Search results for "PC"

showing 10 items of 2805 documents

A search for neutrino emission from the Fermi bubbles with the ANTARES telescope

2014

Adrián-Martínez, S. et al.

Astrofísica[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics and Astronomy (miscellaneous)Physics::Instrumentation and DetectorsRayAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesantaresAstrophysicsddc:500.2Neutrino fluxesGamma ray burstsPartícules (Física nuclear)law.inventionTelescopeneutrinoRaigs gammalaw14. Life underwaterNeutrinsNeutrinosEngineering (miscellaneous)Cherenkov radiationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCOSMIC cancer databaseMuon[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologyAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayfermi bubbles; antares; neutrinoDetectorCharged particleNeutrino astrophysicsFermi bubbleneutrino telecope13. Climate actionFermi bubblesCol·lisions (Física nuclear):Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]FISICA APLICADAFísica nuclearHigh Energy Physics::ExperimentNeutrinoAstrophysics - High Energy Astrophysical PhenomenaAntares neutrino telescopeFermi Gamma-ray Space Telescope
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Searches for clustering in the time integrated skymap of the ANTARES neutrino telescope

2014

Adrián-Martínez, S. et al.

Astrofísica[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeFOS: Physical sciences01 natural sciencesneutrino astronomy0103 physical sciencesNeutrinsNeutrinosCluster analysis010303 astronomy & astrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physics[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]AutocorrelationGamma rayAstrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomyAstronomy and AstrophysicsGalaxyNeutrino astrophysicsneutrino astronomy; neutrino detectors[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]FISICA APLICADA:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]Spatial clusteringNeutrinoMATEMATICA APLICADAAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for Astrophysicsneutrino detectors
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ANTARES constrains a blazar origin of two IceCube PeV neutrino events

2015

Abstract Context. The source(s) of the neutrino excess reported by the IceCube Collaboration is unknown. The TANAMI Collaboration recently reported on the multiwavelength emission of six bright, variable blazars which are positionally coincident with two of the most energetic IceCube events. Objects like these are prime candidates to be the source of the highest-energy cosmic rays, and thus of associated neutrino emission. Aims. We present an analysis of neutrino emission from the six blazars using observations with the ANTARES neutrino telescope. Methods. The standard methods of the ANTARES candidate list search are applied to six years of data to search for an excess of muons and hence th…

Astrofísicaactive [Galaxies]Astrophysics::High Energy Astrophysical PhenomenaMonte Carlo methodFluxFOS: Physical sciencesCosmic rayAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics7. Clean energy01 natural sciencesSpectral line0103 physical sciencesNeutrinoGalaxies: active; Neutrinos; Quasars: generalNeutrinsNeutrinosBlazar010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)MuonCosmologia010308 nuclear & particles physicsFísicaAstronomy and Astrophysicsgeneral [Quasars]Galaxies: activeAstronomy and AstrophysicNeutrino astrophysicsQuasars generalCosmologyneutrinos – galaxies: active – quasars: generalQuasars: generalSpace and Planetary ScienceGalaxies activeCol·lisions (Física nuclear)Galaxies: active; Neutrinos; Quasars: general; Astronomy and Astrophysics; Space and Planetary Science:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]FISICA APLICADAFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical PhenomenaMATEMATICA APLICADA[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Event (particle physics)Astronomy & astrophysics
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Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and Ic…

2019

[EN] Astrophysical sources of gravitational waves, such as binary neutron star and black hole mergers or core-collapse supernovae, can drive relativistic outflows, giving rise to non-thermal high-energy emission. High-energy neutrinos are signatures of such outflows. The detection of gravitational waves and high-energy neutrinos from common sources could help establish the connection between the dynamics of the progenitor and the properties of the out¿ow. We searched for associated emission of gravitational waves and high-energy neutrinos from astrophysical transients with minimal assumptions using data from Advanced LIGO from its first observing run O1, and data from the ANTARES and IceCub…

