Search results for "partícules"

showing 10 items of 522 documents

Photon events with missing energy at root s=183 to 189 GeV

2000

The production of single photons has been studied in the reaction e+e- -> gamma + invisible particles at centre-of-mass energies of 183 GeV and 189 GeV. A previously published analysis of events with multi-photon final states accompanied by missing energy has been updated with 189 GeV data. The data were collected with the DELPHI detector and correspond to integrated luminosities of about 51 pb^{-1} and 158 pb^{-1} at the two energies. The number of light neutrino families is measured to be 2.84 +/- 0.15(stat) +/- 0.14(syst). The absence of an excess of events beyond that expected from Standard Model processes is used to set limits on new physics as described by supersymmetric and compos…

NEUTRALINOSParticle physicsDIMENSIONSPhotonPhysics and Astronomy (miscellaneous)Physics beyond the Standard ModelAstrophysics::High Energy Astrophysical PhenomenaSTANDARD MODELFOS: Physical sciencesScale (descriptive set theory)7. Clean energy01 natural sciencesPartícules (Física nuclear)Standard ModelHigh Energy Physics - ExperimentGravitationHigh Energy Physics - Experiment (hep-ex)E(+)E(-) COLLISIONSSIGNALSSEARCH0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]010306 general physicsNuclear ExperimentEngineering (miscellaneous)DELPHIPhysicsMissing energy010308 nuclear & particles physicsSUPERLIGHT GRAVITINOLEPLARGE ELECTRON POSITRON COLLIDERSINGLE-PHOTONCOLLIDERSPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIPARTICLE PHYSICSProduction (computer science)Física nuclearHigh Energy Physics::ExperimentNeutrinoE(+)E(-) COLLISIONS; SUPERLIGHT GRAVITINO; STANDARD MODEL; SINGLE-PHOTON; COLLIDERS; SEARCH; LEP; NEUTRALINOS; DIMENSIONS; SIGNALSParticle Physics - Experiment
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Search for supersymmetric particles in scenarios with a gravitino LSP and stau NLSP

2000

Sleptons, neutralinos and charginos were searched for in the context of scenarios where the lightest supersymmetric particle is the gravitino. It was assumed that the stau is the next-to-lightest supersymmetric particle. Data collected with the DELPHI detector at a centre-of-mass energy near 189 GeV were analysed combining the methods developed in previous searches at lower energies. No evidence for the production of these supersymmetric particles was found. Hence, limits were derived at 95% confidence level.

NEUTRALINOSParticle physicsPhysics and Astronomy (miscellaneous)LOWEST ORDER CALCULATIONSPAIR PRODUCTIONENERGIESMONTE-CARLO SIMULATIONpluridisciplinarityFOS: Physical sciences2-PHOTON PROCESSESContext (language use)01 natural sciencesLightest Supersymmetric ParticlePartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)E(+)E(-) COLLISIONS0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]RADIATIVE-CORRECTIONSontology010306 general physicsEngineering (miscellaneous)DELPHIPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyreflexivityLEPscience studiesepistemologieLARGE ELECTRON POSITRON COLLIDERhistory of sciencePARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; DELPHIMONTE-CARLO SIMULATION; LOWEST ORDER CALCULATIONS; RADIATIVE-CORRECTIONS; PAIR PRODUCTION; E(+)E(-) COLLISIONS; 2-PHOTON PROCESSES; ENERGIES; BREAKING; LEP; NEUTRALINOSParticlePARTICLE PHYSICSGravitinoFísica nuclearHigh Energy Physics::ExperimentcomplexityParticle Physics - ExperimentBREAKING
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GEANT4 simulation of the neutron background of the C6D6 set-up for capture studies at n_TOF

