Search results for "Galaxy Astrophysics"

showing 10 items of 1297 documents

Extinction risk under coloured environmental noise

2000

Positively autocorrelated red environmental noise is characterized by a strong dependence of expected sample variance on sample length. This dependence has to be taken into account when assessing extinction risk under red and white uncorrelated environmental noise. To facilitate a comparison between red and white noise, their expected variances can be scaled to be equal, but only at a chosen time scale. We show with a simple one-dimensional population dynamics model that the different but equally reasonable choices of the time scale yield qualitatively different results on the dependence of extinction risk on the colour of environmental noise: extinction risk might increase as well as decre…

0106 biological sciences0303 health scienceseducation.field_of_studyExtinctionScale (ratio)EcologyAutocorrelationPopulationWhite noiseBiological Sciences010603 evolutionary biology01 natural sciences010601 ecology03 medical and health sciencesNoiseStatisticsSample varianceeducationEnvironmental noiseAstrophysics::Galaxy AstrophysicsEcology Evolution Behavior and Systematics030304 developmental biologyMathematicsEcography
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Giant, unconventional anomalous Hall effect in the metallic frustrated magnet candidate, KV 3 Sb 5

2020

The anomalous Hall effect soars when Dirac quasiparticles meet frustrated magnetism.

02 engineering and technology01 natural sciencesCondensed Matter::Materials ScienceHall effectCondensed Matter::Superconductivity0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physicsAstrophysics::Galaxy AstrophysicsResearch ArticlesPhysicsMultidisciplinaryCondensed matter physicsScatteringDirac (video compression format)PhysicsSciAdv r-articles021001 nanoscience & nanotechnologyCondensed Matter::Mesoscopic Systems and Quantum Hall EffectSemimetalFerromagnetismMagnetQuasiparticleSpin Hall effectCondensed Matter::Strongly Correlated Electrons0210 nano-technologyResearch ArticleScience Advances
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Impact of accumulated dust particles' charge on the photovoltaic module performance

2016

Abstract This work is focused on analysing effect of accumulated dust particles' charge on PV module performance. In the Dundee University's laboratory, dust particles have been created through epoxy powder and charged by using corona and tribo-electric charging methods by varying the charge levels of the accumulated dust particles. The PV module output has analysed for finding a relation between charge levels of the accumulated dust particles and its output voltage. Obtained experimental results have shown that charge level of accumulated dust particles on PV module's have significant impact on its output and dust particle accumulations are not associated with panel tilt angle.

020209 energyDust particlesAstrophysics::Cosmology and Extragalactic Astrophysics02 engineering and technology010501 environmental sciencescomplex mixtures01 natural sciencesCorona (optical phenomenon)0202 electrical engineering electronic engineering information engineeringAstrophysics::Solar and Stellar AstrophysicsElectrical and Electronic EngineeringAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsbusiness.industryPhotovoltaic systemElectrical engineeringCharge (physics)Condensed Matter PhysicsElectrostaticsrespiratory tract diseasesSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsComputational physicsParticleAstrophysics::Earth and Planetary AstrophysicsbusinessBiotechnologyVoltageJournal of Electrostatics
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"Table 1" of "Observation and measurement of forward proton scattering in association with lepton pairs produced via the photon fusion mechanism at A…

2022

The measured fiducial cross sections. The first systematic uncertainty is the combined systematic uncertainty excluding luminosity, the second is the luminosity

13000.0Astrophysics::High Energy Astrophysical PhenomenaIntegrated Cross SectionAstrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIGlepton pair productionInclusiveProton-Proton ScatteringP P --> L+ L- P Xphoton-photon fusionAstrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentAstrophysics::Galaxy Astrophysics
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"Table 3" of "Measurement of the $ZZ$ Production Cross Section in $pp$ Collisions at $\sqrt{s}$ = 13 TeV with the ATLAS Detector"

2016

Measured fiducial cross section in the $\mu^+\mu^-\mu^+\mu^-$ channel. The first systematic uncertainty is the combined systematic uncertainty excluding luminosity uncertainty, the second is the luminosity uncertainty.

