measurements. We present a novel technique to reconstruct GeV particle tracks in LS, whose main property, the resolution of topological features and changes in the differential energy loss $\mathrm{d}E/\mathrm{d}x$, allows for improved rejection strategies. Different to common track reconstruction approaches, our method does not rely on concrete track / topology hypotheses. Instead, based on a r…

Astroparticle physicsPhysicsPhysics - Instrumentation and DetectorsPhotonMuonPhysics::Instrumentation and Detectors010308 nuclear & particles physicsDetectorFOS: Physical sciencesInstrumentation and Detectors (physics.ins-det)ScintillatorTopology01 natural sciencesNeutrino detector0103 physical sciencesHigh Energy Physics::ExperimentNeutrino010306 general physicsInstrumentationImage resolutionMathematical PhysicsJournal of Instrumentation
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Does the Sun Shine byppor CNO Fusion Reactions?

2002

We show that solar neutrino experiments set an upper limit of 7.8% (7.3% including the recent KamLAND measurements) to the fraction of energy that the Sun produces via the CNO fusion cycle, which is an order of magnitude improvement upon the previous limit. New experiments are required to detect CNO neutrinos corresponding to the 1.5% of the solar luminosity that the standard solar model predicts is generated by the CNO cycle.

Astrophysics and AstronomyAstrofísica nuclearCNO cycleNuclear TheoryPhysics::Instrumentation and DetectorsSolar neutrinoSolar luminosityFOS: Physical sciencesGeneral Physics and AstronomyAstrophysicsAstrophysics7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear Theory (nucl-th)High Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsNuclear fusionNuclear Experiment (nucl-ex)010306 general physicsNeutrino oscillationNuclear ExperimentAstrophysics::Galaxy AstrophysicsPhysicsStandard solar modelReaccions nuclears010308 nuclear & particles physicsAstrophysics (astro-ph)FísicaHigh Energy Physics - PhenomenologyPhysics::Space PhysicsNuclear astrophysicsHigh Energy Physics::ExperimentNuclear reactionsNeutrinoOrder of magnitudePhysical Review Letters
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Prospects for discovering supersymmetric long-lived particles with MoEDAL

2020

We present a study on the possibility of searching for long-lived supersymmetric partners with the MoEDAL experiment at the LHC. MoEDAL is sensitive to highly ionising objects such as magnetic monopoles or massive (meta)stable electrically charged particles. We focus on prospects of directly detecting long-lived sleptons in a phenomenologically realistic model which involves an intermediate neutral long-lived particle in the decay chain. This scenario is not yet excluded by the current data from ATLAS or CMS, and is compatible with astrophysical constraints. Using Monte Carlo simulation, we compare the sensitivities of MoEDAL versus ATLAS in scenarios where MoEDAL could provide discovery re…

Astrophysics and AstronomyParticle physicsPhysics and Astronomy (miscellaneous)Regular Article - Experimental PhysicsPhysics::Instrumentation and DetectorsMagnetic monopoleFOS: Physical scienceslcsh:AstrophysicsElementary particle01 natural sciencesHigh Energy Physics - ExperimentParticle decayHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)lcsh:QB460-4660103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityInvariant mass010306 general physicsEngineering (miscellaneous)Particle Physics - Phenomenologyastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Large Hadron Colliderhep-ex010308 nuclear & particles physicsSuperpartnerhep-phSupersymmetryHigh Energy Physics - PhenomenologyMoEDAL experimentlcsh:QC770-798Astrophysics - High Energy Astrophysical PhenomenaParticle Physics - ExperimentEuropean Physical Journal
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High magnetic fields for fundamental physics

2018

Various fundamental-physics experiments such as measurement of the birefringence of the vacuum, searches for ultralight dark matter (e.g., axions), and precision spectroscopy of complex systems (including exotic atoms containing antimatter constituents) are enabled by high-field magnets. We give an overview of current and future experiments and discuss the state-of-the-art DC- and pulsed-magnet technologies and prospects for future developments.

Astrophysics and AstronomyPhysics - Instrumentation and Detectorsmagnet: designmagnetic field: highAtomic Physics (physics.atom-ph)AxionsDark matterComplex systemOther Fields of PhysicsFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesphysics.atom-phNOPhysics - Atomic PhysicsNuclear physicsPhysics and Astronomy (all)Neutrino mass0103 physical sciencesDark matter[ PHYS.PHYS.PHYS-GEN-PH ] Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Axions; Dark matter; High-field magnets; Neutrino mass; Spectroscopy; Vacuum birefringence; Physics and Astronomy (all)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Detectors and Experimental Techniques010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Axionphysics.ins-detSpectroscopyactivity reportExotic atomPhysicsVacuum birefringence010308 nuclear & particles physicsInstrumentation and Detectors (physics.ins-det)Polarization (waves)magnet: technology[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]3. Good healthMagnetic fieldHigh-field magnetsAntimatterMagnetAstrophysics - Instrumentation and Methods for Astrophysicsastro-ph.IM
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Probing secret interactions of eV-scale sterile neutrinos with the diffuse supernova neutrino background

