Search results for " Experiments"

showing 10 items of 315 documents

Femtolensing by dark matter revisited

2018

Femtolensing of gamma ray bursts (GRBs) has been put forward as an exciting possibility to probe exotic astrophysical objects with masses below $10^{-13}$ solar masses such as small primordial black holes or ultra-compact dark matter minihalos, made up for instance of QCD axions. In this paper we critically review this idea, properly taking into account the extended nature of the source as well as wave optics effects. We demonstrate that most GRBs are inappropriate for femtolensing searches due to their large sizes. This removes the previous femtolensing bounds on primordial black holes, implying that vast regions of parameter space for primordial black hole dark matter are not robustly con…

Astrophysics and AstronomyCosmology and Nongalactic Astrophysics (astro-ph.CO)spectraAstrophysics::High Energy Astrophysical PhenomenaDark mattergravitational lensinghaloFOS: Physical sciencesPrimordial black holegamma ray experimentsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsParameter space01 natural sciencesHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciences010306 general physicsAxionParticle Physics - PhenomenologyPhysicsQuantum chromodynamicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Solar mass010308 nuclear & particles physicsraydark matter experimentsprimordial black holesAstronomy and Astrophysicshep-phPhysical opticsHigh Energy Physics - Phenomenologypair production13. Climate actionastro-ph.COGamma-ray burstlimitsAstrophysics - High Energy Astrophysical Phenomenagravitational-wavesAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of Cosmology and Astroparticle Physics
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Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons

2017

High energy cosmic ray electrons plus positrons (CREs), which lose energy quickly during their propagation, provide an ideal probe of Galactic high-energy processes and may enable the observation of phenomena such as dark-matter particle annihilation or decay. The CRE spectrum has been directly measured up to $\sim 2$ TeV in previous balloon- or space-borne experiments, and indirectly up to $\sim 5$ TeV by ground-based Cherenkov $\gamma$-ray telescope arrays. Evidence for a spectral break in the TeV energy range has been provided by indirect measurements of H.E.S.S., although the results were qualified by sizeable systematic uncertainties. Here we report a direct measurement of CREs in the …

Astrophysics::High Energy Astrophysical PhenomenaDark matterFOS: Physical sciencesCosmic rayElectron01 natural sciencesdark matterHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Positroncosmic rays0103 physical sciences010303 astronomy & astrophysicsCherenkov radiationHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicscosmic rays dark matter electrons space experimentsMultidisciplinaryAnnihilation010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleSpectrum (functional analysis)electronsGalaxyHigh Energy Physics - PhenomenologyHigh Energy Physics::Experimentspace experimentsAstrophysics - High Energy Astrophysical Phenomena
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Medium modification of the shape of small-radius jets in central Pb-Pb collisions at √sNN = 2.76 TeV

2018

We present the measurement of a new set of jet shape observables for track-based jets in central Pb-Pb collisions at sNN−−−√=2.76 TeV. The set of jet shapes includes the first radial moment or angularity, g; the momentum dispersion, pTD; and the difference between the leading and sub-leading constituent track transverse momentum, LeSub. These observables provide complementary information on the jet fragmentation and can constrain different aspects of the theoretical description of jet-medium interactions. The jet shapes were measured for a small resolution parameter R = 0.2 and were fully corrected to particle level. The observed jet shape modifications indicate that in-medium fragmentation…

Astrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::Experimenthiukkasfysiikkaheavy ion experiments
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Constraints on neutrino emission from nearby galaxies using the 2MASS redshift survey and IceCube

2020

The distribution of galaxies within the local universe is characterized by anisotropic features. Observatories searching for the production sites of astrophysical neutrinos can take advantage of these features to establish directional correlations between a neutrino dataset and overdensities in the galaxy distribution in the sky. The results of two correlation searches between a seven-year time-integrated neutrino dataset from the IceCube Neutrino Observatory, and the 2MASS Redshift Survey (2MRS) catalog are presented here. The first analysis searches for neutrinos produced via interactions between diffuse intergalactic Ultra-High Energy Cosmic Rays (UHECRs) and the matter contained within …

Astrophysics::High Energy Astrophysical PhenomenaUHE [cosmic radiation]FOS: Physical sciencesanisotropyAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesIceCubeIceCube Neutrino Observatoryneutrino astronomyneutrino experiments0103 physical sciencessiteAstrophysics::Galaxy Astrophysicsastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)densityneutrino astronomy; neutrino detectors; neutrino experiments010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicsflux [neutrino]redshiftRedshift surveyGalaxyRedshiftobservatoryNeutrino detectorPhysics and Astronomymultiplet13. Climate actioncorrelationPhysique des particules élémentairesIntergalactic travelHigh Energy Physics::ExperimentgalaxyNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical Phenomenaneutrino detectors
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Experimental observations of upstream overdeepening