2014

The neutron sensitivity of the C6D6 detector setup used at n_TOF facility for capture measurements has been studied by means of detailed GEANT4 simulations. A realistic software replica of the entire n_TOF experimental hall, including the neutron beam line, sample, detector supports and the walls of the experimental area has beeni mplemented in the simulations. The simulations have been analyzed in the same manner as experimental data, in particular by applying the Pulse Height Weighting Technique. The simulations have been validated against a measurement of the neutron background performed with anatC sample, showing an excellent agreement above 1 keV. At lower energies, an additional compo…

Neutron captureNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaGEANT4 simulations; Neutron time of flight; Neutron background; n_TOF; Neutron captureFOS: Physical sciencesNeutronN-TOF7. Clean energy01 natural sciencesPartícules (Física nuclear)Nuclear physicsCross section (physics)0103 physical sciencesNeutronNuclear Experiment (nucl-ex)010306 general physicsGEANT4 simulations;N-TOF;Neutron time of flight;Neutron capture;Neutron backgroundNuclear ExperimentInstrumentationphysics.ins-detNuclear ExperimentGEANT4Line (formation)Particles (Nuclear physics)PhysicsBonner sphere:Energies::Energia nuclear [Àrees temàtiques de la UPC]NeutronsGEANT4 simulation:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsDetectorFísicaNeutron sensitivityDetectorInstrumentation and Detectors (physics.ins-det)Neutron radiationNEUTRON TIME OF FLIGHTNeutron captureBackgroundDeuteriumN_TOFGEANT4 simulationsNeutron backgroundSimulation
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Updated determination of the solar neutrino fluxes from solar neutrino data

2016

Journal of High Energy Physics 2016.3 (2016): 132 reproduced by permission of Scuola Internazionale Superiore di Studi Avanzati (SISSA)

Normalization (statistics)Particle physicsNuclear and High Energy PhysicsSolar and atmospheric neutrinosSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaBayesian probabilityPosterior probabilitySolar neutrinosFOS: Physical sciences7. Clean energy01 natural sciencesHigh Energy Physics - Experimentsymbols.namesakeHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Neutrins solars0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010306 general physicsNeutrino oscillationSolar and Stellar Astrophysics (astro-ph.SR)Physics010308 nuclear & particles physicsParticle physicsFísicaMarkov chain Monte CarloNeutrino physicsHigh Energy Physics - PhenomenologyDistribution functionAstrophysics - Solar and Stellar Astrophysics13. Climate actionPhysics::Space PhysicssymbolsAstrophysics::Earth and Planetary AstrophysicsNeutrinoFísica de partícules
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First observation of a baryonic Bc+ decay

2014

A baryonic decay of the $B_c^+$ meson, $B_c^+\to J/\psi p\overline{p}\pi^+$, is observed for the first time, with a significance of $7.3$ standard deviations, in $pp$ collision data collected with the LHCb detector and corresponding to an integrated luminosity of $3.0$ fb$^{-1}$ taken at center-of-mass energies of $7$ and $8$ $\mathrm{TeV}$. With the $B_c^+\to J/\psi \pi^+$ decay as normalization channel, the ratio of branching fractions is measured to be \begin{equation*} \frac{\mathcal{B}(B_c^+\to J/\psi p\overline{p}\pi^+)}{\mathcal{B}(B_c^+\to J/\psi \pi^+)} = 0.143^{\,+\,0.039}_{\,-\,0.034}\,(\mathrm{stat})\pm0.013\,(\mathrm{syst}). \end{equation*} The mass of the $B_c^+$ meson is dete…

