0000000000476825

AUTHOR

J. Li

showing 75 related works from this author

Search for the pair production of scalar top quarks in the acoplanar charm jet final state in collisions at

2007

A search for the pair production of scalar top quarks, {bar t}, has been performed in 360 pb{sup -1} of data from p{bar p} collisions at a center-of-mass energy of 1.96 TeV, collected by the D0 detector at the Fermilab Tevatron collider. The {bar t} decay mode considered is {bar t} {yields} c{bar {chi}}{sub 1}{sup 0}, where {bar {chi}}{sub 1}{sup 0} is the lightest supersymmetric particle. The topology analyzed therefore consists of a pair of acoplanar heavy-flavor jets with missing transverse energy. The data show good agreement with the standard model expectation, and a 95% C.L. exclusion domain in the (m{sub {tilde t}}, m{sub {tilde {chi}}{sub 1}{sup 0}}) plane has been determined, exten…

QuarkPhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTevatronSupersymmetry01 natural sciences7. Clean energyLightest Supersymmetric ParticleStandard Modellaw.inventionNuclear physicsPair productionlaw0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsColliderEnergy (signal processing)Physics Letters B
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Measurement of the top quark mass in the dilepton channel

2007

We present a measurement of the top quark mass in the dilepton channel based on approximately 370/pb of data collected by the D0 experiment during Run II of the Fermilab Tevatron collider. We employ two different methods to extract the top quark mass. We show that both methods yield consistent results using ensemble tests of events generated with the D0 Monte Carlo simulation. We combine the results from the two methods to obtain a top quark mass m_t = 178.1 +/- 8.2 GeV. The statistical uncertainty is 6.7 GeV and the systematic uncertainty is 4.8 GeV.

Nuclear and High Energy PhysicsParticle physicsTop quarkMonte Carlo methodTevatronFOS: Physical sciences01 natural sciencesBottom quarkHigh Energy Physics - Experimentlaw.inventionNuclear physicsHigh Energy Physics - Experiment (hep-ex)law0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Physics::Atomic and Molecular ClustersFermilab010306 general physicsColliderNuclear ExperimentPhysics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyD0 experimentNonlinear Sciences::Exactly Solvable and Integrable SystemsExperimental High Energy PhysicsHigh Energy Physics::ExperimentCommunication channel
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Positioning the principles of precision medicine in care pathways for allergic rhinitis and chronic rhinosinusitis – A EUFOREA-ARIA-EPOS-AIRWAYS IC…

2017

Precision medicine (PM) is increasingly recognized as the way forward for optimizing patient care. Introduced in the field of oncology, it is now considered of major interest in other medical domains like allergy and chronic airway diseases, which face an urgent need to improve the level of disease control, enhance patient satisfaction and increase effectiveness of preventive interventions. The combination of personalized care, prediction of treatment success, prevention of disease and patient participation in the elaboration of the treatment plan is expected to substantially improve the therapeutic approach for individuals suffering from chronic disabling conditions. Given the emerging dat…

allergic rhinitis; integrated care pathway; precision medicine; rhinosinusitisAllergyRhinosinusitisDiseaseAllergic rhinitis0302 clinical medicineQUALITY-OF-LIFEMedicineImmunology and Allergy030223 otorhinolaryngologySinusitisNASAL POLYPOSISRhinitisPrecision medicineintegrated care pathway3. Good healthAlgorithmREAL-LIFEIMPACT OUTCOMESARIA and EPOS working groups1107 ImmunologyDISEASESGA(2)LENDisease Progressionallergic rhinitiLife Sciences & BiomedicineENDOSCOPIC SINUS SURGERYAlgorithmsHumanIntegrated care pathwayallergic rhinitis; integrated care pathway; precision medicine; rhinosinusitis; Adult; Algorithms; Chronic Disease; Disease Progression; Humans; Precision Medicine; Rhinitis Allergic; Sinusitis; Young Adult; Immunology and Allergy; ImmunologyAdultmedicine.medical_specialtyprecision medicineImmunologyrhinosinusitiPHENOTYPESVALIDATIONYoung Adult03 medical and health sciencesTherapeutic approachAllergicPatient satisfactionQuality of life (healthcare)HumansSinusitisPatient participationIMMUNOTHERAPYIntensive care medicinerhinosinusitisAsthmaScience & Technologyallergic rhinitis; integrated care pathway; precision medicine; rhinosinusitis; Immunology and Allergy; Immunologyallergic rhinitisbusiness.industrymedicine.diseasePrecision medicineSinusitiRhinitis AllergicSEVERITY030228 respiratory system3121 General medicine internal medicine and other clinical medicineChronic DiseasePhysical therapyASTHMAbusiness
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Search for scalar leptoquarks in the acoplanar jet topology in pp¯ collisions at s=1.96 TeV

2006

A search for leptoquarks has been performed in 310 pb{sup -1} of data from p{bar p} collisions at a center-of-mass energy of 1.96 TeV, collected by the D0 detector at the Fermilab Tevatron Collider. The topology analyzed consists of acoplanar jets with missing transverse energy. The data show good agreement with standard model expectations, and a lower mass limit of 136 GeV has been set at the 95% C.L. for a scalar leptoquark decaying exclusively into a quark and a neutrino.

QuarkPhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTevatronTopology01 natural sciencesStandard Modellaw.inventionNuclear physicslaw0103 physical sciencesHigh Energy Physics::ExperimentLeptoquarkFermilabNeutrino010306 general physicsColliderLeptonPhysics Letters B
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Feasibility and physics potential of detecting $^8$B solar neutrinos at JUNO

2021

The Jiangmen Underground Neutrino Observatory (JUNO) features a 20 kt multi-purpose underground liquid scintillator sphere as its main detector. Some of JUNO's features make it an excellent location for 8B solar neutrino measurements, such as its low-energy threshold, high energy resolution compared with water Cherenkov detectors, and much larger target mass compared with previous liquid scintillator detectors. In this paper, we present a comprehensive assessment of JUNO's potential for detecting 8B solar neutrinos via the neutrino-electron elastic scattering process. A reduced 2 MeV threshold for the recoil electron energy is found to be achievable, assuming that the intrinsic radioactive …

Physics - Instrumentation and Detectorsneutrino: solarPhysics::Instrumentation and DetectorsSolar neutrinoscintillation counter: liquidhigh [energy resolution]01 natural sciences7. Clean energymass [target]High Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)JUNO; Neutrino oscillation; Solar neutrinoelastic scattering [neutrino electron]KamLAND[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]flavor [transformation]neutrino oscillationInstrumentationJiangmen Underground Neutrino ObservatoryPhysicsElastic scatteringJUNOliquid [scintillation counter]neutrino oscillation solar neutrino JUNOSettore FIS/01 - Fisica Sperimentaleoscillation [neutrino]Instrumentation and Detectors (physics.ins-det)Monte Carlo [numerical calculations]neutrino electron: elastic scatteringtensionmass difference [neutrino]ddc:nuclear reactor [antineutrino]observatoryHigh Energy Physics - PhenomenologyPhysics::Space Physicsneutrino: flavorsolar [neutrino]target: massNeutrinonumerical calculations: Monte CarloNuclear and High Energy PhysicsParticle physicsNeutrino oscillationmatter: solarCherenkov counter: waterneutrino: mass differenceFOS: Physical sciencesSolar neutrinoNOtransformation: flavoruraniumPE2_20103 physical scienceselectron: recoil: energyantineutrino: nuclear reactorsolar [matter]ddc:530ddc:610Sensitivity (control systems)[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNeutrino oscillationbackground: radioactivityCherenkov radiationAstrophysiquesolar neutrino010308 nuclear & particles physicswater [Cherenkov counter]radioactivity [background]flavor [neutrino]Astronomy and Astrophysicssensitivityneutrino: mixing anglerecoil: energy [electron]energy spectrum [electron]electron: energy spectrumHigh Energy Physics::Experimentsphereneutrino: oscillationenergy resolution: highEnergy (signal processing)mixing angle [neutrino]
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Optimization of the JUNO liquid scintillator composition using a Daya Bay antineutrino detector

2021

To maximize the light yield of the liquid scintillator (LS) for the Jiangmen Underground Neutrino Observatory (JUNO), a 20 t LS sample was produced in a pilot plant at Daya Bay. The optical properties of the new LS in various compositions were studied by replacing the gadolinium-loaded LS in one antineutrino detector. The concentrations of the fluor, PPO, and the wavelength shifter, bis-MSB, were increased in 12 steps from 0.5 g/L and <0.01 mg/L to 4 g/L and 13 mg/L, respectively. The numbers of total detected photoelectrons suggest that, with the optically purified solvent, the bis-MSB concentration does not need to be more than 4 mg/L. To bridge the one order of magnitude in the detect…

organic compounds: admixtureNuclear and High Energy PhysicsPhysics - Instrumentation and DetectorsLiquid scintillatorscintillation counter: liquidAnalytical chemistryFOS: Physical sciencesmodel: opticalScintillatorWavelength shifterantineutrino: detector01 natural sciencesNOHigh Energy Physics - Experimentwavelength shifterHigh Energy Physics - Experiment (hep-ex)PE2_2Daya BayNeutrino0103 physical sciencesfluorine: admixture[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ddc:530neutrino oscillation[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsInstrumentationJiangmen Underground Neutrino ObservatoryPhysicsJUNO010308 nuclear & particles physicsSettore FIS/01 - Fisica SperimentaleDetectorLight yield; Liquid scintillator; NeutrinoInstrumentation and Detectors (physics.ins-det)Yield (chemistry)Scintillation counterComposition (visual arts)photon: yieldNeutrinoLight yieldNuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run

2018

Made available in DSpace on 2018-11-26T17:45:14Z (GMT). No. of bitstreams: 0 Previous issue date: 2018-03-22 Australian Research Council Council of Scientific and Industrial Research of India Department of Science and Technology, India Science AMP; Engineering Research Board (SERB), India Ministry of Human Resource Development, India Spanish Agencia Estatal de Investigacion Vicepresidencia i Conselleria d'Innovacio, Recerca i Turisme Conselleria d'Educacio i Universitat del Govern de les Illes Balears Conselleria d'Educacio, Investigacio, Cultura i Esport de la Generalitat Valenciana National Science Centre of Poland Swiss National Science Foundation (SNSF) Russian Foundation for Basic Rese…

Physics and Astronomy (miscellaneous)Astrophysics::High Energy Astrophysical PhenomenaAstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsLIGO-VirgoMagnetar01 natural sciencesGeneral Relativity and Quantum CosmologyGravitational waves long transients LIGOGravitational wavesGeneral Relativity and Quantum CosmologyUPPER LIMITSSearch algorithmSIGNALS0103 physical sciencesWaveformlong transientsHigh Energy PhysicsLIGO010306 general physicsgravitational wave010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSQCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsLIGO-Virgo; gravitational waves; long duration transient[PHYS]Physics [physics]Gravitational wavelong duration transientLIGOgravitational waves; LIGO-Virgo; long duration transient; Physics and Astronomy (miscellaneous)Black holeMODELNeutron starAmplitudegravitational wavesBLACK-HOLEComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRADIATIONNEUTRINOAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Search for Stopped Gluinos frompp¯Collisions ats=1.96  TeV

2007

Long-lived, heavy particles are predicted in a number of models beyond the standard model of particle physics. We present the first direct search for such particles' decays, occurring up to 100 h after their production and not synchronized with an accelerator bunch crossing. We apply the analysis to the gluino (g), predicted in split supersymmetry, which after hadronization can become charged and lose enough momentum through ionization to come to rest in dense particle detectors. Approximately 410 pb(-1) of p (p) over bar collisions at root s = 1.96 TeV collected with the D0 detector during Run II of the Fermilab Tevatron collider are analyzed in search of such "stopped gluinos" decaying in…

PhysicsParticle physicsGluinoSplit supersymmetry010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTevatronGeneral Physics and Astronomy01 natural sciences7. Clean energyHadronizationlaw.inventionGluonNuclear physicsParticle decaylaw0103 physical sciencesNeutralinoHigh Energy Physics::Experiment010306 general physicsColliderPhysical Review Letters
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Observation and Properties of the Orbitally ExcitedBs2*Meson

2008

We report the direct observation of the excited L=1 state B_{s2}* in fully reconstructed decays to B+K-. The mass of the B_{s2}* meson is measured to be {5839.6 +- 1.1 (stat.) +- 0.7 (syst.) MeV/c^2, and its production rate relative to the B+ meson is measured to be [1.15 +- 0.23 (stat.) +- 0.13 (syst.)] %.

