0000000001163405

AUTHOR

M Wolf

showing 7 related works from this author

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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Lateral distribution of muons in IceCube cosmic ray events

2013

In cosmic ray air showers, the muon lateral separation from the center of the shower is a measure of the transverse momentum that the muon parent acquired in the cosmic ray interaction. IceCube has observed cosmic ray interactions that produce muons laterally separated by up to 400 m from the shower core, a factor of 6 larger distance than previous measurements. These muons originate in high pT (>2  GeV/c) interactions from the incident cosmic ray, or high-energy secondary interactions. The separation distribution shows a transition to a power law at large values, indicating the presence of a hard pT component that can be described by perturbative quantum chromodynamics. However, the ra…

Nuclear and High Energy PhysicsENERGIESPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayAstrophysicsddc:500.201 natural sciences7. Clean energyPower lawIceCubeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0103 physical sciencescosmic radiation : interactionddc:530Charm (quantum number)Ultra-high-energy cosmic ray010306 general physicsZenithPhysicsQuantum chromodynamicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Muon010308 nuclear & particles physicsAstrophysics::Instrumentation and Methods for AstrophysicsGluonMODELPhysics and Astronomy13. Climate actionTEVHigh Energy Physics::ExperimentGLUONAstrophysics - High Energy Astrophysical Phenomena
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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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Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector

2013

We report on results of an all-sky search for high-energy neutrino events interacting within the IceCube neutrino detector conducted between May 2010 and May 2012. The search follows up on the previous detection of two PeV neutrino events, with improved sensitivity and extended energy coverage down to approximately 30 TeV. Twenty-six additional events were observed, substantially more than expected from atmospheric backgrounds. Combined, both searches reject a purely atmospheric origin for the twenty-eight events at the $4\sigma$ level. These twenty-eight events, which include the highest energy neutrinos ever observed, have flavors, directions, and energies inconsistent with those expected…

Particle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)General Science & TechnologyPhysics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2AstrophysicsIceCube Collaboration01 natural sciences7. Clean energyHigh Energy Physics - ExperimentIceCube Neutrino ObservatoryIceCubeHigh Energy Physics - Experiment (hep-ex)MD Multidisciplinary0103 physical sciences010303 astronomy & astrophysicsastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Multidisciplinaryhep-ex010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyneutrinosSolar neutrino problemKM3NeTNeutrino detector13. Climate actionastro-ph.COMeasurements of neutrino speedHigh Energy Physics::Experimentddc:500NeutrinoNeutrino astronomyAstrophysics - High Energy Astrophysical PhenomenaphysicsAstrophysics - Cosmology and Nongalactic AstrophysicsScience
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Precision electroweak measurements on the Z resonance

2005

We report on the final electroweak measurements performed with data taken at the Z resonance by the experiments operating at the electron-positron colliders SLC and LEP. The data consist of 17 million Z decays accumulated by the ALEPH, DELPHI, L3 and OPAL experiments at LEP, and 600 thousand Z decays by the SLD experiment using a polarised beam at SLC. The measurements include cross-sections, forward-backward asymmetries and polarised asymmetries. The mass and width of the Z boson, $\MZ$ and $\GZ$, and its couplings to fermions, for example the $\rho$ parameter and the effective electroweak mixing angle, are precisely measured. The number of light neutrino species is determined to be 2.9840…