Nuclear TheoryAnalytical chemistryGeneral Physics and Astronomy01 natural sciencesSettore FIS/04 - Fisica Nucleare e SubnucleareHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]TOOLFactorizationNuclear ExperimentQCPhysicsPhysicsParticle physics12.39.StPhysical SciencesComputer Science::Mathematical SoftwareFísica nuclearLHCMESONParticle Physics - ExperimentComputer Science::Machine LearningMeson530 Physics14.40.NdPhysics MultidisciplinaryFOS: Physical sciencesPhysics InstituteLHCb - Abteilung HofmannAstrophysics::Cosmology and Extragalactic AstrophysicsComputer Science::Digital LibrariesNONuclear physicsPhysics and Astronomy (all)Hadronic decays of bottom meson0103 physical sciencesPi010306 general physicsScience & Technology010308 nuclear & particles physicshep-exHigh Energy Physics::Phenomenologymeson; toolBaryonLHCb13.25.HwBottom mesons (|B|>0)High Energy Physics::ExperimentFísica de partículesExperiments
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Precision Measurement of the Mass and Lifetime of the Ξ[0 over b] Baryon

2014

Using a proton-proton collision data sample corresponding to an integrated luminosity of 3 fb$^{-1}$ collected by LHCb at center-of-mass energies of 7 and 8 TeV, about 3800 $\Xi_b^0\to\Xi_c^+\pi^-$, $\Xi_c^+\to pK^-\pi^+$ signal decays are reconstructed. From this sample, the first measurement of the $\Xi_b^0$ baryon lifetime is made, relative to that of the $\Lambda_b^0$ baryon. The mass differences $M(\Xi_b^0)-M(\Lambda_b^0)$ and $M(\Xi_c^+)-M(\Lambda_c^+)$ are also measured with precision more than four times better than the current world averages. The resulting values are $\frac{\tau_{\Xi_b^0}}{\tau_{\Lambda_b^0}} = 1.006\pm0.018\pm0.010$, $M(\Xi_b^0) - M(\Lambda_b^0) = 172.44\pm0.39\pm…

Nuclear TheoryAnalytical chemistryGeneral Physics and Astronomyinclusive weak decays; discarding 1/N(C); beaty; charm; ruleLambdaHigh Energy Physics - Experimenthigh energy physicsSettore FIS/04 - Fisica Nucleare e Subnucleare[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]INCLUSIVE WEAK DECAYS; DISCARDING 1/N(C); BEAUTY; CHARM; RULENuclear ExperimentQCPhysicsprecision measurementPhysicsintegrated luminosityParticle physicsBEAUTYtransverse momentaPseudorapidityPhysical SciencesTransverse momentumINCLUSIVE WEAK DECAYSFísica nuclearLHC13.30.Egtellurium compoundsParticle Physics - Experiment530 PhysicsAstrophysics::High Energy Astrophysical PhenomenaPhysics MultidisciplinarypseudorapiditiesPhysics InstituteLHCb - Abteilung HofmannAstrophysics::Cosmology and Extragalactic AstrophysicsCHARMNuclear physicsPhysics and Astronomy (all)Pi14.20.MrScience & Technologycenter-of-mass energiesmass differencetransverse momenta; precision measurement; center-of-mass energies; tellurium compounds; production rates; pseudorapidities; high energy physics; integrated luminosity; hadrons; mass difference; proton proton collisionsDISCARDING 1/N(C)BaryonLHCbproton proton collisionshadronsHadronic decays of baryonBottom baryons (|B|>0)Physics::Accelerator Physicsproduction ratesFísica de partículesExperimentsRULE
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Measurement of the top quark pair production cross section in pp collisions at sqrt(s) = 7 TeV in dilepton final states with ATLAS

2012

A measurement of the production cross section of top quark pairs (t (t) over bar) in proton-proton collisions at a center-of-mass energy of 7 TeV recorded with the ATLAS detector at the Large Hadron Collider is reported. Candidate events are selected in the dilepton topology with large missing transverse energy and at least two jets. Using a data sample corresponding to an integrated luminosity of 35 pb(-1), a t (t) over bar production cross section sigma(t (t) over bar) = 177 +/- 20(stat.) +/- 14(syst.) +/- 7(lum.) pb is measured for an assumed top quark mass of m(t) = 172.5 GeV. A second measurement requiring at least one jet identified as coming from a b quark yields a comparable result,…