PhysicsMeson010308 nuclear & particles physicsDirect observationFOS: Physical sciencesGeneral Physics and Astronomy01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)Particle decayExcited state0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics::ExperimentMolecular orbitalAtomic physicsNuclear Experiment010306 general physicsProduction ratePhysical Review Letters
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Measurement of theΛbLifetime in the Exclusive DecayΛb→J/ψΛ

2007

We have measured the {lambda}{sub b} lifetime using the exclusive decay {lambda}{sub b}{yields}J/{psi}{lambda}, based on 1.2 fb{sup -1} of data collected with the D0 detector during 2002-2006. From 171 reconstructed {lambda}{sub b} decays, where the J/{psi} and {lambda} are identified via the decays J/{psi}{yields}{mu}{sup +}{mu}{sup -} and {lambda}{yields}p{pi}, we measured the {lambda}{sub b} lifetime to be {tau}({lambda}{sub b})=1.218{sub -0.115}{sup +0.130}(stat){+-}0.042(syst) ps. We also measured the B{sup 0} lifetime in the decay B{sup 0}{yields}J/{psi}({mu}{sup +}{mu}{sup -})K{sub S}{sup 0}({pi}{sup +}{pi}{sup -}) to be {tau}(B{sup 0})=1.501{sub -0.074}{sup +0.078}(stat){+-}0.050(sy…

PhysicsCrystallographyParticle decayPair production010308 nuclear & particles physicsBranching fraction0103 physical sciencesGeneral Physics and Astronomy010306 general physicsLambda01 natural sciencesPhysical Review Letters
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Tests of General Relativity with GW170817

2019

The recent discovery by Advanced LIGO and Advanced Virgo of a gravitational wave signal from a binary neutron star inspiral has enabled tests of general relativity (GR) with this new type of source. This source, for the first time, permits tests of strong-field dynamics of compact binaries in presence of matter. In this paper, we place constraints on the dipole radiation and possible deviations from GR in the post-Newtonian coefficients that govern the inspiral regime. Bounds on modified dispersion of gravitational waves are obtained; in combination with information from the observed electromagnetic counterpart we can also constrain effects due to large extra dimensions. Finally, the polari…

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftenneutron star: binaryAstronomyTestingGravitational WaveGeneral Physics and AstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmologystrong fieldddc:550general relativityLIGOQCSettore FIS/01PhysicsPhysicsGravitational effectsarticlePolarization (waves)Gravitational-wave signalsExtra dimensionsgravitational wavesPhysical SciencesExtra dimensions[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Large extra dimensiondispersionBinary neutron starsgravitational radiation: polarizationGeneral RelativityGeneral relativitygr-qcPhysics MultidisciplinaryGRAVITATIONAL-WAVE OBSERVATIONSFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)gravitational wavesblack holesGravity wavesMASSgravitational radiation: direct detectionGravitation and Astrophysicselectromagnetic field: productionRelativityGeneral Relativity and Quantum CosmologyDipole radiationsGRAVITYTests of general relativitygravitation: weak field0103 physical sciencesddc:530High Energy Physicscapture010306 general physicsGravitational Wave; General RelativitySTFCradiation: dipolepolarizationScience & TechnologyStrong fieldGravitational wavegravitational radiationRCUKbinary: compactgravitational radiation detectorLIGONeutron starVIRGODewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikNewtonianshigher-dimensional
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Erratum: “Searches for Gravitational Waves from Known Pulsars at Two Harmonics in 2015–2017 LIGO Data” (2019, ApJ, 879, 10)

2019

Two analysis errors have been identified that affect the results for a handful of the high-value pulsars given in Table 1 of Abbott et al. (2019). One affects the Bayesian analysis for the five pulsars that glitched during the analysis period, and the other affects the 5n-vector analysis for J0711-6830. Updated results after correcting the errors are shown in Table 1, which now supersedes the results given for those pulsars in Table 1 of Abbott et al. (2019). Updated versions of figures can be seen in Figures 1-4. Bayesian analysis.-For the glitching pulsars, the signal phase evolution caused by the glitch was wrongly applied twice and was therefore not consistent with our expected model of…

Known Pulsars010504 meteorology & atmospheric sciencesAstronomyAstrophysicsTable (information)Velagravitational waves; pulsars01 natural sciencesPulsar0103 physical sciencesLimit (mathematics)010303 astronomy & astrophysicsgravitational waveComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciencesPhysics[PHYS]Physics [physics]Gravitational waveTwo HarmonicsAstronomy and AstrophysicsGravitational Waves Known Pulsars Two Harmonics ErratumLIGOAmplitudegravitational wavesSpace and Planetary SciencepulsarsErratumGlitch (astronomy)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysical Journal
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Measurement of the differential cross section for the production of an isolated photon with associated jet in pp¯ collisions at s=1.96 TeV

2008

The process ppbar -> photon + jet + X is studied using 1.0 fb^-1 of data collected by the D0 detector at the Fermilab Tevatron ppbar collider at a center-of-mass energy sqrt(s)=1.96 TeV. Photons are reconstructed in the central rapidity region |y_gamma|<1.0 with transverse momenta in the range 3015 GeV. The differential cross section d^3sigma/dPt_gamma dy_gamma dy_jet is measured as a function of Pt_gamma in four regions, differing by the relative orientations of the photon and the jet in rapidity. Ratios between the differential cross sections in each region are also presented. Next-to-leading order QCD predictions using different parameterizations of parton distribution functions and theo…

PhysicsQuantum chromodynamicsNuclear and High Energy PhysicsJet (fluid)Particle physicsPhoton010308 nuclear & particles physicsTevatronParton7. Clean energy01 natural scienceslaw.inventionNuclear physicslaw0103 physical sciencesHigh Energy Physics::ExperimentRapidityFermilab010306 general physicsColliderPhysics Letters B
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Hadron energy reconstruction for the ATLAS calorimetry in the framework of the non-parametrical method

2002

This paper discusses hadron energy reconstruction for the ATLAS barrel prototype combined calorimeter (consisting of a lead-liquid argon electromagnetic part and an iron-scintillator hadronic part) in the framework of the non-parametrical method. The non-parametrical method utilizes only the known $e/h$ ratios and the electron calibration constants and does not require the determination of any parameters by a minimization technique. Thus, this technique lends itself to an easy use in a first level trigger. The reconstructed mean values of the hadron energies are within $\pm 1%$ of the true values and the fractional energy resolution is $[(58\pm3)% /\sqrt{E}+(2.5\pm0.3)%]\oplus (1.7\pm0.2)/E…

Nuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsHadronFOS: Physical scienceschemistry.chemical_elementCalorimetryElectronCalorimetry01 natural sciencesPartícules (Física nuclear)High Energy Physics - ExperimentEnergy measurementNuclear physicsHigh Energy Physics - Experiment (hep-ex)PionShower counter0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Computer data analysis[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Combined calorimeterDetectors and Experimental Techniques010306 general physicsNuclear ExperimentInstrumentationPhysicsLarge Hadron ColliderArgon010308 nuclear & particles physicsSHOWER DEVELOPMENT; RESOLUTIONSHOWER DEVELOPMENTCalorimeterRESOLUTIONchemistryScintillation counterHigh Energy Physics::ExperimentCompensation
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Search for scalar top quarks in the acoplanar charm jets and missing transverse energy final state in pp¯ collisions at s=1.96 TeV

2008

We present a search for the pair production of scalar top quarks, $\tilde{t}$, using 995 pb$^{-1}$ of data collected in $p\bar{p}$ collisions with the D0 detector at the Fermilab Tevatron Collider at $\sqrt{s} = 1.96$ TeV. Both scalar top quarks are assumed to decay into a charm quark and a neutralino ($\tilde{\chi}^{0}_{1}$), where $\tilde{\chi}^{0}_{1}$ is the lightest supersymmetric particle. This leads to a final state with two acoplanar charm jets and missing transverse energy. We find the yield of such events to be consistent with the standard model expectation, and exclude sets of $\tilde{t}$ and $\tilde{\chi}^{0}_{1} $ masses at the 95% C.L. that substantially extend the domain excl…

QuarkPhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::Phenomenology01 natural sciencesLightest Supersymmetric ParticleCharm quarkStandard ModelNuclear physicsPair production0103 physical sciencesNeutralinoHigh Energy Physics::ExperimentCharm (quantum number)010306 general physicsEnergy (signal processing)Physics Letters B
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Inhibition of Trypanosoma cruzi by plant extracts used in Chinese medicine.

2004

In this work, we assessed the effect of extracts obtained from 17 plants used in traditional Chinese medicine. These extracts were tested in vitro with the epimastigote form of Trypanosoma cruzi, clone Bra C(15) C(2), at 27 degrees C in F-29 medium at a concentration of 100 microg/ml in axenic cultures. Allopurinol was used as reference drug. Seven plant extracts showed inhibitory activities lower than 25%. Pueraria lobata, Mahonia beaei, Dictamus dasycarpus, Kochia scoparia, Sophora flavescens and Ligustrum lucidum showed effects with inhibition values between 25% and 60%, whereas Lithospermum erythrorhizon, Saussurea lappa, Melia toosendan and Cinnamomum cassia showed the greatest inhibit…

MalePuerariaTrypanosoma cruziMahoniaPharmacognosyPlant RootsInhibitory Concentration 50Parasitic Sensitivity TestsCassiaDrug DiscoveryAnimalsMedicine Chinese TraditionalRats WistarPharmacologySophora flavescensPlants MedicinalbiologyTraditional medicinePlant StemsPlant ExtractsGeneral Medicinebiology.organism_classificationLithospermum erythrorhizonTrypanocidal AgentsRatsFruitSeedsPlant BarkScopariaRhizomeCinnamomumPhytotherapyFitoterapia
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MACVIA-ARIA Sentinel NetworK for allergic rhinitis (MASK-rhinitis): the new generation guideline implementation

2015

Accepted Article

AllergyAllergyMedical InformaticSettore MED/10 - MALATTIE DELL'APPARATO RESPIRATORIOWORLD-HEALTH-ORGANIZATIONReviewComorbidityWeb BrowserHealth informatics:Medicina Clínica [Ciências Médicas]ARIA; ICT; MACVIA-LR; allergic rhinitis; asthma; clinical decision support system; conjunctivitis; visual analogue scalevisual analogue scaleQUALITY-OF-LIFEconjunctivitisMedicineImmunology and AllergyDisease management (health)ComputingMilieux_MISCELLANEOUSRhinitisClinical Trials as TopicCLIMATE-CHANGE[SDV.MHEP] Life Sciences [q-bio]/Human health and pathologyAllergenHealth PolicyDisease ManagementRANDOMIZED CONTROLLED-TRIAL3. Good healthCHRONIC RESPIRATORY-DISEASESclinical decision support systemINTEGRATED CARE PATHWAYS1107 ImmunologyVISUAL ANALOG SCALESPractice Guidelines as TopicMedical emergencyallergic rhinitiLife Sciences & BiomedicineHumanEUROPEAN INNOVATION PARTNERSHIPImmunologyClinical Decision-MakingSocio-culturaleReproducibility of Resultallergic rhinitis; ARIA; asthma; Information and communications technology; MACVIA-LR; Allergens; Biomarkers; Clinical Decision-Making; Clinical Trials as Topic; Comorbidity; Disease Management; Health Planning; Health Policy; Humans; Medical Informatics; Practice Guidelines as Topic; Reproducibility of Results; Rhinitis Allergic; Web Browser; Immunology and Allergy; ImmunologyInformation and communications technologyClinical decision support systemMACVIA-LRQuality of life (healthcare)AllergicARIA; Information and communications technology; MACVIA-LR; allergic rhinitis; asthmaJournal ArticleHumansCiências Médicas::Medicina ClínicaAsthmaScience & Technologyallergic rhinitisARIAbusiness.industrySettore MED/09 - MEDICINA INTERNAReproducibility of ResultsGuidelineBiomarkerta3121Allergensasthmamedicine.diseaseRhinitis AllergicIntegrated careHealth PlanningPOLLEN COUNTSICTallergic rhinitis; ARIA; asthma; Information and communications technology; MACVIA-LR; Allergens; Biomarkers; Clinical Decision-Making; Clinical Trials as Topic; Comorbidity; Disease Management; Health Planning; Health Policy; Humans; Medical Informatics; Practice Guidelines as Topic; Reproducibility of Results; Rhinitis Allergic; Web BrowserImmunologybusinessDECISION-SUPPORT-SYSTEMSBiomarkersMedical Informatics[SDV.MHEP]Life Sciences [q-bio]/Human health and pathology
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GW190521: A Binary Black Hole Merger with a Total Mass of 150  M⊙

2020

LIGO Scientific Collaboration and Virgo Collaboration: et al.

AstronomyGeneral Physics and Astronomydetector: networkAstrophysicsGravitational waves; Binary black holes Intermediate mass black holes01 natural sciencesGeneral Relativity and Quantum Cosmologygravitational waves; black holesGW190521 BBHIntermediate mass black holesLIGO10. No inequalityQCQBSettore FIS/01astro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsPAIR-INSTABILITYSettore FIS/05Physicsstatistical analysis: BayesianSupernovaPhysical SciencesPhysique des particules élémentaires[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaGravitational wavedata analysis methodBinary black holes Intermediate mass black holesgr-qcPhysics MultidisciplinaryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Physics and Astronomy(all)Gravitation and AstrophysicsGravitational wavespair-instabilitySettore FIS/05 - Astronomia e AstrofisicaBinary black holeBinary black holesNeutron starsgravitational wavessupernova0103 physical sciences010306 general physicsLuminosity distanceSTFCGW190521Science & Technology9. Industry and infrastructureGravitational wavegravitational radiationRCUKblack hole: massgravitational waves black holegravitational radiation detectorLIGORedshiftBlack holewave: modelVIRGOblack hole: binaryIntermediate-mass black holegravitational radiation: emissionBBH[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Performance of the upgraded PreProcessor of the ATLAS Level-1 Calorimeter Trigger

2020

The PreProcessor of the ATLAS Level-1 Calorimeter Trigger prepares the analogue trigger signals sent from the ATLAS calorimeters by digitising, synchronising, and calibrating them to reconstruct transverse energy deposits, which are then used in further processing to identify event features. During the first long shutdown of the LHC from 2013 to 2014, the central components of the PreProcessor, the Multichip Modules, were replaced by upgraded versions that feature modern ADC and FPGA technology to ensure optimal performance in the high pile-up environment of LHC Run 2. This paper describes the features of the newMultichip Modules along with the improvements to the signal processing achieved.

