Search results for " nuclear"

showing 10 items of 11776 documents

Electrical conductivity of glass fiber-reinforced plastic with nanomodified matrix for damage diagnostic

2021

The electrical conductivity of glass fiber-reinforced plastic (GFRP) with epoxy matrix modified by multiwall carbon nanotubes (MWCNT) was studied. The electrical conductivity of nanomodified lamina and multi-layered GFRP was investigated on several levels using a structural approach. Components of the electrical conductivity tensor for unidirectional-reinforced monolayer were calculated similarly as in micromechanics using the conductivity of the nanomodified matrix. The electrical conductivity of multilayer composite was calculated using laminate theory and compared with values measured experimentally for various fiber orientation angles. Calculated and experimental data were in good agree…

voltage distributionTechnologyMaterials scienceGlass fiberCarbon nanotubeConductivityArticlelaw.inventionFracture toughnessmicromechanicsElectrical resistance and conductancelawGeneral Materials ScienceComposite materialinterlaminar fractureMicroscopyQC120-168.85carbon nanotubeselectrical conductivityTQH201-278.5glass fiber reinforced plasticMicromechanicsFracture mechanicsdamage diagnosticFibre-reinforced plasticEngineering (General). Civil engineering (General)TK1-9971Descriptive and experimental mechanicsElectrical engineering. Electronics. Nuclear engineeringTA1-2040
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Few-body insights of multiquark exotic hadrons

2018

In this contribution we discuss the adequate treatment of the $4-$ and $5-$body dynamics within a constituent quark framework. We stress that the variational and Born-Oppenheimer approximations give energies rather close to the exact ones, while the diquark approximation might be rather misleading. Hall-Post inequalities provide very useful lower bounds that exclude possible stable states for some mass ratios and color wave functions.

wave functionhadron: exoticBorn–Oppenheimer approximationConstituent quarkFOS: Physical sciences01 natural sciencesStability (probability)symbols.namesakeTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)multiquarkquark: constituent0103 physical sciences010306 general physicsWave functionBorn-Oppenheimer approximationStable statePhysics010308 nuclear & particles physicsExotic hadronMass ratiostabilityDiquarkHigh Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]symbolsapproximation: diquarkmass ratio
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IEEE Access Special Section Editorial: Exploiting the Benefits of Interference in Wireless Networks: Energy Harvesting and Security

2018

Interference used to be viewed as a harmful factor in wireless networks, which can reduce the quality of information transmission. To combat against interference, many interference management techniques have emerged. Due to the latest research advances, interference (or noise) can also be exploited to offer some benefits to wireless networks. The first aspect is that interference in multi-user networks can be collected as a green power supply for the transceivers, known as wireless energy harvesting. Another application is that one can generate artificial noise to disrupt the adversarial eavesdropping, and guarantee the security of wireless networks. Therefore, conventional interference man…

wireless networksGeneral Computer ScienceComputer sciencenoise (radio technology)ComputerApplications_COMPUTERSINOTHERSYSTEMShäiriötInterference (communication)General Materials Sciencekohinakyberturvallisuusta213Wireless networkbusiness.industryComputerSystemsOrganization_COMPUTER-COMMUNICATIONNETWORKSGeneral EngineeringEavesdroppingTransmission (telecommunications)interferenceslcsh:Electrical engineering. Electronics. Nuclear engineeringTransceiverbusinessenergiantuotantolcsh:TK1-9971Energy harvestinglangattomat verkotComputer networkIEEE Access
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Underwater Multirobot Cooperative Intervention MAC Protocol

