0000000000188611

AUTHOR

Anne Robert

showing 8 related works from this author

First observation of the doubly charmed baryon decay Ξcc++→Ξc+π+

2018

The doubly charmed baryon decay Ξcc++→Ξc+π+ is observed for the first time, with a statistical significance of 5.9σ, confirming a recent observation of the baryon in the Λc+K−π+π+ final state. The data sample used corresponds to an integrated luminosity of 1.7 fb−1, collected by the LHCb experiment in pp collisions at a center-of-mass energy of 13 TeV. The Ξcc++ mass is measured to be 3620.6±1.5(stat)±0.4(syst)±0.3(Ξc+) MeV/c2 and is consistent with the previous result. The ratio of branching fractions between the decay modes is measured to be [B(Ξcc++→Ξc+π+)×B(Ξc+→pK−π+)]/[B(Ξcc++→Λc+K−π+π+)×B(Λc+→pK−π+)]=0.035±0.009(stat)±0.003(syst).

Particles and fieldGeneral Physics and Astronomy01 natural sciencesNONuclear physicsPhysics and Astronomy (all)Condensed Matter::Superconductivity0103 physical sciencesPhysicLHCb - Abteilung HintonSDG 7 - Affordable and Clean Energy010306 general physicsPhysics/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energy010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyParticle physicsHEPBaryonLHCbCharmed baryonHadron colliderHigh Energy Physics::ExperimentB physics Branching fraction CP violation Hadron-Hadron scattering (experiments)LHCFísica de partículesExperiments
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Interaction of iron(II)-heme and artemisinin with a peptide mimic of Plasmodium falciparum HRP-II

2007

Abstract The interaction of heme or heme-artemisinin adducts (heme-art) with different peptides mimicking repeat sequences of the Histidine-Rich-Protein-II of Plasmodium falciparum (PfHRP-II) was investigated. The pseudo-first order rate constants of the coordination of heme or heme-art onto a histidine rich peptide, used as a mimic of PfHRP-II putative heme binding sequence, are of the same order of magnitude, namely 42 and 14 s −1 , respectively. Despite the intrinsic reactivity of the carbonyl at C10 of heme-art toward a hydroxyl function, a peptide containing a serine or threonine residue does not readily react with heme-art adducts. Therefore, a much higher affinity of heme-art compare…

Heme bindingStereochemistryIronPlasmodium falciparumProtozoan ProteinsmalariaPeptide010402 general chemistry01 natural sciencesBiochemistryInorganic Chemistry03 medical and health scienceschemistry.chemical_compoundResidue (chemistry)[ SDV.BBM.BC ] Life Sciences [q-bio]/Biochemistry Molecular Biology/Biomolecules [q-bio.BM]hemozoinAnimals[SDV.BBM.BC]Life Sciences [q-bio]/Biochemistry Molecular Biology/Biochemistry [q-bio.BM]hemeHemealkylationHistidineComputingMilieux_MISCELLANEOUS030304 developmental biologychemistry.chemical_classification0303 health sciencesMolecular StructurebiologyHemozoinMolecular MimicryProteinsPlasmodium falciparumbiology.organism_classificationArtemisininsProtein tertiary structure3. Good health0104 chemical sciencesKineticsModels ChemicalchemistryBiochemistryartemisininPeptidesProtein Binding
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Updated determination of D0–D¯0 mixing and CP violation parameters with D0→K+π− decays

2018

We report measurements of charm-mixing parameters based on the decay-time-dependent ratio of D0→K+π- to D0→K-π+ rates. The analysis uses a data sample of proton-proton collisions corresponding to an integrated luminosity of 5.0  fb-1 recorded by the LHCb experiment from 2011 through 2016. Assuming charge-parity (CP) symmetry, the mixing parameters are determined to be x′2=(3.9±2.7)×10-5, y′=(5.28±0.52)×10-3, and RD=(3.454±0.031)×10-3. Without this assumption, the measurement is performed separately for D0 and D¯0 mesons, yielding a direct CP-violating asymmetry AD=(-0.1±9.1)×10-3, and magnitude of the ratio of mixing parameters 1.00<|q/p|<1.35 at the 68.3% confidence level. All results incl…

