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showing 10 items of 2432 documents

1,2-DICHLOROETHANE CONTAMINATED AQUIFER: MICROBIAL COMMUNITY RESPONSE TO BIOSTIMULATION IN MICROCOSM

2022

anaerobic microcosm12-dichloroethane contaminated groundwaterbacterial communitiesSettore BIO/19 - Microbiologia Generale
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Study of anthropogenic sinkholes in the Marsala area (western Sicily) through numerical analyses of instability processes in underground quarries

2011

anthropogenic sinkholeSettore GEO/04 - Geografia Fisica E GeomorfologiaSicilySettore GEO/05 - Geologia Applicataunderground quarry
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Search for low-energy neutrinos from astrophysical sources with Borexino

2019

We report on searches for neutrinos and antineutrinos from astrophysical sources performed with the Borexino detector at the Laboratori Nazionali del Gran Sasso in Italy. Electron antineutrinos ($\bar{\nu}_e$) are detected in an organic liquid scintillator through the inverse $\beta$-decay reaction. In the present work we set model-independent upper limits in the energy range 1.8-16.8 MeV on neutrino fluxes from unknown sources that improve our previous results, on average, by a factor 2.5. Using the same data set, we first obtain experimental constraints on the diffuse supernova $\bar{\nu}_e$ fluxes in the previously unexplored region below 8 MeV. A search for $\bar{\nu}_e$ in the solar ne…

antineutrinosPhysics - Instrumentation and Detectorssolar flaresmagnetic field: highneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoscintillation counter: liquidelastic scatteringantineutrino/e: particle identification01 natural sciences7. Clean energyneutrino: fluxlaw.inventionHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]neutrino: supernova26.65.+t010303 astronomy & astrophysicsBorexinoElastic scatteringPhysicsSolar flareSupernova Relic Neutrinosneutrino: energy spectrumS067EB8neutrinosInstrumentation and Detectors (physics.ins-det)neutrino: magnetic momentDiffuse Supernova Neutrino Background3. Good healthSupernovaHomestakeddc:540neutrino: flavorAntineutrinoBorexinoNeutrino97.60.BwHomestake experimentFlareantineutrino/e: fluxAntineutrinos13.15.+G; 26.65.+T; 29.40.Mc; 97.60.Bw; Antineutrinos; Diffuse supernova neutrino background; Neutrinos; Solar flares; Supernova relic neutrinosAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSupernova relic neutrinosupernova relic neutrinosNONuclear physics13.15.+gPE2_2Antineutrinos; Neutrinos; Diffuse supernova neutrino background; Supernova relic neutrinos; Solar flares0103 physical sciencesNeutrino[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Neutrinosdiffuse supernova neutrino background010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstronomy and Astrophysicsneutrino: particle source29.40.McGran SassoSolar flareSolar Flares13. Climate actionspectralHigh Energy Physics::Experimentexperimental results
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Borexino’s search for low-energy neutrino and antineutrino signals correlated with gamma-ray bursts

2017

International audience; A search for neutrino and antineutrino events correlated with 2350 gamma-ray bursts (GRBs) is performed with Borexino data collected between December 2007 and November 2015. No statistically significant excess over background is observed. We look for electron antineutrinos ( ν¯e ) that inverse beta decay on protons with energies from 1.8  MeV to 15  MeV and set the best limit on the neutrino fluence from GRBs below 8  MeV. The signals from neutrinos and antineutrinos from GRBs that scatter on electrons are also searched for, a detection channel made possible by the particularly radio-pure scintillator of Borexino. We obtain currently the best limits on the neutrino f…

antineutrinoselectronAntineutrinosneutrino: solarPhysics::Instrumentation and Detectorsdata acquisitionSolar neutrino[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]Astrophysics::High Energy Astrophysical Phenomenalow energy/MeV neutrinosElectrongamma ray: burst01 natural sciencesNuclear physicsLow energy/MeV neutrino0103 physical sciencesNeutrinoLow energy/MeV neutrinosNeutrinosNuclear Experiment010303 astronomy & astrophysicsGamma-ray burstBorexinoscintillation counterPhysicsflavor010308 nuclear & particles physicsbackgroundgamma-ray burstsneutrinosAntineutrinos; Gamma-ray bursts; Low energy/MeV neutrinos; Neutrinos; Astronomy and AstrophysicsAstronomy and Astrophysicssemileptonic decayantineutrinocorrelation: timeNeutrino detectorInverse beta decayddc:540Scintillation counterreadoutHigh Energy Physics::ExperimentBorexinoGamma-ray burstsNeutrinoGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Oppilaiden näkemyksiä luonnontieteiden opettajan auktoriteetistä