2020

This work introduces a Medium Access Control (MAC) protocol designed to allow a group of underwater robots that share a wireless communication channel to effectively communicate with each other. The goal of the Underwater Multirobot Cooperative Intervention MAC (UMCI-MAC) protocol presented in this work is to minimize the end to end delay and the jitter. The access to the medium in UMCI-MAC follows a Time Division Multiple Access (TDMA) strategy which is arbitrated by a master, which also has the capability to prioritize the transmission of some nodes over the rest of the network. Two experiments have been carried out with a team of four Autonomous Underwater Vehicles (AUV) in order to comp…

wireless networksaccess protocolsGeneral Computer ScienceComputer scienceUnderwater communicationsEnd-to-end delayTime division multiple accessThroughput02 engineering and technologyteleroboticsTelecomunicació0203 mechanical engineering0202 electrical engineering electronic engineering information engineeringWirelessGeneral Materials ScienceJitterbusiness.industryNetwork packetWireless networkComputerSystemsOrganization_COMPUTER-COMMUNICATIONNETWORKSGeneral Engineering020302 automobile design & engineering020206 networking & telecommunicationsApplication layerunderwater communicationslcsh:Electrical engineering. Electronics. Nuclear engineeringremotely operated vehiclesbusinessCommunications protocolRobotsProtocols de xarxes d'ordinadorslcsh:TK1-9971Underwater acoustic communicationComputer networkCommunication channelIEEE Access
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The Large Observatory For x-ray Timing

2014

The Large Observatory For x-ray Timing (LOFT) was studied within ESA M3 Cosmic Vision framework and participated in the final down-selection for a launch slot in 2022-2024. Thanks to the unprecedented combination of effective area and spectral resolution of its main instrument, LOFT will study the behaviour of matter under extreme conditions, such as the strong gravitational field in the innermost regions of accretion flows close to black holes and neutron stars, and the supra-nuclear densities in the interior of neutron stars. The science payload is based on a Large Area Detector (LAD, 10 m 2 effective area, 2-30 keV, 240 eV spectral resolution, 1 deg collimated field of view) and a WideFi…

x-ray and γ-ray instrumentationcompact objects; microchannel plates; X-ray detectors; X-ray imaging; X-ray spectroscopy; X-ray timing; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringVisionX-ray timingObservatoriesField of view01 natural sciences7. Clean energyneutron starsObservatory010303 astronomy & astrophysicsPhysicsEquipment and servicesApplied MathematicsAstrophysics::Instrumentation and Methods for AstrophysicsSteradian[ SDU.ASTR.IM ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Computer Science Applications1707 Computer Vision and Pattern RecognitionX-ray detectorsCondensed Matter Physicscompact objectsX-ray spectroscopyAstrophysics - Instrumentation and Methods for AstrophysicsX-ray detector[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Cosmic VisionSpectral resolutionmicrochannel platesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesNOmicrochannel platecompact objects; microchannel plates; X-ray detectors; X-ray imaging; X-ray spectroscopy; X-ray timing; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Applied Mathematics; Electrical and Electronic EngineeringSettore FIS/05 - Astronomia e AstrofisicaX-rayscompact object0103 physical sciencesElectronicOptical and Magnetic MaterialsElectrical and Electronic EngineeringSpectral resolutionInstrumentation and Methods for Astrophysics (astro-ph.IM)dense hadronic matterSensors010308 nuclear & particles physicsX-ray imagingAstronomyAccretion (astrophysics)[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Neutron star13. Climate actionx-ray and γ-ray instrumentation; neutron stars; dense hadronic matter[ PHYS.ASTR.IM ] Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Gamma-ray burstastro-ph.IM
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The XENON1T Dark Matter Experiment

2017

The XENON1T experiment at the Laboratori Nazionali del Gran Sasso (LNGS) is the first WIMP dark matter detector operating with a liquid xenon target mass above the ton-scale. Out of its 3.2 t liquid xenon inventory, 2.0 t constitute the active target of the dual-phase time projection chamber. The scintillation and ionization signals from particle interactions are detected with low-background photomultipliers. This article describes the XENON1T instrument and its subsystems as well as strategies to achieve an unprecedented low background level. First results on the detector response and the performance of the subsystems are also presented. © 2017, The Author(s).

