Search results for "RSTS"

showing 10 items of 97 documents

Observation of High-Energy Astrophysical Neutrinos in Three Years of IceCube Data

2014

A search for high-energy neutrinos interacting within the IceCube detector between 2010 and 2012 provided the first evidence for a high-energy neutrino flux of extraterrestrial origin. Results from an analysis using the same methods with a third year (2012-2013) of data from the complete IceCube detector are consistent with the previously reported astrophysical flux in the 100 TeV - PeV range at the level of $10^{-8}\, \mathrm{GeV}\, \mathrm{cm}^{-2}\, \mathrm{s}^{-1}\, \mathrm{sr}^{-1}$ per flavor and reject a purely atmospheric explanation for the combined 3-year data at $5.7 \sigma$. The data are consistent with expectations for equal fluxes of all three neutrino flavors and with isotrop…

FLUXACTIVE GALACTIC NUCLEICosmology and Nongalactic Astrophysics (astro-ph.CO)TELESCOPESolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaGeneral Physics and AstronomyFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energyIceCubeIceCube Neutrino ObservatoryHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)SEARCH0103 physical sciencesddc:550010303 astronomy & astrophysicsGAMMA-RAY BURSTSPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsGlashow resonanceHigh Energy Physics::PhenomenologyASTRONOMYAstronomySolar neutrino problemBLAZARSPhysics and AstronomyNeutrino detector13. Climate actionLEPTONSJETSMeasurements of neutrino speedHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyEMISSIONAstrophysics - High Energy Astrophysical PhenomenaphysicsAstrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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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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Farmaceita un ārsta komunikācijas analīze Latvijā

2019

Sadarbība un informācijas apmaiņa starp ārstu un farmaceitu ir praksē pierādīts modelis veiksmīgam pacienta ārstniecības procesam. Lai sasniegtu veiksmīgu ārstniecības procesu ir nepieciešama komunikācija, kura ne vienmēr norisinās starp veselības aprūpes speciālistiem, šajā gadījumā starp ārstu un farmaceitu. Tas ir viens no iemesliem medicīnisko kļūdu pieļaušanā, pacienta līdzestības mazināšanā un terapijas efektivitātē. Bakalaura darba mērķis ir analizēt komunikāciju starp ārstu un farmaceitu Latvijā. Darba veikšanā tika izmantota empīriskā pētījuma metode. Anketas aizpildīja atsevišķi ārstniecības speciālisti, farmaceiti un medicīnas studenti. Kopā tika saņemtas 109 anketas. Anketas atb…

FarmaceitsFarmaceitiskā aprūpeFarmācijaĀrstsKomunikācijaVeselības aprūpe
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Network Physiology of Cortico–Muscular Interactions

2020

Skeletal muscle activity is continuously modulated across physiologic states to provide coordination, flexibility and responsiveness to body tasks and external inputs. Despite the central role the muscular system plays in facilitating vital body functions, the network of brain-muscle interactions required to control hundreds of muscles and synchronize their activation in relation to distinct physiologic states has not been investigated. Recent approaches have focused on general associations between individual brain rhythms and muscle activation during movement tasks. However, the specific forms of coupling, the functional network of cortico-muscular coordination, and how network structure a…

Flexibility (anatomy)Computer sciencePhysiologybrain wavesPhysiologynetwork physiologylcsh:Physiology03 medical and health sciencesMuscle tone0302 clinical medicineRhythmInteraction networkPhysiology (medical)medicinesleepSettore MAT/07 - Fisica Matematica030304 developmental biologySlow-wave sleepOriginal Research0303 health scienceslcsh:QP1-981burstsMuscular systemSkeletal muscledynamic networksSleep in non-human animalsmedicine.anatomical_structuremuscle tonetime delay stabilitysynchronization030217 neurology & neurosurgeryFrontiers in Physiology
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Scaler mode technique for the ARGO-YBJ detector