PhysicsParticle physicsLuminosity (scattering theory)Meson010308 nuclear & particles physicsmedia_common.quotation_subject01 natural sciencesAsymmetrySymmetry (physics)0103 physical sciencesCP violationCharm (quantum number)010306 general physicsMixing (physics)Bar (unit)media_commonPhysical Review D
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Measurement of atmospheric neutrino oscillations with the ANTARES neutrino telescope

2012

The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximal mixing, a mass …

Nuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Physics::Instrumentation and DetectorsSolar neutrinoAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesddc:500.2Neutrino telescope01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Experiment0103 physical sciencesNeutrinsHigh Energy PhysicsNeutrinos010306 general physicsNeutrino oscillationPhysicsMuonANTARES:Física [Àrees temàtiques de la UPC]010308 nuclear & particles physicsNeutrino oscillations[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]High Energy Physics::PhenomenologySolar neutrino problemNeutrino astrophysicsCosmic neutrino backgroundNeutrino detectorFISICA APLICADAMeasurements of neutrino speedFísica nuclearHigh Energy Physics::ExperimentNeutrino[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Physics Letters B
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Measurement of the c0 Baryon Lifetime

2018

We report a measurement of the lifetime of the $��_c^0$ baryon using proton-proton collision data at center-of-mass energies of 7 and 8~TeV, corresponding to an integrated luminosity of 3.0 fb$^{-1}$ collected by the LHCb experiment. The sample consists of about 1000 $��_b^-\to��_c^0��^-\bar��_�� X$ signal decays, where the $��_c^0$ baryon is detected in the $pK^-K^-��^+$ final state and $X$ represents possible additional undetected particles in the decay. The $��_c^0$ lifetime is measured to be $��_{��_c^0} = 268\pm24\pm10\pm2$ fs, where the uncertainties are statistical, systematic, and from the uncertainty in the $D^+$ lifetime, respectively. This value is nearly four times larger than, …

Particles and fieldGeneral PhysicsMesonGeneral Physics and AstronomyFOS: Physical sciences01 natural sciences7. Clean energyOmega09 EngineeringNOLuminosityHigh Energy Physics - Experiment (hep-ex)Physics and Astronomy (all)0103 physical sciencesPhysicHeavy baryonTOOLSDG 7 - Affordable and Clean EnergyLHCb - Abteilung Hinton010306 general physicsINCLUSIVE WEAK DECAYS; DISCARDING 1/N(C); RULE; TOOL01 Mathematical SciencesQuantum chromodynamicsPhysics/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energy02 Physical Sciences010308 nuclear & particles physicsQuark modelParticle physicsState (functional analysis)HEPDISCARDING 1/N(C)BaryonLHCbHadron colliderHigh Energy Physics::ExperimentINCLUSIVE WEAK DECAYSLHCAtomic physicsFísica de partículesExperimentsRULECharm physics Oscillation Flavor physics Hadron-Hadron scattering
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Measurement of the neutrino-oxygen neutral-current interaction cross section by observing nuclear deexcitation gamma rays

2014

We report the first measurement of the neutrino-oxygen neutral-current quasielastic (NCQE) cross section. It is obtained by observing nuclear deexcitation $\gamma$-rays which follow neutrino-oxygen interactions at the Super-Kamiokande water Cherenkov detector. We use T2K data corresponding to $3.01 \times 10^{20}$ protons on target. By selecting only events during the T2K beam window and with well-reconstructed vertices in the fiducial volume, the large background rate from natural radioactivity is dramatically reduced. We observe 43 events in the $4-30$ MeV reconstructed energy window, compared with an expectation of 51.0, which includes an estimated 16.2 background events. The background …