Physics - Instrumentation and Detectors:Kjerne- og elementærpartikkelfysikk: 431 [VDP]Computer sciencePhysics::Instrumentation and Detectors01 natural sciencesHigh Energy Physics - Experiment030218 nuclear medicine & medical imaginglaw.inventionSubatomär fysikHigh Energy Physics - Experiment (hep-ex)0302 clinical medicinelawSubatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]PreprocessorDetectors and Experimental Techniquesphysics.ins-detInstrumentationMathematical PhysicsFPGASettore FIS/01Signal processingLarge Hadron ColliderInstrumentation and Detectors (physics.ins-det)trigger [calorimeter]ATLASCalorimeters; Trigger concepts and systems (hardware and software)Calorimetermedicine.anatomical_structure:Nuclear and elementary particle physics: 431 [VDP]Trigger concepts and systems (hardware and software)design [electronics]Particle Physics - ExperimentComputer hardwareperformanceCiências Naturais::Ciências Físicas530 Physics:Ciências Físicas [Ciências Naturais]Analog-to-digital converterFOS: Physical sciences61003 medical and health sciencesCalorimetersAtlas (anatomy)0103 physical sciencesmedicineHigh Energy Physicsddc:610[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]Field-programmable gate arraysignal processingCalorimeterScience & Technologyhep-ex010308 nuclear & particles physicsbusiness.industrycalorimeter: trigger530 Physikcalibrationanalog-to-digital converterpile-upExperimental High Energy Physicselectronics: readoutbusinessreadout [electronics]Energy (signal processing)electronics: design
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Search for the Standard Model Higgs Boson in the Missing Energy and Acoplanarb-Jet Topology ats=1.96  TeV

2008

We report a search for the standard model Higgs boson in the missing energy and acoplanar b-jet topology, using an integrated luminosity of 0.93 fb(-1) recorded by the D0 detector at the Fermilab Tevatron p (p) over bar Collider. The analysis includes signal contributions from p (p) over bar -> ZH -> v (v) over barb (b) over bar, as well as from WH production in which the charged lepton from the W boson decay is undetected. Neural networks are used to separate signal from background. In the absence of a signal, we set limits on sigma(p (p) over bar -> VH) x B(H -> b (b) over bar) at the 95% C.L. of 2.6-2.3 pb, for Higgs boson masses in the range 105-135 GeV, where V W, Z. The corresponding …

PhysicsParticle physicsMissing energy010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTevatronGeneral Physics and AstronomyTopology01 natural sciencesStandard Modellaw.inventionNuclear physicsParticle decayPair productionlaw0103 physical sciencesHiggs bosonHigh Energy Physics::Experiment010306 general physicsColliderLeptonPhysical Review Letters
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Search for techniparticles in e +jets events at D0

2006

We search for the technicolor process ppbar -&gt; rho_T/omega_T -&gt;W+pi_T in events containing one electron and two jets, in data corresponding to an integrated luminosity of 390 pb-1, recorded by the D0 experiment at the Fermilab Tevatron. Technicolor predicts that technipions, pi_T, decay dominantly into b-bbar, b-cbar, or bbar-c, depending on their charge. In these events b and c quarks are identified by their secondary decay vertices within jets. Two analysis methods based on topological variables are presented. Since no excess above the standard model prediction was found, the result is presented as an exclusion in the pi_T vs. rho_T mass plane for a given set of model parameters.

PhysicsQuarkParticle physicsLuminosity (scattering theory)010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTevatronFOS: Physical sciencesGeneral Physics and AstronomyTechnicolor01 natural sciences7. Clean energyOmegaHigh Energy Physics - ExperimentStandard ModelNuclear physicsHigh Energy Physics - Experiment (hep-ex)Particle decay12.60.Nz 13.85.Rm0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics::Experiment010306 general physicsBar (unit)
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Measurement of the ratios of the Z/γ∗+⩾n jet production cross sections to the total inclusive Z/γ∗ cross section in pp¯ collisions at s=1.96 TeV

2008

We present a study of events with Z bosons and jets produced at the Fermilab Tevatron Collider in ppbar collisions at a center of mass energy of 1.96 TeV. The data sample consists of nearly 14,000 Z/G* -> e+e- candidates corresponding to the integrated luminosity of 340 pb-1 collected using the D0 detector. Ratios of the Z/G* + >= n jet cross sections to the total inclusive Z/G* cross section have been measured for n = 1 to 4 jet events. Our measurements are found to be in good agreement with a next-to-leading order QCD calculation and with a tree-level QCD prediction with parton shower simulation and hadronization.

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsLuminosity (scattering theory)010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyTevatronJet (particle physics)01 natural sciences7. Clean energyHadronizationNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentCenter of mass010306 general physicsParton showerBosonPhysics Letters B
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Measurement of the Semileptonic Branching Ratio ofBs0to an Orbitally ExcitedDs**State:Br(Bs0→Ds1−(2536)μ+νX)

2009

In a data sample of approximately 1.3 fb-1 collected with the D0 detector between 2002 and 2006, the orbitally excited charm state D_s1(2536) has been observed with a measured mass of 2535.7 +/- 0.6 (stat) +/- 0.5 (syst) MeV via the decay mode B0_s -> D_s1(2536) mu nu X. A first measurement is made of the branching ratio product Br(b(bar) -> D_s1(2536) mu nu X).Br(D_s1(2536)->D* K0_S). Assuming that D_s1(2536) production in semileptonic decay is entirely from B0_s, an extraction of the semileptonic branching ratio Br(B0_s -> D_s1(2536) mu nu X) is made.

Semileptonic decayPhysicsMeson010308 nuclear & particles physicsBranching fractionQuark modelAnalytical chemistryGeneral Physics and AstronomyState (functional analysis)01 natural sciencesNuclear physicsPair productionExcited state0103 physical sciences010306 general physicsBar (unit)Physical Review Letters
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Search for the lightest scalar top quark in events with two leptons in pp¯ collisions at s=1.96 TeV

2009

Abstract We report results of a search for the pair production of the lightest supersymmetric partner of the top quark, t ˜ 1 , using a data set corresponding to an integrated luminosity of 1 fb −1 collected by the DO detector at a p p ¯ center-of-mass energy of 1.96 TeV at the Fermilab Tevatron collider. Both scalar top quarks are assumed to decay into a b quark, a charged lepton and a scalar neutrino. The search is performed in the electron plus muon and dielectron final states. The signal topology consists of two isolated leptons, missing transverse energy, and jets. We find no evidence for this process and exclude regions of parameter space in the framework of the minimal supersymmetric…

QuarkPhysicsNuclear and High Energy PhysicsParticle physicsTop quark010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTevatronElementary particle7. Clean energy01 natural sciencesBottom quarkNuclear physicsPair production0103 physical sciencesHigh Energy Physics::ExperimentFermilabNeutrino010306 general physicsLeptonMinimal Supersymmetric Standard ModelPhysics Letters B
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The INTEGRAL view of the pulsating hard X-ray sky: from accreting and transitional millisecond pulsars to rotation-powered pulsars and magnetars

2020

arXiv:2012.01346v1

Astrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsMagnetarQuantitative Biology::OtherComputer Science::Digital Libraries01 natural sciencesNeutron starsX-rays: binariesSettore FIS/05 - Astronomia E AstrofisicaPulsarMillisecond pulsar0103 physical sciencesMagnetarsAccretion disks magnetars neutron stars pulsar X-rays:binaries X-rays:burstseducationX-rays: bursts010303 astronomy & astrophysicsPulsarsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)education.field_of_study010308 nuclear & particles physicsCrab PulsarAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsAccretion (astrophysics)Neutron starSpace and Planetary ScienceAccretion disksSpin-upAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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P-26 RATIONALE 305: Tislelizumab plus chemotherapy versus placebo plus chemotherapy as first-line therapy in patients with gastric or gastroesophagea…

2020

Chemotherapymedicine.medical_specialtybusiness.industrymedicine.medical_treatmentHematologyGastroesophageal Junction AdenocarcinomaPlaceboGastroenterologyFirst line therapyOncologyInternal medicinemedicineIn patientbusinessAnnals of Oncology
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MOESM1 of Scaling up strategies of the chronic respiratory disease programme of the European Innovation Partnership on Active and Healthy Ageing (Act…

2016

Additional file 1. IPCRG scaling up activities.

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Constraining the p -Mode– g -Mode Tidal Instability with GW170817

2019

We analyze the impact of a proposed tidal instability coupling p modes and g modes within neutron stars on GW170817. This nonresonant instability transfers energy from the orbit of the binary to internal modes of the stars, accelerating the gravitational-wave driven inspiral. We model the impact of this instability on the phasing of the gravitational wave signal using three parameters per star: An overall amplitude, a saturation frequency, and a spectral index. Incorporating these additional parameters, we compute the Bayes factor (lnB!pgpg) comparing our p-g model to a standard one. We find that the observed signal is consistent with waveform models that neglect p-g effects, with lnB!pgpg=…

Physics010308 nuclear & particles physicsGravitational waveGeneral Physics and AstronomyBreaking wave7. Clean energy01 natural sciencesInstabilityComputational physicsNeutron starStarsAmplitude13. Climate action0103 physical sciencesWaveformExtreme value theory010303 astronomy & astrophysicsPhysical Review Letters
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Search for pair production of second generation scalar leptoquarks

2008

We report on a search for the pair production of second generation scalar leptoquarks (LQ) in ppbar collisions at the center of mass energy sqrt(s)=1.96 TeV using a data set corresponding to an integrated luminosity of 1.0 fb-1 collected with the D0 experiment at the Fermilab Tevatron Collider. Topologies arising from the LQLQbar-&gt;muqnuq and LQLQbar-&gt;muqmuq decay modes are investigated. No excess of data over the standard model prediction is observed and upper limits on the leptoquark pair production cross section are derived at the 95% C.L. as a function of the leptoquark mass and the branching fraction beta for the decay LQ-&gt;muq. These are interpreted as lower limits on the lepto…

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsBranching fractionScalar (mathematics)High Energy Physics::PhenomenologyTevatronFOS: Physical sciencesD0 experiment7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsHigh Energy Physics - Experiment (hep-ex)Pair production0103 physical sciencesExperimental High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSING[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Grand Unified TheoryLeptoquarkHigh Energy Physics::ExperimentFermilab010306 general physics
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XIPE: the x-ray imaging polarimetry explorer

2016

XIPE, the X-ray Imaging Polarimetry Explorer, is a mission dedicated to X-ray Astronomy. At the time of writing XIPE is in a competitive phase A as fourth medium size mission of ESA (M4). It promises to reopen the polarimetry window in high energy Astrophysics after more than 4 decades thanks to a detector that efficiently exploits the photoelectric effect and to X-ray optics with large effective area. XIPE uniqueness is time-spectrally-spatially- resolved X-ray polarimetry as a breakthrough in high energy astrophysics and fundamental physics. Indeed the payload consists of three Gas Pixel Detectors at the focus of three X-ray optics with a total effective area larger than one XMM mirror bu…

X-ray AstronomyHigh-energy astronomyPolarimetryX-ray opticsX-ray telescopeCondensed Matter Physic01 natural sciencesObservatory0103 physical sciencesPolarimetryElectronicOptical and Magnetic MaterialsSpectral resolutionElectrical and Electronic Engineering010303 astronomy & astrophysicsGas Pixel DetectorPhysicsX-ray astronomyta115X-ray optics010308 nuclear & particles physicsElectronic Optical and Magnetic MaterialApplied MathematicsVegaAstronomyComputer Science Applications1707 Computer Vision and Pattern RecognitionGas Pixel Detector; Polarimetry; X-ray Astronomy; X-ray opticsCondensed Matter PhysicsComputer Science ApplicationsApplied MathematicGas Pixel Detector; Polarimetry; X-ray Astronomy; X-ray optics; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringGas Pixel Detector; Polarimetry; X-ray Astronomy; X-ray optics; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications; Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringComputer Vision and Pattern RecognitionX-ray optic
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Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network

2019

Gravitational wave astronomy has been firmly established with the detection of gravitational waves from the merger of ten stellar mass binary black holes and a neutron star binary. This paper reports on the all-sky search for gravitational waves from intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network. The search uses three independent algorithms: two based on matched filtering of the data with waveform templates of gravitational wave signals from compact binaries, and a third, model-independent algorithm that employs no signal model for the incoming signal. No intermediate mass black hole binary event was detected in this sear…

binary: massneutron star: binaryAstronomybinary: angular momentumAstrophysicsdetector: network01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsLIMITSclustersLIGOgravitational waveGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCQBastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01black hole: spinPhysicsintermediate mass black hole binarieNumerical relativityGeneral relativitygravitational wavesgravitational waves; intermediate mass black hole binaries; Advanced LIGO and VirgoPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenastarsGeneral relativitygr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesalternative theories of gravitySTARS; CLUSTERS; LIMITSAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & Astrophysicsgravitational radiation: direct detectionGeneral Relativity and Quantum CosmologySettore FIS/05 - Astronomia e AstrofisicaBinary black hole0103 physical sciencesddc:530010306 general physicsAstrophysics::Galaxy AstrophysicsSTFCScience & Technology010308 nuclear & particles physicsGravitational waveAdvanced LIGO and Virgointermediate mass black hole binariesRCUKGravitational Wave Physicsblack hole: massMass ratiobinary: compact04.80.NnLIGOgravitational radiation detectorNeutron starVIRGOblack hole: binaryIntermediate-mass black holerelativity theorygravitational radiation: emission95.55.Ymmass ratioDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik07.05.Kflimits[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]CLUSTERSSTARSGravitational waves Black holes (astronomy) Gravitational self force
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Erratum to: “Search for particles decaying into a Z boson and a photon in pp¯ collisions at s=1.96 TeV” [Phys. Lett. B 641 (2006) 415]

2009

Search for particles decaying into a Z boson and a photon in collisions p (p)over-bar at root s = 1.96 TeV (vol 641, pg 415, 2006)

PhysicsNuclear and High Energy PhysicsParticle physicsPhoton010308 nuclear & particles physicsHigh Energy Physics::Phenomenology0103 physical sciencesHigh Energy Physics::Experiment010303 astronomy & astrophysics01 natural sciencesPhysics Letters B
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Surgeons' fear of getting infected by COVID19: A global survey

2020

During the last three months, COVID- 19 pandemic had led to a serious backlog of operations globally, and plans for restarting operation are imperative. Recommendations for surgical activities were studied, aiming to protect the surgical staff from being infected. In the meantime, it is also important to give attention to the surgeon’s personal feeling during work. We conducted a survey to investigate global surgi- cal practices during the COVID-19 pandemic, and the surgeon’s personal feeling was also investigated in the sur- vey. In this special letter, we performed multivariate analysis to explore factors that associated with surgeon’s fear of getting infected by COVID-19.