2008

The ARGO-YBJ experiment has been designed to study the Extensive Air Showers with an energy threshold lower than that of the existing arrays by exploiting the high altitude location(4300 m a.s.l. in Tibet, P.R. China) and the full ground plane coverage. The lower energy limit of the detector (E $\sim$ 1 GeV) is reached by the scaler mode technique, i.e. recording the counting rate at fixed time intervals. At these energies, transient signals due to local (e.g. Forbush Decreases) and cosmological (e.g. Gamma Ray Bursts) phenomena are expected as a significant variation of the counting rate compared to the background. In this paper the performance of the ARGO-YBJ detector operating in scaler …

Gamma ray burstAstrophysics::High Energy Astrophysical PhenomenaCamere a piani resistiviFOS: Physical sciencesCosmic rayAstrophysicsRivelatori di sciami estesi01 natural sciencesRaggi cosmiciOpticsSettore FIS/05 - Astronomia e Astrofisica0103 physical sciencesLimit (music)010303 astronomy & astrophysicsArgoGround planegamma ray bursts cosmic rays extended air showersPhysics010308 nuclear & particles physicsbusiness.industrySettore FIS/01 - Fisica SperimentaleAstrophysics (astro-ph)DetectorMode (statistics)Astronomy and AstrophysicsSciami estesibusinessGamma-ray burstEnergy (signal processing)
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Search for Neutrino‐induced Cascades from Gamma‐Ray Bursts with AMANDA

2007

Using the neutrino telescope AMANDA-II, we have conducted two analyses searching for neutrino-induced cascades from gamma-ray bursts. No evidence of astrophysical neutrinos was found, and limits are presented for several models. We also present neutrino effective areas which allow the calculation of limits for any neutrino production model. The first analysis looked for a statistical excess of events within a sliding window of 1 or 100 seconds (for short and long burst classes, respectively) during the years 2001-2003. The resulting upper limit on the diffuse flux normalization times E^2 for the Waxman-Bahcall model at 1 PeV is 1.6 x 10^-6 GeV cm^-2 s^-1 sr^-1 (a factor of 120 above the the…

Gamma rays: burstsNormalization (statistics)PhysicsRange (particle radiation)MuonAstrophysics::High Energy Astrophysical PhenomenaGamma rays: bursts; Neutrinos; TelescopesAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysicsCoincidenceSpace and Planetary ScienceCascadeAstronomiaDiffuse fluxHigh Energy Physics::ExperimentNeutrinosNeutrinoGamma-ray burstTelescopesThe Astrophysical Journal
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Constraints on Minute-Scale Transient Astrophysical Neutrino Sources

2019

High-energy neutrino emission has been predicted for several short-lived astrophysical transients including gamma-ray bursts (GRBs), core-collapse supernovae with choked jets, and neutron star mergers. IceCube's optical and x-ray follow-up program searches for such transient sources by looking for two or more muon neutrino candidates in directional coincidence and arriving within 100 s. The measured rate of neutrino alerts is consistent with the expected rate of chance coincidences of atmospheric background events and no likely electromagnetic counterparts have been identified in Swift follow-up observations. Here, we calculate generic bounds on the neutrino flux of short-lived transient so…

HIGH-ENERGY NEUTRINOSAstrophysics::High Energy Astrophysical PhenomenaPopulationGeneral Physics and AstronomyFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences7. Clean energy0103 physical sciencesMuon neutrinoddc:530education010303 astronomy & astrophysicsPhysicsGAMMA-RAY BURSTSHigh Energy Astrophysical Phenomena (astro-ph.HE)education.field_of_studyMuon010308 nuclear & particles physicsSupernovaNeutron starPhysics and Astronomy13. Climate actionPhysique des particules élémentairesHigh Energy Physics::ExperimentNeutrinoGamma-ray burstAstrophysics - High Energy Astrophysical PhenomenaEnergy (signal processing)
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Evidence for Astrophysical Muon Neutrinos from the Northern Sky with IceCube