Nuclear TheoryHigh Energy Physics::PhenomenologyHigh Energy Physics::ExperimentFísica nuclearNuclear ExperimentPartícules (Física nuclear)
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Four-neutrino oscillations at SNO

2000

We discuss the potential of SNO to constraint the four-neutrino mixing schemes favoured by the results of all neutrino oscillations experiments. These schemes allow simultaneous transitions of solar $\nu_e's$ into active $\nu_\mu$'s, $\nu_\tau$'s and sterile $\nu_s$ controlled by the additional parameter $\cos^2(\vartheta_{23}) \cos^2(\vartheta_{24})$ and they contain as limiting cases the pure $\nu_e$-active and $\nu_e$-sterile neutrino oscillations. We first obtain the solutions allowed by the existing data in the framework of the BP00 standard solar model and quantify the corresponding predictions for the CC and the NC/CC event ratios at SNO for the different allowed regions as a functio…

Nuclear and High Energy PhysicsAstrofísica nuclearOscillationsAstrophysics (astro-ph)High Energy Physics::PhenomenologyFOS: Physical sciencesAstrophysicsPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Phenomenological theory (Physics)AstronomiaFenomenologia (Física)Oscil·lacionsHigh Energy Physics::ExperimentNuclear astrophysicsNeutrinsNeutrinosParticles (Nuclear physics)
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Seasonal dependence in the solar neutrino flux

1999

MSW solutions of the solar neutrino problem predict a seasonal dependence of the zenith angle distribution of the event rates, due to the non-zero latitude at the Super-Kamiokande site. We calculate this seasonal dependence and compare it with the expectations in the no-oscillation case as well as just-so scenario, in the light of the latest Super-Kamiokande 708-day data. The seasonal dependence can be sizeable in the large mixing angle MSW solution and would be correlated with the day-night effect. This may be used to discriminate between MSW and just-so scenarios and should be taken into account in refined fits of the data.

Nuclear and High Energy PhysicsAstrofísica nuclearSolar neutrinoFluxFOS: Physical sciencesContext (language use)AstrophysicsAtmospheric sciencesAstrophysicsPartícules (Física nuclear)LatitudeHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)medicineNeutrinsNeutrinosNeutrino oscillationPhysics::Atmospheric and Oceanic PhysicsMixing (physics)ZenithParticles (Nuclear physics)PhysicsAstrophysics (astro-ph)High Energy Physics::PhenomenologyFísicaSeasonalitySolar neutrino problemmedicine.diseaseAtomic and Molecular Physics and OpticsHigh Energy Physics - PhenomenologyEnvironmental scienceNuclear astrophysicsHigh Energy Physics::ExperimentEvent (particle physics)
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Zenith angle distributions at Super-Kamiokande and SNO and the solution of the solar neutrino problem

2000

We have performed a detailed study of the zenith angle dependence of the regeneration factor and distributions of events at SNO and SK for different solutions of the solar neutrino problem. In particular, we discuss oscillatory behaviour and the synchronization effect in the distribution for the LMA solution, the parametric peak for the LOW solution, etc.. Physical interpretation of the effects is given. We suggest a new binning of events which emphasizes distinctive features of zenith angle distributions for the different solutions. We also find the correlations between the integrated day-night asymmetry and the rates of events in different zenith angle bins. Study of these correlations st…

Nuclear and High Energy PhysicsAstrofísica nuclearmedia_common.quotation_subjectSolar neutrinoSolar neutrinosFOS: Physical sciencesAstrophysicsAstrophysicsAsymmetryPartícules (Física nuclear)High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)Neutrins solarsNeutrino oscillationZenithParametric statisticsmedia_commonParticles (Nuclear physics)PhysicsSistema solarAstrophysics (astro-ph)FísicaSolar neutrino problemHigh Energy Physics - PhenomenologyDistribution (mathematics)High Energy Physics::ExperimentNuclear astrophysicsSuper-KamiokandeSolar system
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