Surgery COVID-19medicine.medical_specialty2019-20 coronavirus outbreakInfectious Disease Transmission Patient-to-Professionalsurvey covid19Coronavirus disease 2019 (COVID-19)Attitude of Health PersonnelSettore MED/18 - CHIRURGIA GENERALESevere acute respiratory syndrome coronavirus 2 (SARS-CoV-2)Infectious Disease TransmissionCOVID-19. Global surgery.MEDLINEGlobal HealthNOPatient-to-ProfessionalTumours of the digestive tract Radboud Institute for Health Sciences [Radboudumc 14]Surveys and QuestionnairesCorrespondencemedicineGlobal healthInfection controlHumansGeneralPersonal protective equipmentPersonal Protective EquipmentLS7_4SurgeonsInfection Controlcovid-19; pandemic; surgerySARS-CoV-2business.industrypandemicVaccinationCOVID-19covidFearSettore MED/18Occupational DiseasesCOVID-19; Global Health; Humans; Infection Control; Occupational Diseases; Personal Protective Equipment; Surgeons; Surveys and Questionnaires; Attitude of Health Personnel; Fear; Infectious Disease Transmission Patient-to-ProfessionalSurgeon - infection - COVID19 - surveyFamily medicineSurgerybusiness
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Measurement of the isolated photon cross section in pp¯ collisions at s=1.96 TeV

2006

The cross section for the inclusive production of isolated photons has been measured in p anti-p collisions at sqrt{s}=1.96 TeV with the D0 detector at the Fermilab Tevatron Collider. The photons span transverse momenta 23 to 300 GeV and have pseudorapidity |eta|<0.9. The cross section is compared with the results from two next-to-leading order perturbative QCD calculations. The theoretical predictions agree with the measurement within uncertainties.

PhysicsNuclear and High Energy PhysicsParticle physicsPhoton010308 nuclear & particles physicsTevatronPerturbative QCD7. Clean energy01 natural sciencesNuclear physicsTransverse planePseudorapidity0103 physical sciencesHigh Energy Physics::ExperimentFermilabNuclear Experiment010306 general physicsPhysics Letters B
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Erratum to: “Measurement of the isolated photon cross section in pp¯ collisions at s=1.96 TeV” [Phys. Lett. B 639 (2006) 151]

2008

Measurement of the isolated photon cross section in p(p)over-bar collisions at root s = 1.96 TeV (vol 639, pg 151, 2006)

Nuclear physicsPhysicsNuclear and High Energy PhysicsCross section (physics)Photon010308 nuclear & particles physics0103 physical sciences010306 general physics01 natural sciencesPhysics Letters B
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Observation of the doubly radiative decay η′→γγπ0

2017

Based on a sample of 1.31 billion J/psi events collected with the BESIII detector, we report the study of the doubly radiative decay eta' -> gamma gamma pi(0) for the first time, where the eta' meson is produced via the J/psi -> gamma eta' decay. The branching fraction of eta' -> gamma gamma pi(0) inclusive decay is measured to be B(eta' -> gamma gamma pi(0))(Incl) = (3.20 +/- 0.07(stat) +/- 0.23(sys)) x 10(-3), while the branching fractions of the dominant process eta' -> gamma omega and the non-resonant component are determined to be B(eta' -> gamma omega) x B(omega -> gamma pi(0)) = (23.7 +/- 1.4(stat) +/- 1.8(sys)) x 10(-4) and B(eta' -> gamma gamma pi(0))(NR) = (6.16 +/- 0.64(stat) +/-…

PhysicsMeson010308 nuclear & particles physicsBranching fractionAstrophysics::High Energy Astrophysical PhenomenaElectron–positron annihilationRadiative decay01 natural sciencesOmegaGamma gammaNuclear physics0103 physical sciencesPiHigh Energy Physics::ExperimentNuclear Experiment010306 general physicsPhysical Review D
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Search for a Higgs boson produced in association with a Z boson

2007

We describe a search for the Standard Model Higgs boson with a mass of 105 GeV/c(2) to 145 GeV/c(2) in data corresponding to an integrated luminosity of approximately 450 pb(-1) collected with the D phi detector at the Fermilab Tevatron p (p) over bar collider at a center-of-mass energy of 1.96 TeV. The Higgs boson is required to be produced in association with a Z boson, and the Z boson is required to decay to either electrons or muons with the Higgs boson decaying to a b (b) over bar pair. The data are well described by the expected background, leading to 95% confidence level cross section upper limits sigma (p (p) over bar -> ZH) x B(H -> b (b) over bar) in the range of 3.1 pb to 4.4 pb.

PhysicsNuclear and High Energy PhysicsParticle physicsMuonLuminosity (scattering theory)010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTevatron7. Clean energy01 natural scienceslaw.inventionStandard ModellawExperimental High Energy Physics0103 physical sciencesHiggs bosonHigh Energy Physics::ExperimentFermilab010306 general physicsColliderBosonPhysics Letters B
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Scaling up strategies of the chronic respiratory disease programme of the European Innovation Partnership on Active and Healthy Ageing (Action Plan B…

2016

Action Plan B3 of the European Innovation Partnership on Active and Healthy Ageing (EIP on AHA) focuses on the integrated care of chronic diseases. Area 5 (Care Pathways) was initiated using chronic respiratory diseases as a model. The chronic respiratory disease action plan includes (1) AIRWAYS integrated care pathways (ICPs), (2) the joint initiative between the Reference site MACVIA-LR (Contre les MAladies Chroniques pour un VIeillissement Actif) and ARIA (Allergic Rhinitis and its Impact on Asthma), (3) Commitments for Action to the European Innovation Partnership on Active and Healthy Ageing and the AIRWAYS ICPs network. It is deployed in collaboration with the World Health Organizatio…

Pulmons -- Malalties obstructivesVeterinary medicineAllergyPublished ErratumLANGUEDOC-ROUSSILLONAllergyRespiratory Medicine and Allergy[SDV]Life Sciences [q-bio]Aparell respiratori -- MalaltiesOPERATIONAL DEFINITIONAlternative medicineReviewChronic respiratory diseasesGLOBAL ALLIANCESYSTEMS MEDICINE0302 clinical medicineMedicine and Health SciencesImmunology and AllergyMACVIA030212 general & internal medicineAIRWAYS ICPLungmedicin och allergiEIP on AHA; European Innovation Partnership on Active and Healthy Ageing; Chronic respiratory diseases; AIRWAYS ICPs; MACVIA; ARIA; Scaling upGINA STRATEGYAIRWAYSUPDATE ARIA 2008Scaling upRespiratory disease:Outras Ciências Agrárias [Ciências Agrárias]3. Good healthChronic respiratory diseaseALLERGIC RHINITISICPsAIRWAYS ICPsGeneral partnershipAction planErratumLife Sciences & BiomedicineAIRWAYS ICPs; ARIA; Chronic respiratory diseases; EIP on AHA; European Innovation Partnership on Active and Healthy Ageing; MACVIA; Scaling upPulmonary and Respiratory Medicinemedicine.medical_specialtyEIP on AHAAIRWAYS ICPs; ARIA; Chronic respiratory diseases; EIP on AHA; European Innovation Partnership on Active and Healthy Ageing; MACVIA; Scaling up; Immunology and AllergyEmerging technologiesImmunologyREFERENCE SITESocio-culturalePredictive medicine03 medical and health sciencesEuropean Innovation Partnership on Active and Healthy AgeingNursingCritical success factorJournal Articlemedicineddc:610Science & TechnologyARIAbusiness.industrySettore MED/09 - MEDICINA INTERNAAIRWAYS-ICPSmedicine.diseaseIntegrated careAlliance030228 respiratory systemCiências Agrárias::Outras Ciências Agrárias3121 General medicine internal medicine and other clinical medicineFamily medicineImmunologyHealthy ageingbusinessSEVERE ASTHMA
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A first search for coincident gravitational waves and high energy neutrinos using LIGO, Virgo and ANTARES data from 2007

2013

A search for high-energy neutrinos coming from the direction of the Sun has been performed using the data recorded by the ANTARES neutrino telescope during 2007 and 2008. The neutrino selection criteria have been chosen to maximize the selection of possible signals produced by the self-annihilation of weakly interacting massive particles accumulated in the centre of the Sun with respect to the atmospheric background. After data unblinding, the number of neutrinos observed towards the Sun was found to be compatible with background expectations. The 90% CL upper limits in terms of spin-dependent and spin-independent WIMP-proton cross-sections are derived and compared to predictions of two sup…

AstrofísicaEXPLOSIONSHigh energyPhotonPOINT SOURCESSUPERCONDUCTING COSMIC STRINGSGravitational waves / experimentsGravitational waves/experimentsAstrophysics01 natural scienceshigh energy neutrinosgravitational wavesgravitational waves / experiment010303 astronomy & astrophysicsQCmedia_commonLine (formation)QBPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)GAMMA-RAY BURSTSdark matter detectorsGravitational waves / experiments; Neutrino astronomy; Astronomy and Astrophysicshigh energy neutrinos[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Settore FIS/01 - Fisica SperimentaleAstrophysics::Instrumentation and Methods for Astrophysicsgravitational waves; gravitational waves / experiments; neutrino astronomy; high energy neutrinos; high energy neutrinosgravitational wavesgravitational wavesparticle physics - cosmology connectionNeutrino astronomyCOSMIC STRINGSRELATIVISTIC JETSNeutrinoAstrophysics - High Energy Astrophysical Phenomenasupersymmetry and cosmology[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]gravitational waves / experiments; neutrino astronomyTELESCOPEmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaSCIENCE RUNFOS: Physical sciencesddc:500.2GAMMA-RAY BURSTS; CORE-COLLAPSE SUPERNOVAE; SUPERCONDUCTING COSMIC STRINGS; MAGNETAR GIANT FLARES; SCIENCE RUN; RELATIVISTIC JETS; POINT SOURCES; BLACK-HOLES; LOCAL-RATE; TELESCOPEGravitational wavesGeneral Relativity and Quantum CosmologyCORE-COLLAPSE SUPERNOVAESettore FIS/05 - Astronomia e AstrofisicaCoincidentneutrino experiments0103 physical sciences010306 general physicsMAGNETAR GIANT FLARESBLACK-HOLESHigh Energy Astrophysical PhenomenaGravitational waveAstronomy[ PHYS.ASTR.HE ] Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Astronomy and AstrophysicsDRIVENUniverseLIGOGIANT FLARESLOCAL-RATEFISICA APLICADALUMINOSITYRADIATIONHigh Energy Physics::Experiment[ SDU.ASTR.HE ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]Experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Observation and Measurement of Forward Proton Scattering in Association with Lepton Pairs Produced via the Photon Fusion Mechanism at ATLAS

2020

The observation of forward proton scattering in association with lepton pairs (eþe− þ p or μþμ− þ p) produced via photon fusion is presented. The scattered proton is detected by the ATLAS Forward Proton spectrometer, while the leptons are reconstructed by the central ATLAS detector. Proton-proton collision data recorded in 2017 at a center-of-mass energy of ffiffiffi s p ¼ 13 TeV are analyzed, corresponding to an integrated luminosity of 14.6 fb−1. A total of 57 (123) candidates in the ee þ p (μμ þ p) final state are selected, allowing the background-only hypothesis to be rejected with a significance exceeding 5 standard deviations in each channel. Proton-tagging techniques are introduced f…