2005

The issue of morphodynamic influence in meandering streams is investigated through a series of laboratory experiments on curved and straight flumes. Both qualitative and quantitative observations confirm the suitability of the recent theoretical developments (Zolezzi & Seminara 2001) that indicate the occurrence of two distinct regimes of morphodynamic influence, depending on the value of the width ratio of the channel β. The threshold value βR separating the upstream from the downstream influence regimes coincides with the resonant value discovered by Blondeaux & Seminara (1985). Indeed it is observed that upstream influence may occur only in relatively wide channels, while narrower stream…

BedformMechanics of MaterialsMechanical EngineeringOverdeepeningThe issue of morphodynamic influence in meandering streams is investigated through a series of laboratory experiments on curved and straight flumes. Both qualitative and quantitative observations confirm the suitability of the recent theoretical developments (Zolezzi & Seminara 2001) that indicate the occurrence of two distinct regimes of morphodynamic influence depending on the value of the width ratio of the channel β. The threshold value βR separating the upstream from the downstream influence regimes coincides with the resonant value discovered by Blondeaux & Seminara (1985). Indeed it is observed that upstream influence may occur only in relatively wide channels while narrower streams are dominated by downstream influence. A series of experiments has been carried out in order to check the above theoretical predictions and show for the first time evidence of the occurrence of upstream overdeepening. Two different sets of experiments have been designed where a discontinuity in channel geometry was present such that the channel morphodynamics was influenced in the upstream direction under super-resonant conditions (β >βR) and in the downstream direction under sub-resonant conditions (β <βR). Experimental results give qualitative and quantitative support to the theoretical predictions and allow us to clarify the limits of the linear analysis.MechanicsLinear analysisCondensed Matter PhysicsWidth ratioGeology
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Effect of a Heavy Rainstorm on the Surface Hydrodynamic Properties of a Sandy-Loam Soil

2022

Changes in surface-soil hydrodynamic properties associated with torrential natural rainstorms are largely unknown. This investigation aimed at verifying if the surface hydrodynamic properties of a sandy-loam soil varied due to the heavy rainfall event (130 mm in nearly three hours) that occurred in the summer of 2020 at Palermo (Italy) and also to establish if soil recovery processes occurred soon after the event. The soil of an orchard was sampled immediately before the rainstorm and a few days and 1.5 months later. The rainstorm determined a moderate decrease (by 1.8 times) of the saturated soil hydraulic conductivity, Ks, and an increase of its relative variability. In the subsequent wee…

Beerkan infiltration experimentsSettore AGR/08 - Idraulica Agraria E Sistemazioni Idraulico-ForestaliEnvironmental ChemistrySandy-loam soilSurface soil hydrodynamic propertieHeavy rainstormGeneral Environmental ScienceWater Science and TechnologyCivil and Structural EngineeringJournal of Hydrologic Engineering
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Complete 1H and 13C NMR assignments of clerodane diterpenoids of Salvia splendens.

2006

Unambiguous and complete assignments of 1H and 13C NMR chemical shifts for five clerodane diterpenes, four of them isolated from Salvia splendens (salviarin, splendidin and splenolides A and B) and one obtained by acetylation of splenolide A, are presented. The assignments are based on 2D shift-correlated [1H,1H–COSY, 1H,13C-gHSQC–1J(C,H) and 1H,13C-gHMBC-nJ(C,H) (n = 2 and 3)] and nuclear Overhauser effect (NOE) experiments. The conformation of the rings of these compounds is supported by the 3J(H,H) values and NOE results. Copyright © 2006 John Wiley & Sons, Ltd.

Carbon IsotopesMagnetic Resonance SpectroscopybiologyStereochemistryChemistryChemical shiftAcetylationGeneral ChemistryNuclear Overhauser effectCarbon-13 NMRSalviabiology.organism_classificationDiterpenes ClerodaneUnambiguous and complete assignments of 1H and 13C NMR chemical shifts for five clerodane diterpenes four of them isolated from Salvia splendens (salviarin splendidin and splenolides A and B) and one obtained by acetylation of splenolide A are presented. The assignments are based on 2D shiftcorrelated [1H1H–COSY 1H13C-gHSQC–1J(CH) and 1H13C-gHMBC-nJ(CH) (n = 2 and 3)] and nuclear Overhauser effect (NOE) experiments. The conformation of the rings of these compounds is supported by the 3J(HH) values and NOE results. Copyright  2006 John Wiley & Sons LtdClerodane DiterpenesProton NMRGeneral Materials ScienceSalviaHydrogenMagnetic resonance in chemistry : MRC
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Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre

