Search results for " background"

showing 10 items of 316 documents

Tracing the Cultural Background of Lone-Wolf Terrorism

2021

The end of the Cold War, as well as the collapse of the Soviet Union, posed new greater challenges and risks for the “Global North.” Terrorism—doubtless—seems to be one of them. Over the recent years, and particularly after 9/11, terrorists changed the focus of their attacks. While classic terrorism targeted important persons such as politicians, chief police officers, or celebrities, modern terrorism planned attacks on leisure-spots spaces, tourist destinations, and lay-persons. This is particularly troublesome for policymakers (who are in charge of orchestrating all-pervading models to preserve homeland security) and for field-workers who are seriously punished when they are in contact wi…

Cultural backgroundInformation Systems and ManagementComputer Networks and CommunicationsHardware and ArchitecturePolitical scienceLone wolfTerrorismCriminologySafety Risk Reliability and QualitySafety ResearchSoftwareInternational Journal of Cyber Warfare and Terrorism
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Statistics Anxiety and Self-Concept of Beginning Students in the Social Sciences - A Matter of Gender and Socio-Cultural Background?

2015

Angst im Fach Statistik und statistisches Selbstkonzept von Studienanfangerinnen und -anfangern in den Sozialwissenschaften - eine Frage des Geschlechts und des sozio-kulturellen Hintergrunds? Es ist weitgehend unerforscht, ob bestimmte Studierendengruppen in den Sozialwissenschaften ihr Studium mit unterschiedlichen Einstellungen zum Fach Statistik beginnen. Im Folgenden wird untersucht, inwieweit das Geschlecht und der sozio-kulturelle Hintergrund einen Einfluss auf die Angst und das Selbstkonzept im Fach Statistik zu Studienbeginn haben. Eine Befragung von 504 Studierenden im ersten Studienjahr an zwei Universitaten und zwei Studiengangen zeigt, dass zwischen den Geschlechtern deutliche …

Cultural backgroundSelf-conceptStatistics anxietyPsychologyHumanities
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Understanding the Context of Teacher Professionalism in Education Systems Undergoing Transition – Kosovo Case

2014

Abstract This qualitative case study examines teacher professionalism in Kosovo in light of its rapidly developing education system. The study involves 14 teachers at the beginning of their careers (1-7 years of experience) examining teacher thinking against the evolving stages of teacher professionalism, namely pre-professionalism, autonomous professionalism, collegial professionalism and post-professionalism. The study reveals that Kosovo teachers reflect strong dominance of pre- professionalism and autonomous professionalism while they demonstrate a weaker reflection of collegial and post- professional aspects of teachers’ work. It provides insights for viewing teacher professionalism wi…

Cultural backgroundsocial beingDominance (economics)Transition (fiction)teacher professionalismPedagogycontextual factorsGeneral Materials ScienceContext (language use)collegialitySociologyCollegialityhistorical backgroundProcedia - Social and Behavioral Sciences
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Measurement of the Atmospheric ve flux in IceCube

2012

We report the first measurement of the atmospheric electron neutrino flux in the energy range between approximately 80 GeV and 6 TeV, using data recorded during the first year of operation of IceCube's DeepCore low energy extension. Techniques to identify neutrinos interacting within the DeepCore volume and veto muons originating outside the detector are demonstrated. A sample of 1029 events is observed in 281 days of data, of which 496 $\pm$ 66(stat.) $\pm$ 88(syst.) are estimated to be cascade events, including both electron neutrino and neutral current events. The rest of the sample includes residual backgrounds due to atmospheric muons and charged current interactions of atmospheric muo…

DEEPCOREParticle physicsAMANDAPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and Astronomyddc:500.201 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsSEARCH0103 physical sciencesddc:550010306 general physicsNeutrino oscillationDETECTORPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologySolar neutrino problemCosmic neutrino backgroundNeutrino detectorPhysics and Astronomy13. Climate actionMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrino astronomyNeutrinoNEUTRINO-INDUCED CASCADESAstrophysics - High Energy Astrophysical PhenomenaPhysical Review Letters
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GW170817: Implications for the Stochastic Gravitational-Wave Background from Compact Binary Coalescences

2018

The LIGO Scientific and Virgo Collaborations have announced the first detection of gravitational waves from the coalescence of two neutron stars. The merger rate of binary neutron stars estimated from this event suggests that distant, unresolvable binary neutron stars create a significant astrophysical stochastic gravitational-wave background. The binary neutron star background will add to the background from binary black holes, increasing the amplitude of the total astrophysical background relative to previous expectations. In the Advanced LIGO-Virgo frequency band most sensitive to stochastic backgrounds (near 25 Hz), we predict a total astrophysical background with amplitude $\Omega_{\rm…