Nuclear and High Energy PhysicsCherenkov detectorPhysics::Instrumentation and DetectorsC-12FOS: Physical sciencesAstronomy & Astrophysicslaw.inventionHigh Energy Physics - ExperimentPhysics Particles & FieldsNuclear physicsSUPER-KAMIOKANDE DETECTORCross section (physics)High Energy Physics - Experiment (hep-ex)lawEXCITATIONABSORPTION[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]SCATTERINGO-16Nuclear ExperimentPhysicsCALIBRATIONScience & TechnologyNeutral currenthep-exPhysicsGamma rayT2K experimentFísica3. Good healthPhysical SciencesNeutrinoWEAKFiducial markerBeam (structure)
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A method for detection of muon induced electromagnetic showers with the ANTARES detector

2012

The primary aim of ANTARES is neutrino astronomy with upward going muons created in charged current muon neutrino interactions in the detector and its surroundings. Downward going muons are background for neutrino searches. These muons are the decay products of cosmic-ray collisions in the Earths atmosphere far above the detector. This paper presents a method to identify and count electromagnetic showers induced along atmospheric muon tracks with the ANTARES detector. The method is applied to both cosmic muon data and simulations and its applicability to the reconstruction of muon event energies is demonstrated. © 2012 Elsevier B.V. All rights reserved.

Physics::Instrumentation and DetectorsAtmospheric muonsDecay productsNeutrino telescopeElectromagnetic shower identification01 natural sciences7. Clean energyneutrino telescope electromagnetic shower identification high energy muons energy reconstruction; high energy muons; neutrino telescope; electromagnetic shower identification; energy reconstructionMuon neutrinoNEUTRINO TELESCOPE010303 astronomy & astrophysicsInstrumentationEnergy reconstructionPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[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]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsHigh energy muonNeutrino detectorMuon colliderNeutrino astronomyFísica nuclearNeutrinoNeutrino telescope; Energy reconstruction; High energy muonsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFLUXNuclear and High Energy PhysicsParticle physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Charged current[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic rayMuon neutrinoNuclear physicsElectromagnetism0103 physical sciencesHigh energy physicsneutrino telescope electromagnetic shower identification high energy muons energy reconstructionInstrumentation and Methods for Astrophysics (astro-ph.IM)MuonANTARES010308 nuclear & particles physicsCharged particles[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]FISICA APLICADATEVPhysics::Accelerator PhysicsHigh Energy Physics::ExperimentNeutrino astronomyNeutrino telescopesElectro-magnetic showersHigh energy muons
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Measurement of the Inclusive NuMu Charged Current Cross Section on Carbon in the Near Detector of the T2K Experiment

2013

T2K has performed the first measurement of nu(mu) inclusive charged current interactions on carbon at neutrino energies of similar to 1 GeV where the measurement is reported as a flux-averaged double differential cross section in muon momentum and angle. The flux is predicted by the beam Monte Carlo and external data, including the results from the NA61/SHINE experiment. The data used for this measurement were taken in 2010 and 2011, with a total of 10.8 x 10(19) protons-on-target. The analysis is performed on 4485 inclusive charged current interaction candidates selected in the most upstream fine-grained scintillator detector of the near detector. The flux-averaged total cross section is (…

Nuclear and High Energy PhysicsHigher educationPhysics::Instrumentation and DetectorsAstrophysics::High Energy Astrophysical PhenomenaNeutrino reactionsLibrary scienceFOS: Physical sciencesddc:500.201 natural sciences7. Clean energyNeutrino scatteringHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Early career010306 general physicsNuclear ExperimentPhysics010308 nuclear & particles physicsbusiness.industry4. EducationNuclear TargetsT2K experimentFísicaRussian federationChristian ministryAngular dependenceHigh Energy Physics::Experimentbusiness
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