xenon: targetPhotomultiplierCosmology and Nongalactic Astrophysics (astro-ph.CO)Physics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)WIMP[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Dark matterchemistry.chemical_elementFOS: Physical scienceslcsh:Astrophysics01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)XENONXenonbackground: lowWIMP[ PHYS.HEXP ] Physics [physics]/High Energy Physics - Experiment [hep-ex]Ionization0103 physical scienceslcsh:QB460-466[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark Matterlcsh:Nuclear and particle physics. Atomic energy. Radioactivity[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsEngineering (miscellaneous)Instrumentation and Methods for Astrophysics (astro-ph.IM)[ PHYS.PHYS.PHYS-INS-DET ] Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]AstrophysiquePhysicsScintillationxenon: liquidTime projection chamberphotomultiplier010308 nuclear & particles physicsDetectorInstrumentation and Detectors (physics.ins-det)dark matter: detectortime projection chamberchemistrylcsh:QC770-798TPCAstrophysics - Instrumentation and Methods for Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]performanceAstrophysics - Cosmology and Nongalactic AstrophysicsEuropean Physical Journal C
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Search for inelastic scattering of WIMP dark matter in XENON1T

2021

We report the results of a search for the inelastic scattering of weakly interacting massive particles (WIMPs) in the XENON1T dark matter experiment. Scattering off $^{129}$Xe is the most sensitive probe of inelastic WIMP interactions, with a signature of a 39.6 keV de-excitation photon detected simultaneously with the nuclear recoil. Using an exposure of 0.89 tonne-years, we find no evidence of inelastic WIMP scattering with a significance of more than 2$\sigma$. A profile-likelihood ratio analysis is used to set upper limits on the cross-section of WIMP-nucleus interactions. We exclude new parameter space for WIMPs heavier than 100 GeV/c${}^2$, with the strongest upper limit of $3.3 \time…

xenon: targetPhotonPhysics::Instrumentation and DetectorsParameter space01 natural sciencesWIMP: dark matterHigh Energy Physics - Experiment; High Energy Physics - Experiment; astro-ph.COHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)XENONRecoilWIMPWIMP nucleus: cross section[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark Matterparameter spaceNuclear ExperimentComputingMilieux_MISCELLANEOUSnucleus: recoilPhysicsDark Matter Inelastic scattering XENON Direct Dark MatterPhysicsphotonAstrophysics::Instrumentation and Methods for AstrophysicsDirect Dark MatterWeakly interacting massive particlesastro-ph.COsignatureAstrophysics - Cosmology and Nongalactic AstrophysicsParticle physicsInelastic scatteringCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterFOS: Physical sciencesWIMP: massAstrophysics::Cosmology and Extragalactic AstrophysicsInelastic scatteringNOPE2_2PE2_10103 physical sciencesddc:530010306 general physics010308 nuclear & particles physicsScatteringWIMP nucleus: interactionDarkmatterWIMP: interactionHigh Energy Physics::Experiment[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics and astroparticle physicsexperimental resultsPhysical Review D. Particles, Fields, Gravitation, and Cosmology
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Search for Light Dark Matter Interactions Enhanced by the Migdal Effect or Bremsstrahlung in XENON1T.

2019

Direct dark matter detection experiments based on a liquid xenon target are leading the search for dark matter particles with masses above ∼5 GeV/c2, but have limited sensitivity to lighter masses because of the small momentum transfer in dark matter-nucleus elastic scattering. However, there is an irreducible contribution from inelastic processes accompanying the elastic scattering, which leads to the excitation and ionization of the recoiling atom (the Migdal effect) or the emission of a bremsstrahlung photon. In this Letter, we report on a probe of low-mass dark matter with masses down to about 85 MeV/c2 by looking for electronic recoils induced by the Migdal effect and bremsstrahlung us…

xenon: targetPhysics - Instrumentation and Detectorsdark matter: interactionelastic scatteringGeneral Physics and Astronomy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)XenonIonizationexcited state[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Nuclear ExperimentLight dark matterElastic scatteringPhysicsxenon: liquidatommomentum transferMomentum transferBremsstrahlungInstrumentation and Detectors (physics.ins-det)photon: bremsstrahlungS030DN5Weakly interacting massive particlesExcited stateAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Dark matterLight Dark Matter Direct search Liquid Xenon TPCFOS: Physical sciencesS030DI5chemistry.chemical_elementNuclear physicsParticle dark matterrecoilionization0103 physical sciencesDark matter[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsscintillation counterS030DP5010308 nuclear & particles physicsdown: masssensitivityDark matter Particle dark matter Weakly interacting massive particles* Automatic Keywords *chemistryElementary Particles and Fieldsbremsstrahlung: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Physical review letters
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XENON1T Dark Matter Data Analysis: Signal Reconstruction, Calibration and Event Selection