2015

Results from the IceCube Neutrino Observatory have recently provided compelling evidence for the existence of a high energy astrophysical neutrino flux utilizing a dominantly Southern Hemisphere dataset consisting primarily of nu_e and nu_tau charged current and neutral current (cascade) neutrino interactions. In the analysis presented here, a data sample of approximately 35,000 muon neutrinos from the Northern sky was extracted from data taken during 659.5 days of livetime recorded between May 2010 and May 2012. While this sample is composed primarily of neutrinos produced by cosmic ray interactions in the Earth's atmosphere, the highest energy events are inconsistent with a hypothesis of …

HIGH-ENERGY NEUTRINOSFLUXESATMOSPHERIC MUONAstrophysics::High Energy Astrophysical PhenomenaSolar neutrinoFOS: Physical sciencesGeneral Physics and AstronomyAstrophysics01 natural sciencesIceCube Neutrino ObservatoryRATIO0103 physical sciencesddc:550010303 astronomy & astrophysicsGAMMA-RAY BURSTSHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSPECTRUMSpectral indexMuon010308 nuclear & particles physicsSolar neutrino problemPhysics and AstronomyNeutrino detector13. Climate actionHigh Energy Physics::ExperimentNeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical Phenomena
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ORIGIN: metal creation and evolution from the cosmic dawn

2012

Herder, Jan-Willem den et al.

HOT INTERGALACTIC MEDIUMUNIVERSEChemical evolutionMission7. Clean energy01 natural sciencesSpectral lineSettore FIS/05 - Astronomia E Astrofisica010303 astronomy & astrophysicsmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)NUCLEOSYNTHESISCOSMIC cancer databaseClusters of galaxiesSatellite MissionEpoch (reference date)Astrophysics::Instrumentation and Methods for AstrophysicsFORESTGALAXIESGamma-ray burstsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaX-ray Mission Gamma-ray bursts Clusters of galaxies Warm-hot intergalactic medium Chemical evolutionWarm-hot intergalactic mediumAstrophysics - Cosmology and Nongalactic AstrophysicsAstrophysics and AstronomyStructure formationCosmology and Nongalactic Astrophysics (astro-ph.CO)Clusters of galaxiemedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaREDSHIFTFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsX-ray Mission Gamma-ray bursts Clusters of galaxies Warm-hot intergalactic medium Chemical evolutionABSORPTION-SPECTRA010309 opticsX-rayYIELDS0103 physical sciencesGamma-ray burstInstrumentation and Methods for Astrophysics (astro-ph.IM)X-ray; Mission; Gamma-ray bursts; Clusters of galaxies; Warm-hot intergalactic medium; Chemical evolutionAstronomyAstronomy and AstrophysicsRedshiftGalaxyUniverse13. Climate actionChemical evolution; Clusters of galaxies; Gamma-ray bursts; Mission; Warm-hot intergalactic medium; X-ray; Astronomy and Astrophysics; Space and Planetary ScienceSpace and Planetary ScienceGamma-ray burstCLUSTERSExperimental Astronomy
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Instability of twisted magnetar magnetospheres

2019

We present three-dimensional force-free electrodynamics simulations of magnetar magnetospheres that demonstrate the instability of certain degenerate, high energy equilibrium solutions of the Grad-Shafranov equation. This result indicates the existence of an unstable branch of twisted magnetospheric solutions and allows to formulate an instability criterion. The rearrangement of magnetic field lines as a consequence of this instability triggers the dissipation of up to 30% of the magnetospheric energy on a thin layer above the magnetar surface. During this process, we predict an increase of the mechanical stresses onto the stellar crust, which can potentially result in a global mechanical f…

High Energy Astrophysical Phenomena (astro-ph.HE)Physicsnumerical [Methods]bursts [X-rays]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and Astrophysicsneutron [Stars]MagnetarInstabilitymagnetars [Stars]Theoretical physicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceMagnetic fieldsPhysics::Space PhysicsCost actionAstrophysics - High Energy Astrophysical PhenomenaPartial supportSolar and Stellar Astrophysics (astro-ph.SR)Astronomía y Astrofísica
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