Astrofísicacollapse [supernova]neutron star: binaryEVENTS GW150914Gravitació010504 meteorology & atmospheric sciencesneutrino: energy: highAstronomyRAYBinary numberbinary [neutron star]Astrophysics7. Clean energy01 natural sciencesPhysical ChemistryAtomicIceCubeneutrinoParticle and Plasma PhysicsAstronomi astrofysik och kosmologiblack holeAstronomy Astrophysics and CosmologyLIGO010303 astronomy & astrophysicsgravitational waveELECTROMAGNETIC SIGNALSQCQBSettore FIS/01PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HE[PHYS]Physics [physics]Astrophysics::Instrumentation and Methods for Astrophysicsneutrinosgravitational waves; neutrinos520 Astronomie und zugeordnete Wissenschaftenddc:observatorySupernovagravitational wavesastrophysics: densityPhysical SciencesNeutrinoAstrophysics - High Energy Astrophysical Phenomenagravitational waves; neutrinos; Astronomy and Astrophysics; Space and Planetary ScienceAstronomical and Space SciencessignaturePhysical Chemistry (incl. Structural)supernova: collapseAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & AstrophysicsGravitational wavesemission [gravitational radiation]Ones gravitacionalsCoincident0103 physical sciencesGravitational Waves Neutrinos LIGO Virgo Antares IceCubeNuclearddc:530Neutrinsenergy: high [neutrino]NeutrinosSTFCAstrophysiqueAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesScience & TechnologyANTARESGravitational waveVirgoOrganic ChemistryAstronomyRCUKMolecularAstronomy and AstrophysicsAstronomieAstronomy and Astrophysic530 PhysikLIGOSciences de l'espaceBlack holemessengerNeutron starAntaresPhysics and AstronomySpace and Planetary ScienceFISICA APLICADA:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]gravitational radiation: emissiondensity [astrophysics]ddc:520[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]EMISSION
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7Be(n,α) and 7Be(n,p) cross-section measurement for the cosmological lithium problem at the n-TOF facility at CERN

2017

One of the most puzzling problems in Nuclear Astrophysics is the “Cosmological Lithium Problem”, i.e the discrepancy between the primordial abundance of \(^{7}\)Li observed in metal poor halo stars (Asplund et al. in Astrophys J 644:229–259, 2006, [1]), and the one predicted by Big Bang Nucleosynthesis (BBN). One of the reactions that could have an impact on the problem is \(^{7}\)Be(n,p)\(^{7}\)Li. Despite of the importance of this reaction in BBN, the cross-section has never been directly measured at the energies of interest for BBN. Taking advantage of the innovative features of the second experimental area at the n\(\_\)TOF facility at CERN (Sabate-Gilarte et al. in Eur Phys J A 53:210,…

AstrofísicanTOFQC1-999chemistry.chemical_elementNeutronAstrophysics01 natural sciences7. Clean energyNuclear physicsPhysics and Astronomy (all)Big Bang nucleosynthesisNucleosynthesisCERN0103 physical sciencesNuclear astrophysicsAstrophysics::Solar and Stellar AstrophysicsNeutron010306 general physicsNuclear ExperimentAstrophysics::Galaxy Astrophysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsPhysicsAlphaLarge Hadron Collider:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsStarschemistryLithiumHaloNucleosynthesisNucleosíntesi
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The n_TOF facility: Neutron beams for challenging future measurements at CERN

2016

The CERN n TOF neutron beam facility is characterized by a very high instantaneous neutron flux, excellent TOF resolution at the 185 m long flight path (EAR-1), low intrinsic background and coverage of a wide range of neutron energies, from thermal to a few GeV. These characteristics provide a unique possibility to perform high-accuracy measurements of neutron-induced reaction cross-sections and angular distributions of interest for fundamental and applied Nuclear Physics. Since 2001, the n TOF Collaboration has collected a wealth of high quality nuclear data relevant for nuclear astrophysics, nuclear reactor technology, nuclear medicine, etc. The overall efficiency of the experimental prog…

AstrofísicanTOF[PHYS.PHYS.PHYS-ACC-PH]Physics [physics]/Physics [physics]/Accelerator Physics [physics.acc-ph]QC1-999Nuclear TheoryNeutronAstrophysics01 natural sciences7. Clean energylaw.inventionNuclear physicsPhysics and Astronomy (all)Neutron fluxlaw0103 physical sciencesCERNNuclear astrophysicsNeutronSpallation010306 general physicsNuclear ExperimentPhysics:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsLarge Hadron Collider:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsPhysicsNuclear dataNuclear reactorNeutron radiationAccelerators and Storage Rings3. Good health13. Climate action
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Efficient generation of energetic ions in multi-ion plasmas by radio-frequency heating

2017

We describe a new technique for the efficient generation of high-energy ions with electromagnetic ion cyclotron waves in multi-ion plasmas. The discussed ‘three-ion’ scenarios are especially suited for strong wave absorption by a very low number of resonant ions. To observe this effect, the plasma composition has to be properly adjusted, as prescribed by theory. We demonstrate the potential of the method on the world-largest plasma magnetic confinement device, JET (Joint European Torus, Culham, UK), and the high-magnetic-field tokamak Alcator C-Mod (Cambridge, USA). The obtained results demonstrate efficient acceleration of 3He ions to high energies in dedicated hydrogen–deuterium mixtures.…