2019

Tässä tutkimuksessa selvitettiin oppilaiden näkemyksiä luonnontieteiden opettajan auktoriteetista, sen muodostumisesta ja kehittämisestä. Tutkimus pohjautuu fenomenologis-hermeneuttisen tutkimuksen piirteisiin. Oppilaiden (N = 25) näkemyksiä selvitettiin kyselytutkimuksen avulla ja tutkimusaineisto analysoitiin sekä tilastollisen analyysin että aineistolähtöisen sisällönanalyysin keinoin. Tulosten perusteella auktoriteetti liitettiin osaksi opettajan persoonaa ja asiantuntijuutta. Osaltaan auktoriteetin katsottiin tarkoittavan myös vuorovaikutussuhdetta, jossa opettajalla on oppilasta enemmän valtaa. Auktoriteetin koettiin muodostuvan vuorovaikutussuhteessa, jossa merkittäviä tekijöitä oliv…

auktoriteettiscience teacherteachershipluonnontieteetopettajuusfenomenologis-hermeneuttinen tutkimushermeneutic phenomenological researchopettajatluonnontieteiden opettajatauthorityopettaja-oppilassuhdegrounded theory
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L’autoreprésentation féminine dans la bande dessinée pornographique

2017

What happens when feminine authors investigate porn-comics and draw themselves in it ? Self-depiction of feminine authors conveys something original in a field where it usually is a way to express a private fantasy. From feminist comics of the 70s to the most recent porn comics, authors’ bodies are not sex objects anymore, they are the subject of a narration. Self-depiction is a new material for porn-comics and gives sincerity to the stories, it may be a way to express political views. Self-fantasy, sex confession or physical metamorphosis are the multiple ways self-depiction provides the feminine author to strengthen her authorship. Implicitly those self-depicted porn-authors draw up an in…

autoportraitHumorself-depictionEroticsAutobiographiefanzinePornographiegender studiesCorpsgenreféminismeundergroundcomicsComicsFeminist studiesErotismeeroticsUndergroundautobiographyAutobiographyAutoreprésentationFanzinebande dessinéehumorhumourFéminismebodyEsthétiqueSelf-depictionHumourAutoportraitpornographycorpsautobiographiepornographieGender studies[SHS.ART] Humanities and Social Sciences/Art and art historyBodyGenreself-portraitPornographyBande dessinéeérotismeesthétiqueSelf-portraitautoreprésentationfeminist studies
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Time-integrated Neutrino Source Searches with 10 years of IceCube Data

2020

Physical review letters 124(5), 051103 (1-9) (2020). doi:10.1103/PhysRevLett.124.051103

background [atmosphere]Astrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysics53001 natural sciencesIceCubeparticle source [neutrino]TRACK RECONSTRUCTION0103 physical sciencesddc:530atmosphere [muon]010306 general physicsAstrophysics::Galaxy Astrophysicsmedia_commonastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MuonAstrophysics::Instrumentation and Methods for AstrophysicsNorthern HemisphereAstronomyGalaxymessengerPhysics and AstronomySkycorrelationtime dependenceupgradegalaxyNeutrinoAstrophysics - High Energy Astrophysical Phenomenastatistical
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Neutrinos below 100 TeV from the southern sky employing refined veto techniques to IceCube data

2020

Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos with a typical energy cutoff well below 100 TeV. For the IceCube Neutrino Observatory located at the South Pole, the southern sky, containing the inner part of the Galactic plane and the Galactic Center, is a particularly challenging region at these energies, because of the large background of atmospheric muons. In this paper, we present recent advancements in data selection strategies for track-like muon neutrino events with energies below 100 TeV from the southern sky. The strategies utilize the outer detector regions as veto and features of the signal pattern to reduce the background of atm…