2021

Full list of authors: Acharyya, A.; Adam, R.; Adams, C.; Agudo, I.; Aguirre-Santaella, A.; Alfaro, R.; Alfaro, J.; Alispach, C.; Aloisio, R.; Alves Batista, R.; Amati, L.; Ambrosi, G.; Angüner, E. O.; Antonelli, L. A.; Aramo, C.; Araudo, A.; Armstrong, T.; Arqueros, F.; Asano, K.; Ascasíbar, Y. Ashley, M.; Balazs, C.; Ballester, O.; Baquero Larriva, A.; Barbosa Martins, V.; Barkov, M.; Barres de Almeida, U.; Barrio, J. A.; Bastieri, D.; Becerra, J.; Beck, G.; Becker Tjus, J.; Benbow, W.; Benito, M.; Berge, D.; Bernardini, E.; Bernlöhr, K.; Berti, A.; Bertucci, B.; Beshley, V.; Biasuzzi, B.; Biland, A.; Bissaldi, E.; Biteau, J.; Blanch, O.; Blazek, J.; Bocchino, F.; Boisson, C.; Bonneau Arbe…

Cherenkov Telescope ArrayMATÉRIA ESCURAscale: TeVAstronomyatmosphere [Cherenkov counter]dark matter experimentDark matter theoryenergy resolutionGamma ray experimentsParticleAstrophysicscosmic background radiation01 natural sciences7. Clean energyHigh Energy Physics - Phenomenology (hep-ph)benchmarkWIMPHESSenergy: fluxTeV [scale]relativistic [charged particle]gamma ray experimentMAGIC (telescope)Monte CarloEvent reconstructionPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Contractionspatial distributiontrack data analysisPhysicsdensity [dark matter]ClumpyAstrophysics::Instrumentation and Methods for AstrophysicsimagingHigh Energy Physics - Phenomenologydark matter experiments; dark matter theory; gamma ray experiments; galaxy morphologyDark matter experimentsFísica nuclearVERITASAstrophysics - High Energy Astrophysical PhenomenaSimulationsnoiseWIMPAstrophysics::High Energy Astrophysical PhenomenaDark mattersatelliteCosmic background radiationFOS: Physical sciencesAnnihilationdark matter: densityAstrophysics::Cosmology and Extragalactic AstrophysicsCherenkov counter: atmosphereheavy [dark matter]530annihilation [dark matter]GLASTDark matter experiments; Dark matter theory; Galaxy morphology; Gamma ray experimentscosmic radiation [p]0103 physical sciencesCherenkov [radiation]Candidatesddc:530AGNCherenkov radiationRadiative Processesthermal [cross section]010308 nuclear & particles physicsFísicadark matter: annihilationGamma-Ray SignalsCherenkov Telescope Array ; dark matter ; Galactic Center ; TeV gamma-ray astronomyAstronomy and AstrophysicsMassCherenkov Telescope Arrayradiation: CherenkovsensitivityMAGICGalaxyAstronomíadark matter: heavygamma rayp: cosmic radiation[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]correlationcharged particle: relativisticflux [energy]Galaxy morphology/dk/atira/pure/subjectarea/asjc/3100/3103galaxysupersymmetry[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cross section: thermal
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Design optimization of mooring system: An application to a vessel-shaped offshore fish farm

2019

Abstract Design optimization of mooring systems of offshore floating structures is a challenging task, partly because of the large number of design variables, complicated design constraints, nonlinear system behavior, and time-consuming numerical simulations. For engineering designs, efficient yet accurate approaches are needed. This paper proposes an integrated optimization methodology for design of mooring systems. The methodology integrates the design of experiments, screening analysis, time-domain simulations, and a metamodel-based optimization procedure. To demonstrate the methodology, the mooring system of a vessel-shaped offshore fish farm was designed considering the ultimate limit …

Computer scienceDesign of experiments0211 other engineering and technologies020101 civil engineering02 engineering and technologyMooring0201 civil engineeringMetamodelingNonlinear systemSearch algorithmKriging021105 building & constructionLimit state designSubmarine pipelineCivil and Structural EngineeringMarine engineeringEngineering Structures
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Critical analysis of conventional thermoeconomic approaches to the diagnosis of multiple faults in air conditioning units: Capabilities, drawbacks an…

2013

Abstract Faults diagnosis in air conditioning systems is a crucial activity, since malfunctions may induce heavy degradation of performance. Among the available techniques, thermoeconomic diagnosis has played a marginal role due to the difficulties encountered when applying the methodology to refrigeration plants. In this paper a critical analysis on capabilities and limits of thermoeconomic diagnosis is proposed. The reference plant is a 120 kWc air-cooled air conditioning system; a simulator is used to evaluate thermodynamic data under normal and faulty conditions, setting up “virtual experiments” to simulate each fault. Five malfunctions are imposed, either individually or simultaneously…

Computer sciencebusiness.industryThermoeconomic diagnosis Refrigeration Multiple faults Virtual experiments Quantitative analysisMechanical EngineeringRefrigerationHardware_PERFORMANCEANDRELIABILITYBuilding and ConstructionEnergy consumptionReliability engineeringRefrigerantAir conditioningSettore ING-IND/10 - Fisica Tecnica IndustrialebusinessGas compressorLeakage (electronics)International Journal of Refrigeration
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