Astrophysical plasmasTokamakradio-frequency heatingCyclotronJoint European TorusPlasma heatingGeneral Physics and AstronomyFREQUENCY114 Physical sciences01 natural sciences7. Clean energyMagnetically confined plasmas010305 fluids & plasmaslaw.inventionIonPHYSICSPhysics and Astronomy (all)FUSIONMODE CONVERSIONlawPhysics::Plasma Physics0103 physical sciencesDielectric heating010306 general physicsPhysics[PHYS]Physics [physics]ta114Solar flare:Física [Àrees temàtiques de la UPC]Plasma dynamicsmulti-ion plasmasSettore FIS/01 - Fisica SperimentaleMagnetic confinement fusionPlasmaHE-3-RICH SOLAR-FLARESTècniques de plasmaJETCYCLOTRON RANGETOKAMAKPhysics::Space PhysicsAtomic physicsHE-3-RICH SOLAR-FLARES; MODE CONVERSION; CYCLOTRON RANGE; FUSION; JET; FREQUENCY; TOKAMAK; PHYSICS
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Search for muon neutrinos from gamma-ray bursts with the ANTARES neutrino telescope using 2008 to 2011 data

2013

Aims. We search for muon neutrinos in coincidence with GRBs with the ANTARES neutrino detector using data from the end of 2007 to 2011. Methods. Expected neutrino fluxes were calculated for each burst individually. The most recent numerical calculations of the spectra using the NeuCosmA code were employed, which include Monte Carlo simulations of the full underlying photohadronic interaction processes. The discovery probability for a selection of 296 GRBs in the given period was optimised using an extended maximum-likelihood strategy. Results. No significant excess over background is found in the data, and 90% confidence level upper limits are placed on the total expected flux according to …

Astrophysics::High Energy Astrophysical PhenomenaNeutrino telescopeMonte Carlo methodgamma-ray burst: generalFOS: Physical sciencesddc:500.201 natural sciencesCoincidenceSpectral lineGamma ray burstsmethods: numericalNuclear physicsneutrinoHigh Energy Physics - Phenomenology (hep-ph)Raigs gamma0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]NeutrinsNeutrinos010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics:Desenvolupament humà i sostenible [Àrees temàtiques de la UPC]Muonnumerical [Methods]010308 nuclear & particles physicsneutrinosAstronomy and Astrophysicsgeneral [Gamma-ray burst]neutrinos - gamma-ray burst: general - methods: numerical; methods: numerical; neutrinos; gamma-ray burst: generalHigh Energy Physics - PhenomenologyGamma-ray burst: general; Methods: numerical; NeutrinosNeutrino detectorSpace and Planetary ScienceFISICA APLICADAFísica nuclearHigh Energy Physics::ExperimentNeutrinoneutrinos - gamma-ray burst: general - methods: numericalGamma-ray burstAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Economía criminal y terror

2001

AtentadosSistema económico mundialCiudadanosGlobalización financieraCorrupción políticaVidal-Beneyto JoséEuros criminalesParaísos fiscales11-SBlanqueoDinero criminalTerrorismoMasa financieraCrisisPublicaciones: Obra periodística: Columnas y artículos de opiniónEconomía criminalVoluntadesDesregulaciónGLOBALIZACIÓNDelincuencia económicaParlamento EuropeoCRIMINALIDADFMIArbitraje internacional
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Successful use of impella CP through femoral access in a patient with bilateral iliac and aortic endoprosthesis in the setting of cardiogenic shock

2019

We report the case of a 67-year-old male, with previous history of severe peripheral vascular disease (abdominal aorta aneurism and bilateral iliac stenosis) requiring the implantation of 3 endoprostheses 7 months ago (Figure 1(A)), and previous myocardial infarction 10 years ago. The left ventricular ejection fraction (LVEF) was preserved at last control (58%). The patient was referred for acute coronary syndrome complicated with pulmonary oedema and cardiogenic shock. Echocardiography showed a severe impairment of LVEF (18%) and the patient was transferred to cathlab for emergency percutaneous coronary intervention (PCI). Coronary angiography via right femoral 7Fr access showed a chronic …

Atherectomy CoronaryMalemedicine.medical_specialtyProstheses and ImplantComputed Tomography AngiographyShock CardiogenicEndoprosthesiCoronary AngiographyHigh risk pciIliac ArteryPercutaneous Coronary InterventionFemoral accessmedicine.arteryCatheterization PeripheralDrug-Eluting Stentmedicinehigh risk PCIHumansAorta AbdominalAcute Coronary SyndromeImpellaPeripheral Vascular DiseasesEndovascular Procedurebusiness.industryVascular diseaseimpellaCardiogenic shockcardiogenic shockEndovascular ProceduresAbdominal aortaDrug-Eluting StentsProstheses and ImplantsGeneral MedicineMiddle Agedmedicine.diseasePeripheralSurgeryFemoral ArteryAcute Coronary Syndrome ...StenosisTreatment OutcomeCardiology and Cardiovascular MedicinebusinessActa Cardiologica
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