2019

The XENON1T experiment at the Laboratori Nazionali del Gran Sasso is the most sensitive direct detection experiment for dark matter in the form of weakly interacting particles (WIMPs) with masses above $6\,$GeV/$c^2$ scattering off nuclei. The detector employs a dual-phase time projection chamber with 2.0 metric tons of liquid xenon in the target. A one metric $\mathrm{ton}\times\mathrm{year}$ exposure of science data was collected between October 2016 and February 2018. This article reports on the performance of the detector during this period and describes details of the data analysis that led to the most stringent exclusion limits on various WIMP-nucleon interaction models to date. In pa…

xenon: targetWIMP nucleon: interactiondata analysis methodPhysics - Instrumentation and Detectorsinteraction: modelPhysics::Instrumentation and DetectorsDark matterchemistry.chemical_elementFOS: Physical sciencesdark matter: direct detection01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)XENONXenon0103 physical sciencesCalibration[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Dark MatterParticle Physics Experiments[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear ExperimentDark Matter Direct Search Signal reconstruction calibratiuonPhysicsxenon: liquidTime projection chamber010308 nuclear & particles physicsScatteringSignal reconstructionDetectorAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)calibrationtime projection chamberEvent selectionchemistryHigh Energy Physics::Experimentperformance
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Excess electronic recoil events in XENON1T

2020

We report results from searches for new physics with low-energy electronic recoil data recorded with the XENON1T detector. With an exposure of 0.65 t-y and an unprecedentedly low background rate of $76\pm2$ events/(t y keV) between 1 and 30 keV, the data enables sensitive searches for solar axions, an enhanced neutrino magnetic moment, and bosonic dark matter. An excess over known backgrounds is observed at low energies and most prominent between 2 and 3 keV. The solar axion model has a 3.4$\sigma$ significance, and a 3D 90% confidence surface is reported for axion couplings to electrons, photons, and nucleons. This surface is inscribed in the cuboid defined by $g_{ae}<3.8 \times 10^{-12}$,…

xenon: targetaxionssolar axionmagnetic momentdimension: 3neutrino: solarPhysics beyond the Standard ModelSolar neutrinodark matter: direct detection01 natural sciences7. Clean energyHigh Energy Physics - ExperimentDark matter direct detection axionHigh Energy Physics - Experiment (hep-ex)neutrinoXENONHigh Energy Physics - Phenomenology (hep-ph)background: lowRecoilelectron: recoil[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]beta-raysParticle Physics Experimentscoupling: (axion 2electron)multi-purpose particle detectornuclear instrumentationComputingMilieux_MISCELLANEOUSinstrumentationPhysicsxenon: liquidboson: dark matteraxion 2nucleontritiumnew physics: search forsemileptonic decayboson: vectortensionneutrino: magnetic momentHigh Energy Physics - Phenomenologyaxion 2photonlow backgroundbosonNeutrinoionizing radiationNucleonAstrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)dark matter detectorelectronic recoilElectron captureXENON1T detectorDark matterlow-energy electronic recoil dataFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]dark matterNONuclear physicsPE2_2PE2_1tritium: semileptonic decay0103 physical sciencessolar axion modelsurface[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]axion: couplingPE2_4010306 general physicspseudoscalarAxiondark matter: vectordark matter XENON1T detector electronic recoilsolar neutrinodetectorDark Matter Axions Beta Decay Liquid Xenon TPC010308 nuclear & particles physicsaxion 2electroncoupling: (axion 2nucleon)dark matter: detectormodel: axionGran Sassometrology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]axionstellar constraintscoupling: (axion 2photon)High Energy Physics::Experimentparticle dark matterdirect detectionbeta decayaxion: solar[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]experimental results
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