0000000000777410

AUTHOR

J Schmidt

showing 5 related works from this author

Search for High-energy Neutrinos from Gravitational Wave Event GW151226 and Candidate LVT151012 with ANTARES and IceCube

2017

[EN] The Advanced LIGO observatories detected gravitational waves from two binary black hole mergers during their first observation run (O1). We present a high-energy neutrino follow-up search for the second gravitational wave event, GW151226, as well as for gravitational wave candidate LVT151012. We find two and four neutrino candidates detected by IceCube, and one and zero detected by ANTARES, within +/- 500 s around the respective gravitational wave signals, consistent with the expected background rate. None of these neutrino candidates are found to be directionally coincident with GW151226 or LVT151012. We use nondetection to constrain isotropic-equivalent high-energy neutrino emission …

POINT-LIKEGravitational-wave observatoryPhysics and Astronomy (miscellaneous)[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]AstronomyELECTROMAGNETIC COUNTERPARTSastro-ph.HE; astro-ph.HEAstrophysics01 natural sciences7. Clean energylocalizationIceCubeBinary black holeLIGO010303 astronomy & astrophysicsTelescopeGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEFollow-upData-acquisition systemobservatoryNeutrino detectorElectromagnetic counterpartsSIMULATIONBlack-hole mergersLigoGamma-ray burstsNeutrinoAstrophysics - High Energy Astrophysical PhenomenaHost galaxiesSimulationGravitational waveBLACK-HOLE MERGERSAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesDATA-ACQUISITION SYSTEMGravitational wavesneutrino: productionGeneral Relativity and Quantum CosmologyBinary black holeOnes gravitacionalsLiGO Observatory0103 physical sciencesNeutrinoGW151226ddc:530NeutrinsNeutrinos010306 general physicsPoint-likeANTARESCosmologiaGravitational wavebackgroundgravitational radiationAstronomy530 PhysikLIGONeutron starGravitational Waves Neutrinos Antares IceCube LIGOAntaresPhysics and Astronomyblack hole: binary13. Climate action:Física::Astronomia i astrofísica [Àrees temàtiques de la UPC]FISICA APLICADAAstronomiaDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]FOLLOW-UPPhysical Review D. Particles and Fields
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Edoxaban versus warfarin for the treatment of symptomatic venous thromboembolism

2013

BackgroundWhether the oral factor Xa inhibitor edoxaban can be an alternative to warfarin in patients with venous thromboembolism is unclear. MethodsIn a randomized, double-blind, noninferiority study, we randomly assigned patients with acute venous thromboembolism, who had initially received heparin, to receive edoxaban at a dose of 60 mg once daily, or 30 mg once daily (e.g., in the case of patients with creatinine clearance of 30 to 50 ml per minute or a body weight below 60 kg), or to receive warfarin. Patients received the study drug for 3 to 12 months. The primary efficacy outcome was recurrent symptomatic venous thromboembolism. The principal safety outcome was major or clinically re…

MESH: Pulmonary EmbolismMale[SDV]Life Sciences [q-bio]Kaplan-Meier Estimate030204 cardiovascular system & hematologylaw.inventionMESH: Venous Thromboembolismchemistry.chemical_compound0302 clinical medicineRandomized controlled trialEdoxabanlawMESH: Double-Blind Method030212 general & internal medicineMESH: WarfarinMESH: AgedMESH: Middle AgedHazard ratioGeneral MedicineVenous ThromboembolismMiddle AgedThrombosis3. Good healthPulmonary embolismAnesthesiaFemaleAnticoagulants EdoxabanMESH: HemorrhageAndexanet alfamedicine.drugMESH: EnoxaparinHemorrhageMESH: AnticoagulantsMESH: Drug Administration ScheduleDrug Administration Schedule03 medical and health sciencesDouble-Blind MethodAged; Anticoagulants; Double-Blind Method; Drug Administration Schedule; Enoxaparin; Female; Hemorrhage; Humans; Kaplan-Meier Estimate; Male; Middle Aged; Pulmonary Embolism; Venous Thromboembolism; WarfarinmedicineHumansEnoxaparinAdverse effectMESH: Kaplan-Meier EstimateAgedMESH: Humansbusiness.industryWarfarinAnticoagulantsmedicine.diseaseMESH: MalechemistryWarfarinbusinessPulmonary EmbolismMESH: FemaleNew England Journal of Medicine
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Direct search for light gluinos

