Search results for "spectrum"

showing 10 items of 2043 documents

Licensed and Unlicensed Spectrum Management for Energy-Efficient Cognitive M2M

2020

Edge computing has emerged as a promising solution for relieving the tension between resource-limited MTDs and computational-intensive tasks. To realize successful task offloading with limited spectrum, we focus on the cognitive machine-to-machine (CM2M) paradigm which enables a massive number of MTDs to either opportunistically use the licensed spectrum that is temporarily available, or to exploit the under-utilized unlicensed spectrum. We formulate the channel selection problem with both licensed and unlicensed spectrum as an adversarial multi-armed bandit (MAB) problem, and combine the exponential-weight algorithm for exploration and exploitation (EXP3) and Lyapunov optimization to devel…

Exploitbusiness.industryComputer scienceReliability (computer networking)Lyapunov optimizationbusinessSelection algorithmSpectrum managementEdge computingCommunication channelEfficient energy useComputer network
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Light-component spectrum of the primary cosmic rays in the multi-TeV region measured by the ARGO-YBJ experiment

2012

The ARGO-YBJ experiment detects extensive air showers in a wide energy range by means of a full-coverage detector which is in stable data taking in its full configuration since November 2007 at the YBJ International Cosmic Ray Observatory (4300 m a.s.l., Tibet, People's Republic of China). In this paper the measurement of the light-component spectrum of primary cosmic rays in the energy region $(5\textdiv{}200)\text{ }\text{ }\mathrm{TeV}$ is reported. The method exploited to analyze the experimental data is based on a Bayesian procedure. The measured intensities of the light component are consistent with the recent CREAM results and higher than that obtained adding the proton and helium sp…

Extended Air Showers Cosmic Rays Gamma Ray sourcesNuclear and High Energy PhysicsProtonTIBETAstrophysics::High Energy Astrophysical PhenomenaExtensive air showerchemistry.chemical_elementCosmic rayHELIUM SPECTRAAstrophysicsPROTONBayesian methodCASCADESSpectral lineSettore FIS/05 - Astronomia E AstrofisicaNuclear magnetic resonanceCosmic-ray observatoryHeliumPhysicsRange (particle radiation)ENERGY-RANGEBALLOON EXPERIMENTNUCLEISettore FIS/01 - Fisica SperimentaleDetectorAstrophysics::Instrumentation and Methods for Astrophysicslight component spectrumchemistryEnergy (signal processing)SYSTEM
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Quantum mechanics-molecular dynamics approach to the interpretation of x-ray absorption spectra.

2009

The quantum mechanics-molecular dynamics approach to the simulation of configuration-averaged EXAFS spectra is proposed, and its application is discussed for the example of the Ti K-edge EXAFS spectrum in cubic perovskite SrTiO(3). Proper use of ab initio quantum mechanics allows a number of empirical parameters, used in the molecular dynamics simulation, to be reduced, whereas the molecular dynamics allows us to account for temperature effects. All together, the approach provides a way of accounting for static and dynamic disorder in EXAFS signals from the coordination shells above the first one, where many-atom (multiple-scattering) effects are often important.

Extended X-ray absorption fine structureAbsorption spectroscopyChemistrySpectrum (functional analysis)Ab initioCondensed Matter PhysicsSpectral lineCondensed Matter::Materials ScienceMolecular dynamicsCondensed Matter::SuperconductivityQuantum mechanicsGeneral Materials ScienceQuantumPerovskite (structure)Journal of physics. Condensed matter : an Institute of Physics journal
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Chanching the externalizing and internalizing spectrum of personality with self-regultaion therapy

2018

This article presents an integrator model of changes in the externalizing and internalizing factors of personality grouped in the General Factor of Personality (GFP), based on the Unique Trait Personality Theory (UTPT) [1]. This theory proposes that a continuum exists between personality and psychopathology, as well as the existence of a GFP that occupies the apex of the hierarchy of personality, and extends from an impulsiveness-and-aggressiveness pole (externalizing spectrum) to an anxiety-and-introversion pole (internalizing spectrum). With an experimental intra-group design, 30 regular users of stimulant drugs (cocaine and amphetamine) used the Self-Regulation Therapy (SRT). The SRT is …

Externalizing spectrummedicine.medical_treatmentmedia_common.quotation_subjectHierarchical structure of the Big FiveDevelopmental psychologySelf-Regulation TherapyUNESCO::FILOSOFÍA:FILOSOFÍA [UNESCO]medicinePersonalityAmphetaminemedia_commonRelaxation (psychology)Classical conditioningGeneral MedicineTerapèuticaGeneral Factor of PersonalityStimulantInternalizing spectrumTraitDroguesPersonalitatPsychologyMATEMATICA APLICADAStimulant drugs.medicine.drugPsychopathology
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Extrapolation of water and formaldehyde harmonic and anharmonic frequencies to the B3LYP/CBS limit using polarization consistent basis sets