:Kjerne- og elementærpartikkelfysikk: 431 [VDP]Photon13000 GeV-cmsLHC ATLASmeasured [channel cross section]General Physics and Astronomy01 natural sciences7. Clean energyHigh Energy Physics - Experimentelectron: pair productionSubatomär fysikHigh Energy Physics - Experiment (hep-ex)Integrated LuminosityFusion Mechanismphoton photon: fusionspectrometer [p]Subatomic Physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]scattering [p p]pair production [lepton]Electroweak interactionQuantum ChromodynamicsParticle productionNuclear ExperimentSettore FIS/01PhysicsQuantum chromodynamicsObservation and MeasurementQuantum electrodynamicsLarge Hadron Colliderp: spectrometerdimuonAtlas (topology)COLLISIONS; PHYSICS; GAMMA; LIGHT; LHCElectroweak interactionDetectorphotonATLASfusion [photon photon]muon: pair production:Nuclear and elementary particle physics: 431 [VDP]PhotoproductionLIGHTCERN LHC CollATLAS DetectorsLHCcolliding beams [p p]channel cross section: measuredParticle Physics - Experimentsmall-angleParticle physicsp p: scatteringCOLLISIONSp: particle identificationCiências Naturais::Ciências Físicas530 Physicslepton: pair production:Ciências Físicas [Ciências Naturais]Particles & FieldsFOS: Physical sciencesparticle identification [p]LHC ATLAS High Energy PhysicsPHYSICS0103 physical sciencesddc:530Cross-Section Measurementpair production [electron]pair production [muon]High Energy Physics010306 general physicsCiencias ExactasATLAS CollaborationScience & TechnologySpectrometerhep-exPomeronsFísicaGAMMALeptonsProton Scatteringexclusive productionPrecision measurementsProton Proton CollisionsStandard DeviationExperimental High Energy PhysicsElementary Particles and FieldsHigh Energy Physics::ExperimentHadron-hadron collisionsp p: colliding beamsLeptonacceptanceexperimental results
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Zγ production and limits on anomalous ZZγ and Zγγ couplings in pp¯ collisions at s=1.96 TeV

2007

We present a study of eey and mu mu gamma events using 1109 (1009) pb-(1) of data in the electron (muon) channel, respectively. These data were collected with the DO detector at the Fermilab Tevatron pp collider at Is = 1.96 TeV. Having observed 453 (515) candidates in the eey (jtAy) final state, we measure the Z gamma production cross section for a photon with transverse energy ET > 7 GeV, separation between the photon and leptons Delta Rey > 0.7, and invariant mass of the di-lepton pair Mee > 30 GeV/(2)(c), to be 4.96 0.30(stat. + syst.) zE 0.30(lumi.) pb, in agreement with the Standard Model prediction of 4.74 0.22 pb. This is the most precise Zy cross section measurement at a hadron col…

PhysicsNuclear and High Energy PhysicsGauge bosonParticle physicsMuonLarge Hadron Collider010308 nuclear & particles physicsTevatron01 natural sciences7. Clean energylaw.inventionStandard ModelNuclear physicslaw0103 physical sciencesHigh Energy Physics::ExperimentFermilab010306 general physicsColliderLeptonPhysics Letters B
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SAX J1808.4-3658, an accreting millisecond pulsar shining in gamma rays?

2016

We report the detection of a possible gamma-ray counterpart of the accreting millisecond pulsar SAX J1808.4-3658. The analysis of ~6 years of data from the Large Area Telescope on board the Fermi Gamma-ray Space Telescope (Fermi-LAT) within a region of 15deg radius around the position of the pulsar reveals a point gamma-ray source detected at a significance of ~6 sigma (Test Statistic TS = 32), with position compatible with that of SAX J1808.4-3658 within 95% Confidence Level. The energy flux in the energy range between 0.6 GeV and 10 GeV amounts to (2.1 +- 0.5) x 10-12 erg cm-2 s-1 and the spectrum is well-represented by a power-law function with photon index 2.1 +- 0.1. We searched for si…

Astrophysics::High Energy Astrophysical PhenomenaPulsar planetEnergy fluxFOS: Physical sciencesGamma-rays: starAstrophysics01 natural sciencesBinary pulsarSettore FIS/05 - Astronomia E AstrofisicaSpitzer Space TelescopePulsarMillisecond pulsar0103 physical sciences010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomyAstronomy and AstrophysicsStars: neutronStars: individual: SAX J1808.4-3658Space and Planetary ScienceOrbital motionstars; Stars: individual: SAX J1808.4-3658; Stars: neutron; Space and Planetary Science; Astronomy and Astrophysics [Gamma-rays]Astrophysics - High Energy Astrophysical PhenomenaFermi Gamma-ray Space Telescope
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Search for flavor-changing-neutral-current D meson decays

2008

We study the flavor-changing-neutral-current process c to u mu+ mu- using 1.3 fb^-1 of p p bar collisions at sqrt(s) = 1.96 TeV recorded by the D0 detector operating at the Fermilab Tevatron Collider. We see clear indications of the Ds+ and D+ to phi pi+ to mu+ mu- pi+ final states with significance greater than four standard deviations above background for the D+ state. We search for the continuum decay of D+ to pi+mu+mu- in the dimuon invariant mass spectrum away from the phi resonance. We see no evidence of signal above background and set a limit of B(D+ to pi+mu+mu-) &lt; 3.9 x 10^-6 at the 90% C.L. This limit places the most stringent constraint on new phenomena in the c to u mu+ mu- t…

PhysicsParticle physicsMeson010308 nuclear & particles physicsFlavor-changing neutral currentHadronTevatronGeneral Physics and AstronomyFOS: Physical sciencesElementary particle01 natural sciences7. Clean energyHigh Energy Physics - ExperimentNuclear physicsParticle decayHigh Energy Physics - Experiment (hep-ex)Pair production0103 physical sciencesD meson[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]High Energy Physics::Experiment010306 general physicsPhysical Review Letters
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HIGH GRADE GLIOMAS AND DIPG

2014

OncologyCancer Researchmedicine.medical_specialtybusiness.industry03 medical and health sciencesAbstracts0302 clinical medicineText miningOncology030220 oncology & carcinogenesisInternal medicinemedicineNeurology (clinical)business030217 neurology & neurosurgery
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Search for R-parity violating supersymmetry via the LLE¯ couplings λ121, λ122 or λ133 in pp¯ collisions at s=1.96 TeV

2006

A search for gaugino pair production with a trilepton signature in the framework of R-parity violating supersymmetry via the couplings lambda_121, lambda_122, or lambda_133 is presented. The data, corresponding to an integrated luminosity of L~360/pb, were collected from April 2002 to August 2004 with the D0 detector at the Fermilab Tevatron Collider, at a center-of-mass energy of sqrt(s)=1.96 TeV. This analysis considers final states with three charged leptons with the flavor combinations eel, mumul, and eetau (l=e or mu). No evidence for supersymmetry is found and limits at the 95% confidence level are set on the gaugino pair production cross section and lower bounds on the masses of the …

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyGauginoTevatronSupersymmetryLambda7. Clean energy01 natural sciencesNuclear physicsCharginoPair productionR-parity0103 physical sciencesNeutralinoHigh Energy Physics::Experiment010306 general physicsPhysics Letters B
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All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data

2019

We present results of an all-sky search for continuous gravitational waves (CWs), which can be produced by fast-spinning neutron stars with an asymmetry around their rotation axis, using data from the second observing run of the Advanced LIGO detectors. We employ three different semi-coherent methods ($\textit{FrequencyHough}$, $\textit{SkyHough}$, and $\textit{Time-Domain $\mathcal{F}$-statistic}$) to search in a gravitational-wave frequency band from 20 to 1922 Hz and a first frequency derivative from $-1\times10^{-8}$ to $2\times10^{-9}$ Hz/s. None of these searches has found clear evidence for a CW signal, so we present upper limits on the gravitational-wave strain amplitude $h_0$ (the …

AstronomyAstrophysicsRotation01 natural sciencesrotationGravitation Cosmology & AstrophysicsGeneral Relativity and Quantum CosmologyPhysics Particles & Fieldscontinuous gravitational waveLIGOneutron starGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)media_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01Physicsastro-ph.HEPhysicsPhysical SystemsAmplitudeGeneral relativitygravitational wavesPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave detectionAstrophysics - High Energy Astrophysical Phenomenacontinuous gravitational waves; Advanced LIGOcontinuous gravitational wavesasymmetryGravitationNeutron stars & pulsarsGeneral relativityFrequency bandmedia_common.quotation_subjectgr-qcFOS: Physical sciencesalternative theories of gravityGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsGravitational waves0103 physical sciencesAdvanced LIGOddc:530Gravitation Cosmology &amp; Astrophysics010306 general physicsgravitational radiation: frequencySTFCgravitational wavesneutron starsGravitational wave sourcesScience & TechnologyGravitational wave sources Gravitational waves Physical Systems Neutron stars and pulsars Gravitational wave detection010308 nuclear & particles physicsGravitational waveRCUKGravitational Wave PhysicsLIGONeutron stars &amp; pulsarsNeutron starSkyNeutron stars and pulsarsDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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GW190412: Observation of a binary-black-hole coalescence with asymmetric masses

2020

LIGO Scientific Collaboration and Virgo Collaboration: et al.

Physics and Astronomy (miscellaneous)AstronomyGravitational wave detection Gravitational wave sources Gravitational waves Astronomical black holesagn discsAstrophysicsdetector: network01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & Fieldsstar-clustersgravitational waves black holesgravitational waves; black holesAGN DISCSgravitational waves; black holes; LIGO; Virgoblack holegeneral relativityLIGOgravitational waveQCQBPhysicsSettore FIS/01astro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)GRAVITATIONAL WAVE-FORMSPROGENITORSCOMPACT BINARIESblack hole: spinPhysicsPERTURBATIONSgravitational wavesPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave detectionAstrophysics - High Energy Astrophysical PhenomenaMETALLICITYmass: asymmetrymetallicitydata analysis methodGeneral relativityMERGERSgr-qcAstrophysics::High Energy Astrophysical PhenomenamultipolePREDICTIONSFOS: Physical sciencesgravitational wavesblack holesGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & Astrophysicsgravitational radiation: direct detectionGravitational wavesGeneral Relativity and Quantum CosmologyTheory of relativityBinary black holeSettore FIS/05 - Astronomia e AstrofisicaAstronomical black holesbinary: coalescence0103 physical sciencesnumerical methodsddc:530STAR-CLUSTERS010306 general physicsnumerical calculationsSTFCAstrophysiqueGravitational wave sourcesScience & Technologymass: solar010308 nuclear & particles physicsGravitational waveVirgogravitational radiationRCUKblack hole: massMass ratioblack holesLIGOEVOLUTIONgravitational radiation detectorBlack holedetector: sensitivityPhysics and Astronomyblack hole: binaryrelativity theorygravitational radiation: emissionmass ratioMultipole expansion[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics and astroparticle physics
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ARIA 2016: Care pathways implementing emerging technologies for predictive medicine in rhinitis and asthma across the life cycle

2016

The Allergic Rhinitis and its Impact on Asthma (ARIA) initiative commenced during a World Health Organization workshop in 1999. The initial goals were (1) to propose a new allergic rhinitis classification, (2) to promote the concept of multi-morbidity in asthma and rhinitis and (3) to develop guidelines with all stakeholders that could be used globally for all countries and populations. ARIA-disseminated and implemented in over 70 countries globally-is now focusing on the implementation of emerging technologies for individualized and predictive medicine. MASK [MACVIA (Contre les Maladies Chroniques pour un Vieillissement Actif)-ARIA Sentinel NetworK] uses mobile technology to develop care p…

PediatricsAIRWAYS ICPs; ARIA; EIP on AHA; ICT; Mobile technology; Rhinitis; Immunology and AllergyIMPACTHay feverRespiratory Medicine and AllergyDiseaseReview[SDV.MHEP.PSR]Life Sciences [q-bio]/Human health and pathology/Pulmonology and respiratory tract0302 clinical medicineQUALITY-OF-LIFEHDE ALERHealth careMedicine and Health SciencesPERSISTENT ALLERGIC RHINITISMedicineImmunology and Allergy030212 general & internal medicine[SDV.IMM.ALL]Life Sciences [q-bio]/Immunology/AllergologyAIRWAYS ICPComputingMilieux_MISCELLANEOUSRhinitiAIRWAYS ICPs; ARIA; EIP on AHA; ICT; Mobile technology; RhinitisLungmedicin och allergiRhinitisPublic Health Global Health Social Medicine and Epidemiology3. Good healthREAL-LIFEAIRWAYS ICPsARIA; Rhinitis; ICT; EIP on AHA; Mobile technology; AIRWAYS ICPsHay feverCLINICAL-PRACTICE GUIDELINESHEALTHPulmonary and Respiratory Medicinemedicine.medical_specialtyEIP on AHAEUROPEAN INNOVATION PARTNERSHIPImmunologySocio-culturaleClinical decision support systemICT; EIP on AHAPredictive medicine03 medical and health sciencesQuality of life (healthcare)Mobile technologyJournal ArticleMobile technologyAsmaAsthmaScience & TechnologyARIAbusiness.industryAIRWAYS ICPs; ARIA; EIP on AHA; ICT; Mobile technology; Rhinitis;Settore MED/09 - MEDICINA INTERNAAIRWAYS-ICPSCorrectionmedicine.disease2008 UPDATEFebre del fencAsthmaFolkhälsovetenskap global hälsa socialmedicin och epidemiologi030228 respiratory systemFamily medicineICTVISUAL ANALOG SCALEbusiness
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Measurement of the ratio of the pp¯→W+c-jet cross section to the inclusive pp¯→W+jets cross section

2008

We present a measurement of the fraction of inclusive W +jets events produced with net charm quantum number 11, denoted W + c-jet, in p collisions at root s = 1.96 TeV using approximately 1 fb(-1) of data collected by the DO detector at the Fermilab Tevatron Collider. We identify the W +jets events via the leptonic W boson decays. Candidate W + c-jet events are selected by requiring a jet containing a muon in association with a reconstructed W boson and exploiting the charge correlation between this muon and W boson decay lepton to perform a nearly model-independent background subtraction. We measure the fraction of W + c-jet events in the inclusive W +jets sample for jet PT > 20 GeV and ps…

PhysicsNuclear and High Energy PhysicsJet (fluid)Particle physicsMuon010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical PhenomenaTevatronCharge (physics)01 natural sciences7. Clean energylaw.inventionNuclear physicslawPseudorapidity0103 physical sciencesHigh Energy Physics::ExperimentFermilabNuclear Experiment010306 general physicsColliderLeptonPhysics Letters B
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Search for supersymmetry in di-photon final states at s=1.96 TeV

2008

We report results of a search for supersymmetry (SUSY) with gauge-mediated symmetry breaking in di-photon events collected by the DO experiment at the Fermilab Tevatron Collider in 2002-2006. In 1.1 fb(-1) of data, we find no significant excess beyond the background expected from the standard model and set the most stringent lower limits to date for a standard benchmark model on the lightest neutralino and chargino masses of 125 GeV and 229 GeV, respectively, at 95% confidence.

