Search results for "HIGH ENERGIES"

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Observation of $Z$ production in proton-lead collisions at LHCb

2014

The first observation of $Z$ boson production in proton-lead collisions at a centre-of-mass energy per proton-nucleon pair of $\sqrt{s_{NN}}=5~\text{TeV}$ is presented. The data sample corresponds to an integrated luminosity of $1.6~\text{nb}^{-1}$ collected with the LHCb detector. The $Z$ candidates are reconstructed from pairs of oppositely charged muons with pseudorapidities between 2.0 and 4.5 and transverse momenta above $20~\text{GeV}/c$. The invariant dimuon mass is restricted to the range $60-120~\text{GeV}/c^2$. The $Z$ production cross-section is measured to be \begin{eqnarray*} ��_{Z\to��^+��^-}(\text{fwd})&=&13.5^{+5.4}_{-4.0}\text{(stat.)}\pm1.2\text{(syst.)}~\text{nb} …

14.70.Hp - Z bosonProtonNuclear Theory01 natural sciencesPhysics Particles & FieldsHigh Energy Physics - ExperimentSettore FIS/04 - Fisica Nucleare e SubnucleareLuminosityHigh Energy Physics - Experiment (hep-ex)Heavy-ion collision[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Electroweak interaction; Forward physics; Heavy Ions; Heavy-ion collision; Particle and resonance productionElectroweak interactionHeavy IonsHeavy IonNuclear ExperimentQCBosonPhysics25.75.Dw - Relativistic heavy-ion collisions: Particle and resonance production; 14.70.Hp - Z bosons; 13.38.Dg - Decays of Z bosons; 12.15.-y - Electroweak interactionsPhysicsHIGH ENERGIES12.15.-y - Electroweak interactionsParticle physicsComputer Science::Computation and Language (Computational Linguistics and Natural Language and Speech Processing)13.38.Dg - Decays of Z bosons25.75.Dw - Relativistic heavy-ion collisions: Particle and resonance productionPhysical SciencesPARTON DISTRIBUTIONS; BOSON PRODUCTION; HIGH ENERGIES; NUCLEAR PDFS; DEUTERIUM; DECAYFísica nuclearProduction (computer science)14.70.Hp - Z bosonsParticle Physics - ExperimentNuclear and High Energy PhysicsParticle physicsNUCLEAR PDFS530 PhysicsDEUTERIUMFOS: Physical sciencesPhysics InstituteLHCb - Abteilung HofmannHadronsParticle and resonance production0103 physical sciencesElectroweak interaction; Forward physics; Heavy Ions; Heavy-ion collision; Particle and resonance production; Nuclear and High Energy PhysicsSDG 7 - Affordable and Clean Energy010306 general physicsForward physicLarge Hadron Collider (France and Switzerland)BOSON PRODUCTION/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyScience & TechnologyMuon010308 nuclear & particles physicshep-exComputer Science::Information RetrievalGran Col·lisionador d'Hadrons13.38.Dg - Decays of Z bosonPARTON DISTRIBUTIONSForward physicsHigh Energy Physics::ExperimentFísica de partículesExperimentsDECAYEnergy (signal processing)JHEP
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The ANTARES telescope neutrino alert system

2012

The ANTARES telescope has the capability to detect neutrinos produced in astrophysical transient sources. Potential sources include gamma-ray bursts, core collapse supernovae, and flaring active galactic nuclei. To enhance the sensitivity of ANTARES to such sources, a new detection method based on coincident observations of neutrinos and optical signals has been developed. A fast online muon track reconstruction is used to trigger a network of small automatic optical telescopes. Such alerts are generated for special events, such as two or more neutrinos, coincident in time and direction, or single neutrinos of very high energy.

Optical telescopesPhysics::Instrumentation and DetectorsAstrophysics7. Clean energy01 natural sciencesGamma ray burstsFOLLOW-UP OBSERVATIONSlaw.inventionlawFlaring activeVery high energiesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsGAMMA-RAY BURSTS[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astrophysics::Instrumentation and Methods for AstrophysicsSupernovaNeutrino detectorNeutrino astronomyFísica nuclearNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFLUX[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 PhenomenaFOS: Physical sciencesOptical telescopeTelescopeMuon tracksCoincidentSEARCHDetection methods0103 physical sciencesCore collapse supernovae010306 general physicsOptical follow-upInstrumentation and Methods for Astrophysics (astro-ph.IM)Neutronsantares; neutrino astronomy; optical follow-up; transient sourcesANTARES010308 nuclear & particles physicsGamma raysAstronomyAstronomy and AstrophysicsAlert systemsStarsTransient sources[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Optical signalsPotential sources13. Climate actionFISICA APLICADAHigh Energy Physics::ExperimentNeutrino astronomyGamma-ray burst
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