2010

The harmonic and anharmonic frequencies of fundamental vibrations in formaldehyde and water were successfully estimated using the B3LYP Kohn-Sham limit. The results obtained with polarization- and correlation-consistent basis sets were fitted with a two-parameter formula. Anharmonic corrections were obtained by a second order perturbation treatment (PT2). We compared the performance of the PT2 scheme on the two title molecules using SCF, MP2 and DFT (BLYP, B3LYP, PBE and B3PW91 functionals) methods combined with polarization consistent pc-n (n = 0, 1, 2, 3, 4) basis sets, Dunning’s basis sets (aug)-cc-pVXZ where X = D, T, Q, 5, 6 and Pople’s basis sets up to 6-311++G(3df,2pd). The influence…

ExtrapolationPerturbation (astronomy)Sensitivity and SpecificityVibrationMolecular physicsCatalysisInorganic ChemistryRoot mean squareFormaldehydeQuantum mechanicsWavenumberIR and Raman theoretical spectraPhysics::Chemical PhysicsPhysical and Theoretical ChemistryBasis setOriginal PaperChemistrySpectrum AnalysisOrganic ChemistryAnharmonicityHarmonicReproducibility of ResultsWaterComplete basis set limitModels TheoreticalPolarization (waves)Computer Science ApplicationsVibrationComputational Theory and MathematicsAnharmonicJournal of Molecular Modeling
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Measurement of the cosmic ray energy spectrum using hybrid events of the Pierre Auger Observatory

2012

The energy spectrum of ultra-high energy cosmic rays above 10$^{18}$ eV is measured using the hybrid events collected by the Pierre Auger Observatory between November 2005 and September 2010. The large exposure of the Observatory allows the measurement of the main features of the energy spectrum with high statistics. Full Monte Carlo simulations of the extensive air showers (based on the CORSIKA code) and of the hybrid detector response are adopted here as an independent cross check of the standard analysis (Phys. Lett. B 685, 239 (2010)). The dependence on mass composition and other systematic uncertainties are discussed in detail and, in the full Monte Carlo approach, a region of confiden…

FLUORESCENCE DETECTORAstronomyAstrophysics::High Energy Astrophysical PhenomenaMonte Carlo methodenergy spectrumFOS: Physical sciencesGeneral Physics and AstronomyFluxCosmic rayEXTENSIVE AIR-SHOWERSSURFACE DETECTOR01 natural sciencesCosmic RayAugerPierre Auger Observatory ; Monte Carlo simulations ; ultra-high energy cosmic raysHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Observatory0103 physical sciencesRECONSTRUCTIONFermilab010306 general physicsUHE Cosmic Rays Monte Carlo Energy SpectrumTRIGGERNuclear PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPierre Auger ObservatoryPACS: 96.50.S 96.50.sb 96.50.sd 98.70.Sa010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Pierre Auger Observatory; Monte Carlo simulations; ultra-high energy cosmic raysPhysicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryPROFILES[PHYS.PHYS.PHYS-SPACE-PH]Physics [physics]/Physics [physics]/Space Physics [physics.space-ph]Experimental High Energy PhysicsSIMULATIONComputingMethodologies_DOCUMENTANDTEXTPROCESSINGARRAYFísica nuclearAstrophysics - High Energy Astrophysical PhenomenaRAIOS CÓSMICOS
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Search for relativistic magnetic monopoles with the ANTARES neutrino telescope

2012

Magnetic monopoles are predicted in various unified gauge models and could be produced at intermediate mass scales. Their detection in a neutrino telescope is facilitated by the large amount of light emitted compared to that from muons. This paper reports on a search for upgoing relativistic magnetic monopoles with the ANTARES neutrino telescope using a data set of 116 days of live time taken from December 2007 to December 2008. The one observed event is consistent with the expected atmospheric neutrino and muon background, leading to a 90% C.L. upper limit on the monopole flux between 1.3 ¿ 10¿17 and 8.9 ¿ 10¿17 cm¿2 s¿1 sr¿1 for monopoles with velocity ß ¿ 0.625.