PhysicsNuclear and High Energy PhysicsParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTevatronSupersymmetry01 natural sciencesStandard ModelNuclear physicsChargino0103 physical sciencesNeutralinoHigh Energy Physics::ExperimentGravitinoFermilabSymmetry breaking010306 general physicsPhysics Letters B
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Gravitational-wave Constraints on the Equatorial Ellipticity of Millisecond Pulsars

2020

We present a search for continuous gravitational waves from five radio pulsars, comprising three recycled pulsars (PSR J0437-4715, PSR J0711-6830, and PSR J0737-3039A) and two young pulsars: the Crab pulsar (J0534+2200) and the Vela pulsar (J0835-4510). We use data from the third observing run of Advanced LIGO and Virgo combined with data from their first and second observing runs. For the first time, we are able to match (for PSR J0437-4715) or surpass (for PSR J0711-6830) the indirect limits on gravitational-wave emission from recycled pulsars inferred from their observed spin-downs, and constrain their equatorial ellipticities to be less than 10-8. For each of the five pulsars, we perfor…

Gravitational waves; Neutron stars; Pulsars; Gravitational wave sources010504 meteorology & atmospheric sciencesAstronomyAstrophysicsVela01 natural sciencesGeneral Relativity and Quantum Cosmology[SPI]Engineering Sciences [physics]neutronMillisecond pulsaremission010303 astronomy & astrophysicsQCQBSettore FIS/01Physicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)[PHYS]Physics [physics]PhysicsAstrophysics::Instrumentation and Methods for Astrophysics[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaGravitational-Waves Pulsars Neutron StarsGravitational wavePROPER MOTIONProper motiongr-qcAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesNeutron starGeneral Relativity and Quantum Cosmology (gr-qc)Gravitational-WavesGravitational wavesNeutron starsSEARCHESSettore FIS/05 - Astronomia e AstrofisicaPulsar0103 physical sciencesPulsar[CHIM]Chemical SciencesAstrophysiqueSTFCPulsarsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesGravitational wave sourcescrab pulsarGravitational waveCrab PulsarRCUKAstronomy and AstrophysicsNeutron StarsGravitational waves Neutron stars Pulsars Gravitational wave sourcesLIGONeutron starSpace and Planetary Science[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Guidance to 2018 good practice: ARIA digitally-enabled, integrated, person-centred care for rhinitis and asthma

2019

AIMS: Mobile Airways Sentinel NetworK (MASK) belongs to the Fondation Partenariale MACVIA-LR of Montpellier, France and aims to provide an active and healthy life to rhinitis sufferers and to those with asthma multimorbidity across the life cycle, whatever their gender or socio-economic status, in order to reduce health and social inequities incurred by the disease and to improve the digital transformation of health and care. The ultimate goal is to change the management strategy in chronic diseases. METHODS: MASK implements ICT technologies for individualized and predictive medicine to develop novel care pathways by a multi-disciplinary group centred around the patients. STAKEHOLDERS: Incl…

SENTINEL NETWORKAllergyRespiratory Medicine and AllergyReviewWORLD-HEALTH-ORGANIZATIONDiseaseRhinitis.App; Asthma; Care pathways; DG Santé; MASK; mHealth; Rhinitis0302 clinical medicineQUALITY-OF-LIFEPRECISION MEDICINEDG SantéHealth careMedicine and Health SciencesGRADING QUALITYImmunology and AllergyMedicinemHealthRinitisLungmedicin och allergiRhinitis0303 health sciencesThe MASK study groupPublic sectorApp ; Asthma ; Care pathways ; MASK ; mHealth ; Rhinitis ; DG SanteMOBILE TECHNOLOGY3. Good healthALLERGIC RHINITISCHRONIC RESPIRATORY-DISEASESRinitemHealthCare pathwaysEUROPEAN SYMPOSIUMCLINICAL-PRACTICE GUIDELINESLife Sciences & BiomedicinePulmonary and Respiratory Medicinemedicine.medical_specialtyMASKImmunologySettore MED/10 - Malattie Dell'Apparato RespiratorioPredictive medicine03 medical and health sciencesQuality of life (healthcare)App -MASKAsma030304 developmental biologyAsthmaARIAScience & TechnologyCare pathwaybusiness.industryChange managementCorrectionDG SanteRC581-607medicine.diseaseAsthma030228 respiratory systemApp; Asthma; Care pathways; DG Santé; MASK; mHealth; Rhinitis; Immunology and Allergy; Immunology; Pulmonary and Respiratory MedicineFamily medicineImmunologic diseases. AllergybusinessApp[SDV.MHEP]Life Sciences [q-bio]/Human health and pathology
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Aqueous-phase reactive species formed by fine particulate matter from remote forests and polluted urban air

2021

In the aqueous phase, fine particulate matter can form reactive species (RS) that influence the aging, properties, and health effects of atmospheric aerosols. In this study, we explore the RS yields of aerosol samples from a remote forest (Hyytiälä, Finland) and polluted urban locations (Mainz, Germany; Beijing, China), and we relate the RS yields to different chemical constituents and reaction mechanisms. Ultra-high-resolution mass spectrometry was used to characterize organic aerosol composition, electron paramagnetic resonance (EPR) spectroscopy with a spin-trapping technique was applied to determine the concentrations of ⚫OH, O2⚫-, and carbon- or oxygen-centered organic radicals, and a …

humic-like substancesAtmospheric ScienceReaction mechanism010504 meteorology & atmospheric sciencesQC1-999Radicalchemistry.chemical_element010501 environmental sciences01 natural scienceswater-soluble pm2.5114 Physical scienceselectron-paramagnetic-resonance11. Sustainabilitypersistent free-radicalsQD1-999Chemical compositionScavenging0105 earth and related environmental sciencespolycyclic aromatic-hydrocarbonsatmospheric hydrogen-peroxideAqueous solutionChemistryhydroxyl radicalsPhysicstransition-metalsParticulatesoxalic-acidAerosolChemistry13. Climate actionEnvironmental chemistryCarbonsecondary organic aerosol
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Search for particles decaying into a Z boson and a photon in pp¯ collisions at s=1.96 TeV

2006

Abstract We present the results of a search for a new particle X produced in p p ¯ collisions at s = 1.96 TeV and subsequently decaying to Zγ. The search uses 0.3 fb−1 of data collected with the DO detector at the Fermilab Tevatron Collider. We set limits on the production cross section times the branching fraction σ ( p p ¯ → X ) × B ( X → Z γ ) that range from 0.4 to 3.5 pb at the 95% C.L. for X with invariant masses between 100 and 1000 GeV / c 2 , over a wide range of X decay widths.

PhysicsNuclear and High Energy PhysicsRange (particle radiation)Particle physicsPhoton010308 nuclear & particles physicsBranching fractionTevatron7. Clean energy01 natural scienceslaw.inventionCross section (physics)law0103 physical sciencesHigh Energy Physics::ExperimentFermilabInvariant (mathematics)010306 general physicsColliderPhysics Letters B
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LAB-STEM CELLS

2012

AbstractsCancer ResearchOncologybusiness.industryMedicineNeurology (clinical)Stem cellbusinessCell biologyNeuro-Oncology
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A combined search for the standard model Higgs boson at s=1.96 TeV

2008

AbstractWe present new results of the search for WH→ℓνbb¯ production in pp¯ collisions at a center-of-mass energy of s=1.96 TeV, based on a dataset with integrated luminosity of 0.44 fb−1. We combine these new results with previously published searches by the D0 collaboration, for WH and ZH production analyzed in the E̸Tbb¯ final state, for ZH (→ℓ+ℓ−bb¯) production, for WH (→WWW) production, and for H (→WW) direct production. No signal-like excess is observed either in the WH analysis or in the combination of all D0 Higgs boson analyses. We set 95% C.L. (expected) upper limits on σ(pp¯→WH)×B(H→bb¯) ranging from 1.6 (2.2) pb to 1.9 (3.3) pb for Higgs boson masses between 105 and 145 GeV, to …

PhysicsNuclear and High Energy PhysicsParticle physicsLuminosity (scattering theory)010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyState (functional analysis)7. Clean energy01 natural sciencesStandard ModelNuclear physicsDirect production0103 physical sciencesHiggs bosonHigh Energy Physics::ExperimentCenter of massNeutrino010306 general physicsLeptonPhysics Letters B
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Correlation between work impairment, scores of rhinitis severity and asthma using the MASK-air ® App

2020

Background: In allergic rhinitis, a relevant outcome providing information on the effectiveness of interventions is needed. In MASK-air (Mobile Airways Sentinel Network), a visual analogue scale (VAS) for work is used as a relevant outcome. This study aimed to assess the performance of the work VAS work by comparing VAS work with other VAS measurements and symptom-medication scores obtained concurrently. Methods: All consecutive MASK-air users in 23 countries from 1 June 2016 to 31 October 2018 were included (14 189 users; 205 904 days). Geolocalized users self-assessed daily symptom control using the touchscreen functionality on their smart phone to click on VAS scores (ranging from 0 to 1…

0301 basic medicineSYMPTOMSSmart phoneAllergyEscala visual analógicaINNOVATION[SDV]Life Sciences [q-bio]Medical and Health SciencesCorrelationvisual analogue scale0302 clinical medicineQuality of lifeVisual analogue scaleQUALITY-OF-LIFEMàscaresImmunology and AllergyscoreNoseRinitisRhinitisPRODUCTIVITY COSTSasthma; MASK; rhinitis; score; visual analogue scaleScoreExplained variationResponse VariabilityMobile ApplicationsALLERGIC RHINITISrhinitimedicine.anatomical_structureTRIALSRinite1107 Immunology[SDV.IMM]Life Sciences [q-bio]/ImmunologySmartphonemedicine.medical_specialtyMASKVisual analogue scaleMASK study groupImmunologyMACVIA-ARIA03 medical and health sciencesAllergicrhinitismedicineHumansvisual analogue scale.TECHNOLOGYIMMUNOTHERAPYAsmaAsthmabusiness.industryasthma; MASK; rhinitis; score; visual analogue scale; Humans; Smartphone; Asthma; Mobile Applications; Rhinitis; Rhinitis Allergicasthmamedicine.diseaseRhinitis AllergicAsthmaRHINOCONJUNCTIVITIS030104 developmental biology030228 respiratory system3121 General medicine internal medicine and other clinical medicinePhysical therapyClinical Medicinebusiness[SDV.MHEP]Life Sciences [q-bio]/Human health and pathology
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Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO-Virgo Run O3a

2022

Abbott, R., et al. (LIGO and VIRGO Collaboration)

neutron star: binaryGravitational waves(678)ELECTROMAGNETIC COUNTERPARTSBinary numberAstrophysics01 natural sciencesLIGOHigh-Energy Phenomena and Fundamental PhysicsQCSUPERNOVAQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01education.field_of_study[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Black holesSettore FIS/0506 humanities and the artsGRBEnergy InjectionSearch for gravitational wave transients associated to GRBs - Fermi and Swift satellitesAFTERGLOWPhysical SciencesRELATIVISTIC JETSAstrophysics - High Energy Astrophysical PhenomenaSwiftGravitational waveBlack-Hole330Evolutiongr-qcGamma Ray Burst LIGO Virgo Gravitational WavesAstrophysics::High Energy Astrophysical PhenomenaGeneral Relativity and Quantum Cosmology (gr-qc)0603 philosophy ethics and religionGravitational-wave astronomyNeutron starsENERGY INJECTIONCORE-COLLAPSEeducationGamma-ray burstScience & TechnologyCore-CollapseVirgoRCUKAstronomy and AstrophysicstriggerLuminosity FunctionDewey Decimal Classification::500 | Naturwissenschaften::520 | Astronomie KartographieGamma Ray BurstSpace and Planetary ScienceBLACK-HOLEddc:520gravitational wave astronomyGravitational wave astronomyGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]LIGO(920)Fermi Gamma-ray Space TelescopeAstronomyAstrophysicsGeneral Relativity and Quantum Cosmologyneutron starsENERGYGravitational wave detectorsGamma-ray bursts(629)Neutron Stars Mergers Gravitational Waves010303 astronomy & astrophysicsgravitational waves; gamma ray bursts; LIGO; Virgo; Fermi; SwiftCompact binary stars(283)astro-ph.HEPhysicscompact binary starsgamma-ray burstsgamma-ray bursts ; gravitational waves; LIGO; Virgogravitational waves060302 philosophy[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]PRECURSOR ACTIVITYGravitational wave astronomy(675)Gamma-ray burstsGW_HIGHLIGHT[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PopulationCompact binary starssatelliteFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & Astrophysicsgamma ray: burstMASS1STGLASTGamma-ray bursts; Gravitational wave astronomy; Gravitational waves; Gravitational wave detectors0103 physical sciencesSTFCFermigravitational waves; gamma-ray bursts; LIGO; Virgo; Fermi; SwiftGravitational wavegravitational radiationgamma ray burstsgamma-ray burts--black holesLIGOEVOLUTIONOBSERVING RUNNeutron stars(1108)Neutron starPhysics and Astronomy[SDU]Sciences of the Universe [physics]LUMINOSITY FUNCTIONBlack holes(162)INJECTIONEMISSION
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A Gravitational-wave Measurement of the Hubble Constant Following the Second Observing Run of Advanced LIGO and Virgo