1999

We present the results for a direct search for light gluinos through the appearance of $\eta\rightarrow 3\pi^{0}$ with high transverse momentum in the vacuum tank of the NA48 experiment at CERN. We find one event within a lifetime range of $10^{-9}-10^{-3}$s and another one between $10^{-10}-10^{-9}$s. Both events are consistent with the expected background from neutrons in the beam, produced by 450 GeV protons impinging on the Be targets, which interact with the residual air in the tank. From these data we give limits on the production of the hypothetical $g\widetilde{g}$ bound state, the $R^0$ hadron, and its $R^0\rightarrow\eta\widetilde{\gamma}$ decay in the $R^0$ mass range between 1 a…

PhysicsgluinoNuclear and High Energy PhysicsParticle physicsGluinoRange (particle radiation)Large Hadron ColliderHadronNA48 experimentSupersymmetrysupersymmetry gluinoNuclear physicsBound stateHigh Energy Physics::ExperimentNeutronsupersymmetryNuclear ExperimentParticle Physics - Experiment
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The beam and detector for the NA48 neutral kaon CP violation experiment at CERN

2007

The beam and detector, used for the NA48 experiment, devoted to the measurement of Re (ε{lunate}′ / ε{lunate}), and for the NA48/1 experiment on rare KS and neutral hyperon decays, are described. © 2007 Elsevier B.V. All rights reserved.

Nuclear and High Energy PhysicsParticle physicsacceleratoriNA62 experiment01 natural sciencesLIQUID-KRYPTON CALORIMETERDECAYSNOfasci di particelleKaon beamsNuclear physicsDRIFT CHAMBER ELECTRONICSCERNViolazione di CP0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Kaon decaysdetector; CP violation; Kaon decays010306 general physicsInstrumentation07.05.Fb; 13.20.Eb; 29.40.Vj; 29.27.EgPhysicsCalorimeterLarge Hadron ColliderdetectorCRYSTAL010308 nuclear & particles physicsLIQUID-KRYPTON CALORIMETER; DRIFT CHAMBER ELECTRONICS; PROTON TAGGING DETECTOR; PC FARM; TRIGGER; SYSTEM; READOUT; DECAYS; PERFORMANCE; CRYSTALDetectorPC FARMHyperonNA48 experimentDetectorsMagnetic spectrometerPERFORMANCErivelatoriREADOUTkaon decayCalorimeterTriggerCP violationfasci di particelle; acceleratori; CERN; Violazione di CP; rivelatori; kaon decayCP violationHigh Energy Physics::ExperimentParticle Physics - ExperimentPROTON TAGGING DETECTORSYSTEMBeam (structure)
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Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

2017

On 2017 August 17, the gravitational-wave event GW170817 was observed by the Advanced LIGO and Virgo detectors, and the gamma-ray burst (GRB) GRB 170817A was observed independently by the Fermi Gamma-ray Burst Monitor, and the Anticoincidence Shield for the Spectrometer for the International Gamma-Ray Astrophysics Laboratory. The probability of the near-simultaneous temporal and spatial observation of GRB 170817A and GW170817 occurring by chance is $5.0\times 10^{-8}$. We therefore confirm binary neutron star mergers as a progenitor of short GRBs. The association of GW170817 and GRB 170817A provides new insight into fundamental physics and the origin of short gamma-ray bursts. We use the ob…

AstrofísicaGravitacióneutron star: binaryclose [binaries]Astronomy[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]BATSE OBSERVATIONSgamma-ray burst: generalEQUIVALENCE PRINCIPLEEXTENDED EMISSIONastro-ph.HE; astro-ph.HEAstrophysicsKilonovageneral [gamma-ray burst]01 natural sciences7. Clean energyGeneral Relativity and Quantum Cosmologyphoton: velocityPROMPT EMISSIONLIGOclose gamma-ray burst: general gravitational waves [binaries]gravitational wave010303 astronomy & astrophysicsGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)BURST SPECTRAQCQBPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)binaries: closeGRBEQUATION-OF-STATEviolation: Lorentzgamma ray: emissiongravitational wavesAstrophysics - High Energy Astrophysical PhenomenaGWradiation: electromagneticAfterglow Light CurvesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstinvariance: LorentzGW GRB LIGO Virgo Fermi BNSGLASTOptical Afterglows0103 physical sciencesgamma ray: detectorBinaries: close; gamma-ray burst: general; gravitational wavesSTFCFermi010308 nuclear & particles physicsGravitational waveVirgogravitational radiationRCUKAstronomy and AstrophysicsAstronomy and Astrophysictime delaysensitivityShapiro delayLIGORedshiftNeutron starVIRGOPhysics and AstronomyHOST GALAXYCPT VIOLATION13. Climate actiongravitationSpace and Planetary ScienceLUMINOSITY FUNCTIONVIEWING ANGLEbinaries: close; gamma-ray burst: general; gravitational waves; Astronomy and Astrophysics; Space and Planetary ScienceBNSspectrometerGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]redshift: measuredFermi Gamma-ray Space TelescopeAstrophysical Journal Letters
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