Top quarkFORWARD-BACKWARD ASYMMETRYPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; ALEPH; DELPHI; L3; OPALGeneral Physics and Astronomy01 natural sciences7. Clean energyHigh Energy Physics - ExperimentSettore FIS/04 - Fisica Nucleare e SubnucleareHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)electron-positron physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Electroweak interactionPhysicsQuantum chromodynamicsOPALElectron–positron physics; Electroweak interactions; Decays of heavy intermediate gauge bosons; Fermion–antifermion production; Precision measurements at the Z resonance; Tests of the Standard Model; Radiative corrections; Effective coupling constants; Neutral weak current; Z boson; W boson; Top quark; Higgs bosonParticle physics - ExperimentPhysicsSettore FIS/01 - Fisica SperimentaleElectroweak interactionFORWARD-BACKWARD ASYMMETRY; FERMION-PAIR PRODUCTION; HADRONIC-Z-DECAYS; TOP-QUARK MASS; ANGLE BHABHA SCATTERING; W-BOSON MASS; CROSS-SECTION ASYMMETRY; Z-LINE-SHAPE; SEMILEPTONIC BRANCHING RATIOS; CARLO EVENT GENERATORdecays of heavy intermediate gauge bosons; effective coupling constants; electron-positron physics; electroweak interactions; fermion-antifermion production; higgs boson; neutral weak current; precision measurements at the z resonance; radiative corrections; tests of the standard model; top quark; w boson; z bosonRadiative correctionsALEPHLARGE ELECTRON POSITRON COLLIDERRadiative correctionHigh Energy Physics - PhenomenologyFIS/01 - FISICA SPERIMENTALEDecays of heavy intermediate gauge bosonsL3Z-LINE-SHAPEHiggs bosonFERMION-PAIR PRODUCTIONPARTICLE PHYSICSFísica nuclearNeutrinoFermion–antifermion productionPrecision measurements at the Z resonanceTests of the Standard ModelParticle physicsZ bosonfermion-antifermion productionElectroweak interactionsHiggs bosonFOS: Physical sciencesddc:500.2Elementary particle physics ; z boson ; LEP ; electroweakDecays of heavy intermediate gauge bosonEffective coupling constantPartícules (Física nuclear)Standard ModelNeutral weak currentelectroweak theory Z boson DELPHI ALEPH OPAL L30103 physical sciencesANGLE BHABHA SCATTERINGCROSS-SECTION ASYMMETRYSEMILEPTONIC BRANCHING RATIOS010306 general physicsTOP-QUARK MASSEffective coupling constantsDELPHICoupling constantElectron–positron physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFermionCARLO EVENT GENERATORTop quarkW-BOSON MASSFORWARD-BACKWARD ASYMMETRY FERMION-PAIR PRODUCTION HADRONIC-Z-DECAYS TOP-QUARK MASS ANGLE BHABHA SCATTERING W-BOSON MASS CROSS-SECTION ASYMMETRY Z-LINE-SHAPE SEMILEPTONIC BRANCHING RATIOS CARLO EVENT GENERATOR[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Experimental High Energy PhysicsElectron–positron physicW bosonHigh Energy Physics::ExperimentFIS/04 - FISICA NUCLEARE E SUBNUCLEAREHADRONIC-Z-DECAYSPHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS
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Search for correlations between the arrival directions of IceCube neutrino events and ultrahigh-energy cosmic rays detected by the Pierre Auger Obser…

2016

This paper presents the results of different searches for correlations between very high-energy neutrino candidates detected by IceCube and the highest-energy cosmic rays measured by the Pierre Auger Observatory and the Telescope Array. We first consider samples of cascade neutrino events and of high-energy neutrino-induced muon tracks, which provided evidence for a neutrino flux of astrophysical origin, and study their cross-correlation with the ultrahigh-energy cosmic ray (UHECR) samples as a function of angular separation. We also study their possible directional correlations using a likelihood method stacking the neutrino arrival directions and adopting different assumptions on the size…

AstronomyAstrophysicsNeutrino experiments ultra high energy cosmic rays cosmic ray experiments neutrino astronomy.01 natural sciencesASTROPHYSICAL SOURCESultra high energy cosmic raylaw.inventionIceCubeAstronomi astrofysik och kosmologimagnetic [deflection]lawAstronomy Astrophysics and Cosmologycosmic ray experiments; neutrino astronomy; neutrino experiments; ultra high energy cosmic rays; Astronomy and Astrophysics010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAngular distanceAstrophysics::Instrumentation and Methods for AstrophysicsVHE [neutrino]GALACTIC MAGNETIC-FIELDcascadeAugerobservatorycosmic radiationCascadestackingcosmic ray experi- mentsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearNeutrinoAstrophysics - High Energy Astrophysical Phenomenaphysics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::High Energy Astrophysical Phenomenacosmic ray experimentFOS: Physical sciencesCosmic rayultra high energy cosmic raysSURFACE DETECTORTelescopeneutrino astronomyneutrino experiments0103 physical sciencesddc:530Angular resolutionHigh Energy PhysicsPierre Auger ObservatorySPECTRUMMuon010308 nuclear & particles physicsAstronomy and Astrophysicsflux [neutrino]ASTROFÍSICAPhysics and Astronomyangular resolutioncorrelationExperimental High Energy Physicsneutrino experimenttracks [muon]cosmic ray experiments
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A Hydrogel Derived From Decellularized Dermal Extracellular Matrix. Biomaterials

2012

The ECM of mammalian tissues has been used as a scaffold to facilitate the repair and reconstruction of numerous tissues. Such scaffolds are prepared in many forms including sheets, powders, and hydrogels. ECM hydrogels provide advantages such as injectability, the ability to fill an irregularly shaped space, and the inherent bioactivity of native matrix. However, material properties of ECM hydrogels and the effect of these properties upon cell behavior are neither well understood nor controlled. The objective of this study was to prepare and determine the structure, mechanics, and the cell response in vitro and in vivo of ECM hydrogels prepared from decellularized porcine dermis and urinar…

ScaffoldHydrogelCell viabilityViscoelasticityECM (extracellular matrix)Surface topography
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