2021

This paper presents the gravitational-wave measurement of the Hubble constant (H 0) using the detections from the first and second observing runs of the Advanced LIGO and Virgo detector network. The presence of the transient electromagnetic counterpart of the binary neutron star GW170817 led to the first standard-siren measurement of H 0. Here we additionally use binary black hole detections in conjunction with galaxy catalogs and report a joint measurement. Our updated measurement is H 0 = km s-1 Mpc-1 (68.3% of the highest density posterior interval with a flat-in-log prior) which is an improvement by a factor of 1.04 (about 4%) over the GW170817-only value of km s-1 Mpc-1. A significant …

Gravitacióneutron star: binarycosmological model010504 meteorology & atmospheric sciencesAstronomyGravitational Waves Hubble constant O2 LIGO Virgodetector: network01 natural sciencesCosmologyGeneral Relativity and Quantum CosmologyLIGOdark energy010303 astronomy & astrophysicsQCPhysicsSettore FIS/01Hubble constantSettore FIS/05CATALOGPhysical Sciencessymbols[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - Cosmology and Nongalactic AstrophysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)DATA RELEASECOSMOLOGICAL PARAMETERSFOS: Physical sciencesO2General Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & AstrophysicsLUMINOSITY FUNCTIONSgravitational radiation: direct detectionGravitational-wave astronomy1STArticleelectromagnetic field: productionsymbols.namesakeBinary black hole0103 physical sciencesDISTRIBUTIONS/dk/atira/pure/subjectarea/asjc/1900/1912K-CORRECTIONSSDG 7 - Affordable and Clean EnergyAstrophysiqueSTFC0105 earth and related environmental sciencesGravitational Waves/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyScience & TechnologyGravitational waveVirgoAstronomyRCUKAstronomy and Astrophysicscosmology; gravitational waves; Hubble constant310 Galaxies and CosmologyLIGOGalaxyEVOLUTIONDewey Decimal Classification::500 | Naturwissenschaften::520 | Astronomie Kartographiegravitational radiation detectorVIRGOblack hole: binarySpace and Planetary Science[SDU]Sciences of the Universe [physics]DENSITYgravitational radiation: emissionDark energyAstronomiaddc:520/dk/atira/pure/subjectarea/asjc/3100/3103galaxyGravitational wave astronomy[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Hubble's lawThe Astrophysical Journal
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Impact of asymptomatic COVID-19 patients in global surgical practice during the COVID-19 pandemic

2020

The rapid spread of COVID-19 has changed the global surgical care. Patients infected with COVID-19 may present without typical symptoms, and such asymptomatic patients may potentially trigger in-hospital outbreaks by transmitting the disease to health care providers and other hospitalized patients. Further, asymptomatic COVID-19 patients have worse postop- erative outcomes with an unexpectedly high morbidity and mortality, reaching 20⋅5 per cent deaths. However, we do not have objective global data on this issue. In an attempt to clarify the current global surgical practice under the COVID-19 pandemic particularly focusing on the preoperative screening of asymptomatic COVID-19 patients, we …

2019-20 coronavirus outbreakmedicine.medical_specialtyCoronavirus disease 2019 (COVID-19)covid-19 pandemic surgerySevere acute respiratory syndrome coronavirus 2 (SARS-CoV-2)Settore MED/18 - CHIRURGIA GENERALEMEDLINECOVID-19. Global surgery.AsymptomaticCOVID-19 Critical Pathways Cross Infection Cross-Sectional Studies Health Care Surveys Humans Pandemics Postoperative Complications SARS-CoV-2 Surgical Procedures Operative Asymptomatic InfectionsCOVID-19; Critical Pathways; Cross Infection; Cross-Sectional Studies; Health Care Surveys; Humans; Pandemics; Postoperative Complications; SARS-CoV-2; Surgical Procedures Operative; Asymptomatic InfectionsNOsurgeryTumours of the digestive tract Radboud Institute for Health Sciences [Radboudumc 14]Postoperative ComplicationsPandemicCorrespondencemedicineHumansPandemicsAsymptomatic InfectionsLS7_4COVIDCross InfectionSurgical ProceduresCritical pathwaysbusiness.industrySARS-CoV-2pandemicCOVID-19Surgical proceduresOperativeSettore MED/18covid 19 surgical practiceCOVID-19 - surgeryCross-Sectional StudiesSurgical Procedures OperativeHealth Care SurveysEmergency medicineCritical Pathwaysmedicine.symptombusiness
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Search for tt¯ resonances in the lepton plus jets final state in pp¯ collisions at s=1.96TeV

2008

We present a search for a narrow-width heavy resonance decaying into top quark pairs X->ttbar in ppbar collisions at sqrt{s}=1.96TeV using approximately 0.9fb^-1 of data collected with the D0 detector at the Fermilab Tevatron Collider. This analysis considers ttbar candidate events in the lepton plus jets channel with at least one identified b jet and uses the ttbar invariant mass distribution to search for evidence of resonant production. We find no evidence for a narrow resonance X decaying to ttbar. Therefore, we set upper limits on sigma*B(X->ttbar) for different hypothesized resonance masses using a Bayesian approach. For a Topcolor-assisted technicolor model, the existence of a leptop…

PhysicsNuclear and High Energy PhysicsParticle physicsTop quark010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHadronTopcolorTevatronTechnicolor7. Clean energy01 natural sciencesNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentInvariant mass010306 general physicsLeptonBosonPhysics Letters B
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Model-independent measurement of the W-boson helicity in top-quark decays at D0.

2008

Made available in DSpace on 2022-04-28T20:37:47Z (GMT). No. of bitstreams: 0 Previous issue date: 2008-02-14 Science and Technology Facilities Council We present the first model-independent measurement of the helicity of W bosons produced in top quark decays, based on a 1fb-1 sample of candidate tt̄ events in the dilepton and lepton plus jets channels collected by the D0 detector at the Fermilab Tevatron pp̄ Collider. We reconstruct the angle θ* between the momenta of the down-type fermion and the top quark in the W boson rest frame for each top quark decay. A fit of the resulting cos θ* distribution finds that the fraction of longitudinal W bosons f0=0.425±0.166(stat)±0.102(syst) and the f…

PhysicsTop quarkParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTevatronGeneral Physics and AstronomyFermionRest frame01 natural sciencesHelicityNuclear physicsParticle decay0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsBosonLepton
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All-sky search for short gravitational-wave bursts in the second Advanced LIGO and Advanced Virgo run

2019

We present the results of a search for short-duration gravitational-wave transients in the data from the second observing run of Advanced LIGO and Advanced Virgo. We search for gravitational-wave transients with a duration of milliseconds to approximately one second in the 32-4096 Hz frequency band with minimal assumptions about the signal properties, thus targeting a wide variety of sources. We also perform a matched-filter search for gravitational-wave transients from cosmic string cusps for which the waveform is well-modeled. The unmodeled search detected gravitational waves from several binary black hole mergers which have been identified by previous analyses. No other significant event…

AstronomyGravitational waves detectionAstrophysicsdetector: network01 natural sciencesSignalGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsGravitational waves detection Stochastic gravitational-wavebinary [black hole]LIGOgravitational waveQCQBmedia_commonastro-ph.HEPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01Physicsgravitational waves neutron starsgravitational wavesGeneral relativityburst [gravitational radiation]network [detector]Physical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]direct detection [gravitational radiation]Advanced VirgoAstrophysics - High Energy Astrophysical PhenomenaFrequency bandsensitivity [detector]gr-qcmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesalternative theories of gravityGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & Astrophysicsgravitational radiation: direct detectionemission [gravitational radiation]Binary black holeSettore FIS/05 - Astronomia e Astrofisicabinary: coalescence0103 physical sciencesgravitational radiation: burstAdvanced LIGOWaveformddc:530010306 general physicscosmic stringSTFCScience & Technology010308 nuclear & particles physicsGravitational waveRCUKStochastic gravitational-waveGravitational Wave PhysicsLIGOgravitational radiation detectorgravitational waves; Advanced LIGO; Advanced VirgoCosmic stringdetector: sensitivityVIRGOPhysics and Astronomyblack hole: binarySkygravitational radiation: emissionDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikcoalescence [binary][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Allergic Rhinitis and its Impact on Asthma (ARIA) Phase 4 (2018): Change management in allergic rhinitis and asthma multimorbidity using mobile techn…

2019

Allergic Rhinitis and its Impact on Asthma (ARIA) has evolved from a guideline by using the best approach to integrated care pathways using mobile technology in patients with allergic rhinitis (AR) and asthma multimorbidity. The proposed next phase of ARIA is change management, with the aim of providing an active and healthy life to patients with rhinitis and to those with asthma multimorbidity across the lifecycle irrespective of their sex or socioeconomic status to reduce health and social inequities incurred by the disease. ARIA has followed the 8-step model of Kotter to assess and implement the effect of rhinitis on asthma multimorbidity and to propose multimorbid guidelines. A second c…

AllergyAllergy:Medicina Básica [Ciências Médicas]asthma -- guidelineAllergic asthmaDECISION-MAKINGAllergic Rhinitis and Its Impact on AsthmaGUIDELINESMedical and Health SciencesMedical Records0302 clinical medicineHealth careImmunology and Allergy030212 general & internal medicineAllergic Rhinitis and Its Impact on Asthma; asthma; Change management; rhinitis; Immunology and Allergy; ImmunologyMASK-RHINITISComputingMilieux_MISCELLANEOUSRinitismobilne aplikacijeupravljanje spremembMedical recordGLOBAL STRATEGYWORK PRODUCTIVITYTelemedicinemobile applications3. Good healthAsma alérgicarhiniti1107 ImmunologyCiências Médicas::Medicina Básicaklinične potiallergic -- guidelineLife Sciences & BiomedicineHumanPATIENT PARTICIPATIONAllergic RhinitisTelemedicinemedicine.medical_specialtyanimal structuresmultimorbidityEUROPEAN INNOVATION PARTNERSHIPImmunologyChange Management[object Object]Settore MED/10 - Malattie Dell'Apparato RespiratorioAsthma/diagnosisCHRONIC DISEASESMACVIA-ARIA03 medical and health sciencesrhinitismedicinemultimorbidnostQUALITYHumanscritical pathwaysastma -- smernicaPatient participationAsmaudc:616.2AsthmaScience & TechnologyARIAbusiness.industryAllergic Rhinitis and Its Impact on Asthma; asthma; Change management; rhinitis; Change Management; Humans; Medical Records; Asthma; Multimorbidity; Rhinitis Allergic; TelemedicineSettore MED/09 - MEDICINA INTERNAchange managementMultimorbidityMobile Airways Sentinel Network (MASK) Study GroupGuidelineasthmata3121medicine.diseaseRinite alérgicaRhinitis AllergicRhinitis Allergic/diagnosisAsthmaIntegrated carealergijski rinitis -- smernicaAllergic Rhinitis and Its Impact on Asthma asthma Change management rhinitis Immunology and Allergy Immunology030228 respiratory systemFamily medicine3121 General medicine internal medicine and other clinical medicineMedical RecordClinical Medicinebusiness[SDV.MHEP]Life Sciences [q-bio]/Human health and pathologyImpact on AsthmaJournal of Allergy and Clinical Immunology
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Search for Subsolar-Mass Ultracompact Binaries in Advanced LIGO's First Observing Run

2018

We present the first Advanced LIGO and Advanced Virgo search for ultracompact binary systems with component masses between 0.2 $M_\odot$ - 1.0 $M_\odot$ using data taken between September 12, 2015 and January 19, 2016. We find no viable gravitational wave candidates. Our null result constrains the coalescence rate of monochromatic (delta function) distributions of non-spinning (0.2 $M_\odot$, 0.2 $M_\odot$) ultracompact binaries to be less than $1.0 \times 10^6 \text{Gpc}^{-3} \text{yr}^{-1}$ and the coalescence rate of a similar distribution of (1.0 $M_\odot$, 1.0 $M_\odot$) ultracompact binaries to be less than $1.9 \times 10^4 \text{Gpc}^{-3} \text{yr}^{-1}$ (at 90 percent confidence). N…

