0000000001138731

AUTHOR

M Colomer

showing 3 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
researchProduct

Investigation of the splitting of quark and gluon jets

1998

The splitting processes in identified quark and gluon jets are investigated using longitudinal and transverse observables. The jets are selected from symmetric three-jet events measured in Z decays L with the {\sc Delphi} detector in 1991-1994. Gluon jets are identified using heavy quark anti-tagging. Scaling violations in identified gluon jets are observed for the first time. The scale energy dependence of the gluon fragmentation function is found to be about two times larger than for the corresponding quark jets, consistent with the QCD expectation $C_A/C_F$. The primary splitting of gluons and quarks into subjets agrees with fragmentation models and, for specific regions of the jet resol…

QuarkParticle physicsPhysics and Astronomy (miscellaneous)Electron–positron annihilationAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::LatticeNuclear Theory7. Clean energy01 natural sciencesPartícules (Física nuclear)Nuclear physics0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsHADRONIZATIONEngineering (miscellaneous)ScalingQuantum chromodynamicsPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyObservableQCDPhoton structure functionHadronizationGluonMODELAVERAGE MULTIPLICITIES; QCD; HADRONIZATION; FRAGMENTATION; MODELFísica nuclearHigh Energy Physics::ExperimentFRAGMENTATIONAVERAGE MULTIPLICITIESParticle Physics - Experiment
researchProduct

Measurement of the charged particle multiplicity of weakly decaying B hadrons

1998

From the Z decays recorded in 1994 and 1995 by the DELPHI detector at LEP, the charged particle multiplicity of weakly decaying B hadrons was measured to be: 4.97 +/- 0.03 +/- 0.06 excluding the K-o and Lambda decay products. (C) 1998 Published by Elsevier Science B.V. All rights reserved.

Nuclear and High Energy PhysicsParticle physicsElectron–positron annihilationHadronMICROVERTEX DETECTOR; DELPHI DETECTOR; PHYSICS01 natural sciencesPartícules (Física nuclear)Nuclear physicsPHYSICS0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Multiplicity (chemistry)010306 general physicsDELPHIPhysics010308 nuclear & particles physicsDetectorMICROVERTEX DETECTORDELPHI DETECTORLARGE ELECTRON POSITRON COLLIDERCharged particlePARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSHigh Energy Physics::ExperimentFísica nuclearParticle Physics - Experiment
researchProduct