Design sensitivityneutron star: binarygravitational radiation: stochasticAstronomyX-ray binaryGeneral Physics and AstronomyAstrophysicsAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologylocalizationGravitational wave backgroundGravitational Waves Neutron Stars Stochastic Background Virgo LIGOblack holeLIGOstochastic modelQCQBPhysicsGAMMA-RAY BURSTSSignal to noise ratioStochastic systemsBlack holesGravitational effectsarticleAstrophysics::Instrumentation and Methods for AstrophysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSING[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sources Experimental studies of gravity Gravitational WavesGravitationBinary neutron starsX-ray bursterBinsAstrophysics::High Energy Astrophysical PhenomenaMERGERSFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesgravitational radiation: direct detectionBinary pulsarNeutron starsSTAR-FORMATIONPhysics and Astronomy (all)General Relativity and Quantum CosmologyBinary black holebinary: coalescence0103 physical sciencesFrequency bandsddc:530RATESINTERFEROMETERS010306 general physicsAstrophysics::Galaxy AstrophysicsNeutronsGravitational Waves010308 nuclear & particles physicsGravitational waveVirgogravitational radiation: backgroundgravitational radiationAstronomyNeutron Stars530 Physikbinary: compactsensitivityStarsLIGObackground: stochasticEVOLUTIONsignal noise ratioVIRGOPhysics and Astronomyblack hole: binarygravitational radiation: emissionStellar black holeStochastic BackgroundDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikHIGH-REDSHIFTneutron star: coalescencePhysical Review Letters
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Pathways to higher education in France and Switzerland: Do vocational tracks facilitate access to higher education for immigrant students?

2014

In this chapter we wish to clarify through which institutional pathways higher education is accessed by immigrant group students in Switzerland and France. We have chosen these two countries because they differ from each other both in their educational systems and in the ways new routes to higher education have been set up through vocationally orientated programmes. The educational landscape in France is characterised by a more school-based system and has a greater tradition of prestigious tertiary education institutions (Duru-Bellat et al., 2008). Moreover, traditional vocational education and training (VET) does not have very high status and therefore fails to attract a large proportion o…

Educational backgroundHigher educationComparaison internationalemedia_common.quotation_subject[SHS.EDU]Humanities and Social Sciences/EducationImmigration[SHS.EDU] Humanities and Social Sciences/EducationeducationInternational ComparisonImmigrationProfessionnalisationDéterminant de la réussitePedagogy050602 political science & public administrationParcours scolaireTrainingFormation professionnelleSociologyAccès à l'enseignement supérieurSocioeconomic statusCursus universitairemedia_commonMedical educationbusiness.industry4. Education05 social sciences050301 educationHigh education[ SHS.EDU ] Humanities and Social Sciences/EducationSwissCountry of origin0506 political sciencedeterminant of successEnseignement professionnelvocationalisationVocational educationÉlèveFranceAccess to Higher EducationStudentbusinesseducational pathways0503 educationAccess to Higher Educationvocational programme
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Effet de l'origine sociale des élèves sur les résultats en lecture d'après PISA

2003

International audience

Effet[SHS.SOCIO]Humanities and Social Sciences/Sociology[SHS.SOCIO] Humanities and Social Sciences/Sociology[SHS.EDU]Humanities and Social Sciences/Education[SHS.EDU] Humanities and Social Sciences/EducationPISAElève[ SHS.EDU ] Humanities and Social Sciences/Education[ SHS.SOCIO ] Humanities and Social Sciences/SociologyAchievementRésultat scolaireOrigine socialeApprentissage de la lectureReading AchievementÉlèveSocioeconomic backgroundLectureRéussite scolaireStudentsComputingMilieux_MISCELLANEOUS
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The dark side of curvature

2009

Geometrical tests such as the combination of the Hubble parameter H(z) and the angular diameter distance d(A)(z) can, in principle, break the degeneracy between the dark energy equation of state parameter w(z), and the spatial curvature Omega(k) in a direct, model-independent way. In practice, constraints on these quantities achievable from realistic experiments, such as those to be provided by Baryon Acoustic Oscillation (BAO) galaxy surveys in combination with CMB data, can resolve the cosmic confusion between the dark energy equation of state parameter and curvature only statistically and within a parameterized model for w(z). Combining measurements of both H(z) and d(A)(z) up to suffici…

Equation of stateCosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmic microwave backgroundFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCurvature01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesDark energy experiments010303 astronomy & astrophysicsPhysics010308 nuclear & particles physicsAngular diameter distanceAstronomy and AstrophysicsRedshiftCosmological parameters from CMBRHigh Energy Physics - PhenomenologysymbolsDark energyBaryon acoustic-oscillationsBaryon acoustic oscillationsHubble's lawAstrophysics - Cosmology and Nongalactic Astrophysics
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Flavor Ratio of Astrophysical Neutrinos above 35 TeV in IceCube

2015

A diffuse flux of astrophysical neutrinos above $100\,\mathrm{TeV}$ has been observed at the IceCube Neutrino Observatory. Here we extend this analysis to probe the astrophysical flux down to $35\,\mathrm{TeV}$ and analyze its flavor composition by classifying events as showers or tracks. Taking advantage of lower atmospheric backgrounds for shower-like events, we obtain a shower-biased sample containing 129 showers and 8 tracks collected in three years from 2010 to 2013. We demonstrate consistency with the $(f_e:f_{\mu}:f_\tau)_\oplus\approx(1:1:1)_\oplus$ flavor ratio at Earth commonly expected from the averaged oscillations of neutrinos produced by pion decay in distant astrophysical sou…

FLUXAMANDAParticle physicsPhysics::Instrumentation and DetectorsENERGIESAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Physics and AstronomyFluxCosmic rayAstrophysicsACCELERATION01 natural sciencesflavor : ratioHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryIceCubeHigh Energy Physics - Experiment (hep-ex)PionObservatory0103 physical sciencesddc:550010306 general physicsNeutrino oscillationHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsSigmashowersCOSMIC-RAYSatmosphere : backgroundtracksneutrino : flavor : rationeutrino : oscillationfluxobservatoryPhysics and Astronomy13. Climate actionHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical Phenomenaneutrino : VHEpi : decay
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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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