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftendensity: fluctuationMACHOAstronomyGeneral Physics and AstronomyPrimordial black holeAstrophysicsCoalescence01 natural sciencesGeneral Relativity and Quantum CosmologylocalizationLIMITSddc:550Massive compact halo objectLIGOneutron starQCQBPhysicseducation.field_of_studyPhysicsDensity fluctuationBinary systemsgravitational wavesPhysical SciencesSearch enginesastro-ph.COblack hole: primordialAstrophysics - Cosmology and Nongalactic AstrophysicsGravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)gr-qcBinary formationAstrophysics::High Energy Astrophysical PhenomenaPopulationDark matterPhysics MultidisciplinaryEarly universeFOS: Physical sciencesPrimordial black holesGeneral Relativity and Quantum Cosmology (gr-qc)dark matter: densityAstrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesCoalescence rateGravitation and AstrophysicsPhysics and Astronomy (all)General Relativity and Quantum Cosmologybinary: coalescence0103 physical sciencesddc:530Delta functions010306 general physicseducationSTFCAstrophysics::Galaxy AstrophysicsScience & Technologymass: solar010308 nuclear & particles physicsGravitational waveStellar evolutionsbinary: formationgravitational radiationRCUKblack hole: massGalaxiesStarsGalaxyLIGOBlack holeVIRGOPhysics and Astronomyblack hole: binarygravitational radiation: emissionDewey Decimal Classification::500 | Naturwissenschaften::530 | PhysikMicro-lensing[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Search for a scalar or vector particle decaying into Zγ in pp¯ collisions at s=1.96 TeV

2009

We present a search for a narrow scalar or vector resonance decaying into Z gamma with a subsequent Z boson decay into a pair of electrons or moons. The data for this search were collected with the D circle divide detecror at the Fermilab Tevatron p (p) over bar collider at a center of mass energy root s = 1.96 TeV. Using 1.1 (1.0) fb(-1) of data, we observe 49 (50) candidate events in the electron (muon) channel, in good agreement with the standard model prediction. From the combination of both channels, we derive 95% C.L. upper limits on the cross section times branching fraction (sigma x B) into Z gamma. These limits range from 0.19 (0.20) pb for a scalar (vector) resonance mass of 600 G…

PhysicsNuclear and High Energy PhysicsParticle physicsPhotonMuon010308 nuclear & particles physicsBranching fractionScalar (mathematics)TevatronElectron01 natural sciencesNuclear physics0103 physical sciencesHigh Energy Physics::ExperimentFermilab010306 general physicsBosonPhysics Letters B
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Search for Gravitational-wave Signals Associated with Gamma-Ray Bursts during the Second Observing Run of Advanced LIGO and Advanced Virgo

2019

We present the results of targeted searches for gravitational-wave transients associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo, which took place from 2016 November to 2017 August. We have analyzed 98 gamma-ray bursts using an unmodeled search method that searches for generic transient gravitational waves and 42 with a modeled search method that targets compact-binary mergers as progenitors of short gamma-ray bursts. Both methods clearly detect the previously reported binary merger signal GW170817, with p-values of <9.38 10-6 (modeled) and 3.1 10-4 (unmodeled). We do not find any significant evidence for gravitational-wave signals associate…

Burst astrophysicAstrofísicaneutron star: binary010504 meteorology & atmospheric sciencesBinary numberAstrophysics01 natural sciencesLIGOQCSUPERNOVArelativistic jetsQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01counterpartGRBGravitational waves (678)Physical SciencesRELATIVISTIC JETSAstrophysics - High Energy Astrophysical PhenomenaGravitational waveGravitationstarsblack-holeAstrophysics::High Energy Astrophysical PhenomenaGeneral Relativity and Quantum Cosmology (gr-qc)precursor activityGravitational wavesSettore FIS/05 - Astronomia e AstrofisicasupernovaCORE-COLLAPSEGamma-ray burstGravitational wave sourcesScience & TechnologyVirgoRCUKAstronomy and AstrophysicsHigh energy astrophysics (739)RedshiftDewey Decimal Classification::500 | Naturwissenschaften::520 | Astronomie Kartographiedetector: sensitivityVIRGOSpace and Planetary Sciencegravitational radiation: emissionBLACK-HOLEddc:520Gravitational wave astronomyGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]STARSGravitacióAstronomySignalGeneral Relativity and Quantum CosmologyBurst astrophysicslocalizationemission010303 astronomy & astrophysicsPhysicsDetectorGamma-ray bursts (629)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sourcePRECURSOR ACTIVITYGamma-ray burstsLIGO (920)High energy astrophysicsdata analysis methodBurst astrophysics (187)FOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstAstronomy & AstrophysicsMASSgravitational radiation: direct detectionGravitational wave astronomy Gravitational wave sources LIGO; Gravitational waves Gamma-ray bursts Burst astrophysics High energy astrophysicsGravitational wave astronomy (675)electromagnetic field: production0103 physical sciencesnumerical calculationsGRB; gravitational waves; LIGO; VirgoSTFC0105 earth and related environmental sciencesgravitational wavesneutron starsGravitational waveCOUNTERPARTgravitational radiationLIGOcore-collapsegravitational radiation detectorGravitational wave sources (677)radiationNeutron starPhysics and AstronomymassRADIATIONEMISSIONGravitational wave astronomy; Gravitational wave sources; LIGO; Gravitational waves; Gamma-ray bursts; Burst astrophysics; High energy astrophysics
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Experimental Discrimination between Charge2e/3Top Quark and Charge4e/3Exotic Quark Production Scenarios

2007

We present the first experimental discrimination between the 2e/3 and 4e/3 top quark electric charge scenarios, using top quark pairs (ttbar) produced in ppbar collisions at sqrt{s}=1.96 TeV by the Fermilab Tevatron collider. We use 370 pb-1 of data collected by the D0 experiment and select events with at least one high transverse momentum electron or muon, high transverse energy imbalance, and four or more jets. We discriminate between b- and bbar-quark jets by using the charge and momenta of tracks within the jet cones. The data is consistent with the expected electric charge, |q|=2e/3. We exclude, at the 92% C.L., that the sample is solely due to the production of exotic quark pairs QQba…

QuarkPhysicsParticle physicsTop quarkMuon010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyTevatronGeneral Physics and AstronomyTop quark condensateJet (particle physics)01 natural sciences7. Clean energyBottom quarkElectric chargeNuclear physics0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsPhysical Review Letters
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A Fermi Gamma-Ray Burst Monitor Search for Electromagnetic Signals Coincident with Gravitational-wave Candidates in Advanced LIGO's First Observing R…

2019

We present a search for prompt gamma-ray counterparts to compact binary coalescence gravitational wave (GW) candidates from Advanced LIGO's first observing run (O1). As demonstrated by the multimessenger observations of GW170817/GRB 170817A, electromagnetic and GW observations provide complementary information about the astrophysical source and, in the case of weaker candidates, may strengthen the case for an astrophysical origin. Here we investigate low-significance GW candidates from the O1 compact-binary coalescence searches using the Fermi Gamma-ray Burst Monitor (GBM), leveraging its all-sky and broad energy coverage. Candidates are ranked and compared to background to measure signific…

AstrofísicaGravitacióAstronomyAstrophysics::High Energy Astrophysical Phenomenagamma-ray burst: generalFOS: Physical sciencesAstrophysicsAstronomy & Astrophysicsgeneral [gamma-ray burst]01 natural sciencesCoincidenceCoincident0103 physical sciences010306 general physics010303 astronomy & astrophysicsgravitational waveSTFCQCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01Physicsastro-ph.HEScience & TechnologySolar flareGravitational wavegamma-ray burst: general; gravitational waves; Astronomy and Astrophysics; Space and Planetary ScienceRCUKAstronomy and AstrophysicsAstronomy and AstrophysicLIGOPhysics and Astronomygravitational wavesSpace and Planetary SciencePhysical Sciencesgamma-ray burst: general; gravitational wavesgeneral; gravitational waves; Astronomy and Astrophysics; Space and Planetary Science [gamma-ray burst]False alarmAstrophysics - High Energy Astrophysical PhenomenaGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Fermi Gamma-ray Space Telescope
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Erratum to: Guidelines for the use and interpretation of assays for monitoring autophagy (3rd edition) (Autophagy, 12, 1, 1-222, 10.1080/15548627.201…

2016

non presente

Molecular Biology; Cell BiologyCell BiologySettore BIO/06 - Anatomia Comparata E CitologiaMolecular Biology
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Search for single production of scalar leptoquarks in pp¯ collisions decaying into muons and quarks with the D0 detector

2007

We report on a search for second generation leptoquarks LQ_2 which decay into a muon plus quark in p\bar{p} collisions at a center-of-mass energy of sqrt{s} = 1.96 TeV in the D0 detector using an integrated luminosity of about 300 pb-1. No evidence for a leptoquark signal is observed and an upper bound on the product of the cross section for single leptoquark production times branching fraction beta into a quark and a muon was determined for second generation scalar leptoquarks as a function of the leptoquark mass. This result has been combined with a previously published D0 search for leptoquark pair production to obtain leptoquark mass limits as a function of the leptoquark-muon-quark cou…

PhysicsQuarkNuclear and High Energy PhysicsParticle physicsMuon010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologyScalar (mathematics)Lambda01 natural sciencesUpper and lower boundsNuclear physicsPair production0103 physical sciencesHigh Energy Physics::ExperimentLeptoquark010306 general physicsPhysics Letters B
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Search for W′ boson production in the W′→tb¯ decay channel

2006

We present a search for the production of a new heavy gauge boson W' that decays to a top quark and a bottom quark. We have analyzed 230 pb(-1) of data collected with the DO detector at the Fermilab Tevatron collider at a center-of-mass energy of 1.96 TeV. No significant excess of events above the standard model expectation is found in any region of the final state invariant mass distribution. We set upper limits on the production cross section of W' bosons times branching ratio to top quarks at the 95% confidence level for several different W, boson masses. We exclude masses between 200 and 610 GeV for a W' boson with standard-model-like couplings, between 200 and 630 GeV for a W, boson wi…

QuarkPhysicsNuclear and High Energy PhysicsGauge bosonTop quarkParticle physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyScalar boson7. Clean energy01 natural sciencesBottom quarkStandard ModelNuclear physicsW and Z bosons0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsBosonPhysics Letters B
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GW170817: Measurements of Neutron Star Radii and Equation of State

2018

On 17 August 2017, the LIGO and Virgo observatories made the first direct detection of gravitational waves from the coalescence of a neutron star binary system. The detection of this gravitational-wave signal, GW170817, offers a novel opportunity to directly probe the properties of matter at the extreme conditions found in the interior of these stars. The initial, minimal-assumption analysis of the LIGO and Virgo data placed constraints on the tidal effects of the coalescing bodies, which were then translated to constraints on neutron star radii. Here, we expand upon previous analyses by working under the hypothesis that both bodies were neutron stars that are described by the same equation…

Dewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftenneutron star: binaryAstronomyGeneral Physics and AstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGRAVITATIONAL-WAVESGW170817BINARIESddc:550DENSELIGODENSE MATTEREquation of State010303 astronomy & astrophysicsQCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)astro-ph.HEPhysicsNeutron Star RadiusPhysicsGravitational effectsEquations of stateParametrizationsElectromagnetic observationsGravitational-wave signals3. Good healthQUADRUPOLE-MOMENTSMacroscopic propertiesPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave sourceAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaEquations of state of nuclear matterGravitational wavesaturation: densityBinary neutron starsNUCLEON MATTEREquations of state of nuclear matter; Gravitational wave sources; Gravitational waves; Nuclear matter in neutron starsGeneral relativitygr-qcAstrophysics::High Energy Astrophysical PhenomenaGW170817 Neutron Star Radius Equation of StatePhysics Multidisciplinaryneutron star: spinFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsGravity wavesgravitational radiation: direct detectionGravitation and AstrophysicsNuclear matter in neutron starsGravitational waveselectromagnetic field: productionPhysics and Astronomy (all)Pulsargalaxy: binary0103 physical sciencesddc:530NeutronMASSESSTFCequation of state: parametrizationAstrophysics::Galaxy AstrophysicsNeutronsExtreme conditionsGravitational wave sourcesEquation of stateScience & TechnologyNeutron Star Interior Composition Explorer010308 nuclear & particles physicsGravitational wavegravitational radiationRCUKFlocculationSaturation densityUNIVERSAL RELATIONSStarsLIGOgravitational radiation detectorNeutron starStarsVIRGOPhysics and Astronomygravitational radiation: emissionneutron star: binary: coalescenceDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]MATTER
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Search for GW signals associated with GRBs

2021

We present the results of targeted searches for gravitational-wave transients associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo, which took place from 2016 November to 2017 August. We have analyzed 98 gamma-ray bursts using an unmodeled search method that searches for generic transient gravitational waves and 42 with a modeled search method that targets compact-binary mergers as progenitors of short gamma-ray bursts. Both methods clearly detect the previously reported binary merger signal GW170817, with p-values of <9.38x10^-6^ (modeled) and 3.1x10^-4^ (unmodeled). We do not find any significant evidence for gravitational-wave signals assoc…

Astrophysics and AstronomyGamma-ray astronomyhigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstellar astronomyGamma ray burstsGravitational wavesCosmologyobservational astronomyGamma ray astronomyGamma-ray burstsAstrophysical ProcessesNatural Sciences
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CCDC 1471779: Experimental Crystal Structure Determination

2016

Related Article: W. Sun, J. Li|2016|Acta Crystallogr.,Sect.E:Cryst.Commun.|72|1116|doi:10.1107/S2056989016010562

Space GroupCrystallographybis(2-methyl-1H-imidazole)-(5101520-tetrakis(4-methylphenyl)porphyrinato)-iron(iii) perchlorate tetrahydrofuran solvateCrystal SystemCrystal StructureCell ParametersExperimental 3D Coordinates
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