FLUXMuon backgroundParticle physicsGauge modelMagnetic monopolesAstrophysics::High Energy Astrophysical PhenomenaMagnetic monopoleneutrino telescopes; antares; magnetic monopoleFOS: Physical sciencesCosmic ray01 natural sciencesNuclear physics0103 physical sciencesNeutronFIELD010306 general physicsDETECTORCherenkov radiationZenithHigh Energy Astrophysical Phenomena (astro-ph.HE)NeutronsPhysicsSPECTRUMAtmospheric neutrinosMagnetic monopoleANTARES:Física::Acústica [Àrees temàtiques de la UPC]MuonCharged particles010308 nuclear & particles physicsAstronomy and AstrophysicsMonopols magnèticsUpper limitsNeutrino detectorMass scaleFISICA APLICADA[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Física nuclearData setsNeutrino telescopes[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - High Energy Astrophysical PhenomenaEvent (particle physics)TelescopesAstroparticle Physics
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IceTop : the surface component of IceCube

2012

IceTop, the surface component of the IceCube Neutrino Observatory at the South Pole, is an air shower array with an area of 1 km2. The detector allows a detailed exploration of the mass composition of primary cosmic rays in the energy range from about 100 TeV to 1 EeV by exploiting the correlation between the shower energy measured in IceTop and the energy deposited by muons in the deep ice. In this paper we report on the technical design, construction and installation, the trigger and data acquisition systems as well as the software framework for calibration, reconstruction and simulation. Finally the first experience from commissioning and operating the detector and the performance as an …

FLUXNuclear and High Energy PhysicsAir showerPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaAir shower; Cosmic rays; Detector; IceCube; IceTopFOS: Physical sciencesCosmic rayddc:500.27. Clean energy01 natural sciencesIceCube Neutrino ObservatoryIceCubeShowerData acquisitioncosmic raysDIGITIZATION0103 physical sciencesSHOWERSCalibrationddc:530Instrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsInstrumentationCosmic raysRemote sensingPhysicsMuondetector010308 nuclear & particles physicsDetectorAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyDetectorENERGY-SPECTRUMAir showerPhysics and AstronomySIMULATIONIceTopHigh Energy Physics::ExperimentAstrophysics - Instrumentation and Methods for Astrophysics
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Constraints on ultra-high-energy cosmic ray sources from a search for neutrinos above 10 PeV with IceCube

2016

We report constraints on the sources of ultra-high-energy cosmic ray (UHECR) above $10^{9}$ GeV, based on an analysis of seven years of IceCube data. This analysis efficiently selects very high energy neutrino-induced events which have deposited energies from $\sim 10^6$ GeV to above $10^{11}$ GeV. Two neutrino-induced events with an estimated deposited energy of $(2.6 \pm 0.3) \times 10^6$ GeV, the highest neutrino energies observed so far, and $(7.7 \pm 2.0) \times 10^5$ GeV were detected. The atmospheric background-only hypothesis of detecting these events is rejected at 3.6$\sigma$. The hypothesis that the observed events are of cosmogenic origin is also rejected at $>$99% CL because of…

FLUXSELECTIONFERMI-LATActive galactic nucleusCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesCosmic rayAstrophysicsParameter space7. Clean energy01 natural sciencesCOSMOGENIC NEUTRINOS; TRACK RECONSTRUCTION; FERMI-LAT; BURSTS; SPECTRUM; MODEL; FLUX; TELESCOPES; SELECTION; EMISSIONPulsar0103 physical sciencesTRACK RECONSTRUCTIONBURSTSddc:550Ultrahigh energy010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)SPECTRUM010308 nuclear & particles physicsStar formationCOSMOGENIC NEUTRINOSAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyMODELPhysics and Astronomy13. Climate actionTELESCOPESHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaEMISSIONEnergy (signal processing)Astrophysics - Cosmology and Nongalactic Astrophysics
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Probing the origin of cosmic-rays with extremely high energy neutrinos using the IceCube Observatory

2013

We have searched for extremely high energy neutrinos using data taken with the IceCube detector between May 2010 and May 2012. Two neutrino induced particle shower events with energies around 1 PeV were observed, as reported previously. In this work, we investigate whether these events could originate from cosmogenic neutrinos produced in the interactions of ultra-high energy cosmic-rays with ambient photons while propagating through intergalactic space. Exploiting IceCube's large exposure for extremely high energy neutrinos and the lack of observed events above 100 PeV, we can rule out the corresponding models at more than 90% confidence level. The model independent quasi-differential 90% …

FLUXSELECTIONFERMI-LATNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)PhotonRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayddc:500.2AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsLIMIT01 natural sciencesIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Particle showerObservatory0103 physical sciencesddc:530010306 general physicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMRange (particle radiation)COSMOGENIC NEUTRINOS010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomyPERFORMANCECOMPONENTMODELPhysics and Astronomy13. Climate actionIntergalactic travelHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaSYSTEMAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review D
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