background [atmosphere]Physics::Instrumentation and Detectorsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenapoleFOS: Physical sciences01 natural sciencesHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryIceCubecharged currentHigh Energy Physics - Experiment (hep-ex)Neutrinos; Point sources; Veto techniquesSEARCHTRACK RECONSTRUCTION0103 physical sciencessupernovaMuon neutrinoatmosphere [muon]Neutrinos010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsneutrino muonMuon010308 nuclear & particles physicsICEGalactic CenterHigh Energy Physics::PhenomenologyVeto techniquesAstronomyPoint sourcesAstronomy and Astrophysicsflux [neutrino]Galactic planeobservatorySupernovaPhysics and AstronomySkyenergy [neutrino]gamma rayddc:540spectralHigh Energy Physics::ExperimentgalaxyNeutrinoAstrophysics - High Energy Astrophysical Phenomena
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Comparison between simulated and observed LHC beam backgrounds in the ATLAS experiment at E beam =4 TeV

2018

Results of dedicated Monte Carlo simulations of beam-induced background (BIB) in the ATLAS experiment at the Large Hadron Collider (LHC) are presented and compared with data recorded in 2012. During normal physics operation this background arises mainly from scattering of the 4 TeV protons on residual gas in the beam pipe. Methods of reconstructing the BIB signals in the ATLAS detector, developed and implemented in the simulation chain based on the FLUKA Monte Carlo simulation package, are described. The interaction rates are determined from the residual gas pressure distribution in the LHC ring in order to set an absolute scale on the predicted rates of BIB so that they can be compared qua…

background [beam]background: inducedPhysics::Instrumentation and DetectorsCiencias FísicasMonte Carlo method01 natural sciencesHigh Energy Physics - ExperimentSubatomär fysik//purl.org/becyt/ford/1 [https]High Energy Physics - Experiment (hep-ex)beam lossesSubatomic Physicsscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]and programsInstrumentationQCMathematical PhysicsPhysicsLarge Hadron ColliderRadiation calculationsAtlas (topology)Accelerator modelling and simulations (multi-particle dynamics; single-particle dynamics)DetectorATLAS experimentSettore FIS/01 - Fisica SperimentaleSimulation methods and programBeams (radiation) Accelerator modelling and simulations (multi-particle dynamics;; single-particle dynamics); Radiation calculations; Simulation methods; and programs; DETECTOR; SEARCHObservableAccelerator modelling and simulations (multi-particle dynamicMonte Carlo [numerical calculations]ATLASNuclear & Particles PhysicsAccelerator modelling and simulationsCERN LHC Coll collimators beam: backgroundcolliding beams [p p]numerical calculations: Monte CarloCIENCIAS NATURALES Y EXACTASParticle Physics - Experimentp p: scatteringAccelerator modelling and simulations (multi-particle dynamics; Radiation calculations; Simulation methods and programs; single-particle dynamics); Instrumentation; Mathematical Physics530 PhysicsCiências Naturais::Ciências Físicas:Ciências Físicas [Ciências Naturais]FOS: Physical sciencesFísica de Partículas y CamposAccelerator Physics and InstrumentationNuclear physicsFLUKAsingle-particle dynamics)ATLAS LHC High Energy PhysicsHIGH ENERGY PHYSICSSEARCH0103 physical sciencesddc:610010306 general physicsAbsolute scaleDETECTORpressure [gas]Science & Technology010308 nuclear & particles physicsScatteringhep-exRadiation calculationscatteringAcceleratorfysik och instrumentering//purl.org/becyt/ford/1.3 [https]ghostAccelerator modelling and simulations (multi-particle dynamicsSimulation methodscorrelationinduced [background]Experimental High Energy Physicsgas: pressureSimulation methods and programsp p: colliding beamsexperimental results
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Spectral shapes of forbidden argon β decays as background component for rare-event searches

2018

The spectral shape of the electrons from the two first-forbidden unique ${\beta }^{-}$ decays of 39Ar and 42Ar were calculated for the first time to the next-to-leading order. Especially the spectral shape of the 39Ar decay can be used to characterize this background component for dark matter searches based on argon. Alternatively, due to the low thresholds of these experiments, the spectral shape can be investigated over a wide energy range with high statistics and thus allow a sensitive comparison with the theoretical predictions, in particular at low electron energies where the shape of the computed β spectrum has a slight dependence on the value of the weak axial-vector coupling constan…

background componentforbidden argon β decayrare-event searchesspectral shapes
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