13000.0Z ProductionAstrophysics::High Energy Astrophysical PhenomenaP P --> Z0 Z0 XIntegrated Cross SectionAstrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIGMuon productionInclusiveProton-Proton ScatteringAstrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentZ pair ProductionAstrophysics::Galaxy Astrophysics
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"Table 1" of "Measurement of the $ZZ$ Production Cross Section in $pp$ Collisions at $\sqrt{s}$ = 13 TeV with the ATLAS Detector"

2016

Measured fiducial cross section in the $e^+e^-e^+e^-$ channel. The first systematic uncertainty is the combined systematic uncertainty excluding luminosity uncertainty, the second is the luminosity uncertainty.

13000.0Z ProductionElectron productionAstrophysics::High Energy Astrophysical PhenomenaP P --> Z0 Z0 XIntegrated Cross SectionAstrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIGInclusiveProton-Proton ScatteringAstrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentZ pair ProductionAstrophysics::Galaxy Astrophysics
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"Table 2" of "Measurement of the $ZZ$ Production Cross Section in $pp$ Collisions at $\sqrt{s}$ = 13 TeV with the ATLAS Detector"

2016

Measured fiducial cross section in the $e^+e^-\mu^+\mu^-$ channel. The first systematic uncertainty is the combined systematic uncertainty excluding luminosity uncertainty, the second is the luminosity uncertainty.

13000.0Z ProductionElectron productionAstrophysics::High Energy Astrophysical PhenomenaP P --> Z0 Z0 XIntegrated Cross SectionAstrophysics::Cosmology and Extragalactic AstrophysicsCross SectionSIGMuon productionInclusiveProton-Proton ScatteringAstrophysics::Solar and Stellar AstrophysicsHigh Energy Physics::ExperimentZ pair ProductionAstrophysics::Galaxy Astrophysics
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"Table 3" of "Measurement of inclusive jet and dijet cross sections in proton-proton collisions at 7 TeV centre-of-mass energy with the ATLAS detecto…

2010

Inclusive jet double-differential cross sections in the |rapidity| range 0.8 to 1.2, using a jet resolution R value of 0.4. The three (sys) errors are respectively, the Absolute JES, the Unfolding and the Luminosity uncertainties.

26119402611940Astrophysics::High Energy Astrophysical PhenomenaRapidity Dependence7000.0Astrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionP P --> JET XInclusiveProton-Proton ScatteringHigh Energy Physics::ExperimentD2SIG/DPT/DYRAPTransverse Momentum DependenceDouble Differential Cross SectionAstrophysics::Galaxy Astrophysics
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"Table 8" of "Measurement of inclusive jet and dijet cross sections in proton-proton collisions at 7 TeV centre-of-mass energy with the ATLAS detecto…

2010

Inclusive jet double-differential cross sections in the |rapidity| range 0.8 to 1.2, using a jet resolution R value of 0.6. The three (sys) errors are respectively, the Absolute JES, the Unfolding and the Luminosity uncertainties.

26119402611940Astrophysics::High Energy Astrophysical PhenomenaRapidity Dependence7000.0Astrophysics::Cosmology and Extragalactic AstrophysicsJet ProductionP P --> JET XInclusiveProton-Proton ScatteringHigh Energy Physics::ExperimentD2SIG/DPT/DYRAPTransverse Momentum DependenceDouble Differential Cross SectionAstrophysics::Galaxy Astrophysics
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"Table 29" of "Jet-hadron correlations measured relative to the second order event plane in Pb-Pb collisions at $\sqrt{s_{\rm{NN}}}$ = 2.76 TeV"

2020

Response matrices for mid-plane jets with kinematic cuts described in the paper for 30-50% centrality in Pb-Pb collisions

2760.0Nuclear ExperimentPB PB --> CHARGED XAstrophysics::Galaxy Astrophysics
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