2020

Sterile neutrinos with mass in the eV-scale and large mixings of order $\theta_0\simeq 0.1$ could explain some anomalies found in short-baseline neutrino oscillation data. Here, we revisit a neutrino portal scenario in which eV-scale sterile neutrinos have self-interactions via a new gauge vector boson $\phi$. Their production in the early Universe via mixing with active neutrinos can be suppressed by the induced effective potential in the sterile sector. We study how different cosmological observations can constrain this model, in terms of the mass of the new gauge boson, $M_\phi$, and its coupling to sterile neutrinos, $g_s$. Then, we explore how to probe part of the allowed parameter spa…

Astrophysics and AstronomySterile neutrinoParticle physicsScale (ratio)Physics::Instrumentation and Detectorsmedia_common.quotation_subjectPhysics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)Big Bang nucleosynthesis0103 physical sciencesNeutrino oscillation010303 astronomy & astrophysicsParticle Physics - Phenomenologymedia_commonastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Gauge boson010308 nuclear & particles physicsHigh Energy Physics::Phenomenologyhep-phAstronomy and AstrophysicsUniverse3. Good healthSupernovaHigh Energy Physics - PhenomenologyHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Combined search for the Standard Model Higgs boson using up to 4.9 fb-1 of pp collision data at √(s)=7 TeV with the ATLAS detector at the LHC

2012

A combined search for the Standard Model Higgs boson with the ATLAS experiment at the LHC using datasets corresponding to integrated luminosities from 1.04 fb(-1) to 4.9 fb(-1) of pp collisions collected at root s = 7 TeV is presented. The Higgs boson mass ranges 112.9-115.5 GeV, 131-238 GeV and 251-466 GeV are excluded at the 95% confidence level (CL), while the range 124-519 GeV is expected to be excluded in the absence of a signal. An excess of events is observed around m(H) similar to 126 GeV with a local significance of 3.5 standard deviations (sigma). The local significances of H -> gamma, H -> ZZ(()*()) -> l(+)l(-)l'(+)l'(-) and H -> WW(*()) l(+)nu l'(-)(nu) over bar, the three most …

Astrophysics::High Energy Astrophysical PhenomenaAcceleradors de partículesCol·lisions (Física nuclear)High Energy Physics::ExperimentPartícules (Física nuclear)Detectors de radiació
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Combined search for the Standard Model Higgs boson in pp collisions at root s=7 TeV with the ATLAS detector

2012

A combined search for the Standard Model Higgs boson with the ATLAS detector at the LHC is presented. The data sets used correspond to integrated luminosities from 4.6 fb(-1) to 4.9 fb(-1) of proton-proton collisions collected at root s = 7 TeV in 2011. The Higgs boson mass ranges of 111.4 GeV to 116.6 GeV, 119.4 GeV to 122.1 GeV, and 129.2 GeV to 541 GeV are excluded at the 95% confidence level, while the range 120 GeV to 560 GeV is expected to be excluded in the absence of a signal. An excess of events is observed at Higgs boson mass hypotheses around 126 GeV with a local significance of 2.9 standard deviations (sigma). The global probability for the background to produce an excess at lea…

Astrophysics::High Energy Astrophysical PhenomenaAcceleradors de partículesCol·lisions (Física nuclear)High Energy Physics::PhenomenologyHigh Energy Physics::ExperimentNuclear ExperimentPartícules (Física nuclear)Detectors de radiació
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Observation of a new particle in the search for the Standard Model Higgs boson with the ATLAS detector at the LHC

2012

A search for the Standard Model Higgs boson in proton-proton collisions with the ATLAS detector at the LHC is presented. The datasets used correspond to integrated luminosities of approximately 4.8 fb(-1) collected at, root s = 7 TeV in 2011 and 5.8 fb(-1) at root s = 8 TeV in 2012. Individual searches in the channels H -> ZZ(()*()) -> 4l, H -> gamma gamma and H -> WW (()*()) -> ev μv in the 8 TeV data are combined with previously published results of searches for H -> ZZ(()*()), WW(*()), b (b) over bar and tau(+)tau(-) in the 7 TeV data and results from improved analyses of the H -> ZZ(()*()) -> 4l and H -> gamma gamma channels in the 7 TeV data. Clear evidence for the production of a neut…

Astrophysics::High Energy Astrophysical PhenomenaAcceleradors de partículesCol·lisions (Física nuclear)High Energy Physics::PhenomenologyHigh Energy Physics::ExperimentPartícules (Física nuclear)Detectors de radiació
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