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showing 12 related works from this author

Kinetic analysis of insulin resistance and serum adipocytokines levels during peginterferon alpha-2A plus ribavirin therapy in non-diabetic HCV patie…

2006

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Global, regional, and national burden of chronic kidney disease, 1990–2017: a systematic analysis for the Global Burden of Disease Study 2017

2020

Abstract: Background Health system planning requires careful assessment of chronic kidney disease (CKD) epidemiology, but data for morbidity and mortality of this disease are scarce or non-existent in many countries. We estimated the global, regional, and national burden of CKD, as well as the burden of cardiovascular disease and gout attributable to impaired kidney function, for the Global Burden of Diseases, Injuries, and Risk Factors Study 2017. We use the term CKD to refer to the morbidity and mortality that can be directly attributed to all stages of CKD, and we use the term impaired kidney function to refer to the additional risk of CKD from cardiovascular disease and gout. Methods Th…

Systems AnalysisGoutCost effectiveness030204 cardiovascular system & hematologyGlobal HealthGLOMERULAR-FILTRATION-RATEGlobal Burden of DiseaseCOST-EFFECTIVENESS0302 clinical medicineCause of DeathPrevalenceGlobal healthDiabetic NephropathiesRegistries030212 general & internal medicineSUB-SAHARAN AFRICA11 Medical and Health SciencesIncidenceMortality rate1. No povertyGeneral MedicineHälsovetenskaperGBD Chronic Kidney Disease CollaborationCKD-EPI EQUATION3. Good healthEuropeCardiovascular Diseases/dk/atira/pure/sustainabledevelopmentgoals/good_health_and_well_beingQuality-Adjusted Life YearsLife Sciences & BiomedicineAsiaOceania195 COUNTRIESATHEROSCLEROSIS RISKCARDIOVASCULAR OUTCOMESRisk AssessmentArticle03 medical and health sciencesMedicine General & InternalSDG 3 - Good Health and Well-beingRISK-FACTORGeneral & Internal MedicineEnvironmental healthHealth SciencesmedicineHumansGBD chronic kidney diseaseMortalityRisk factorRenal Insufficiency ChronicDisease burdenQMScience & TechnologyAustralasiabusiness.industryPERIPHERAL ARTERIAL-DISEASEBayes Theoremmedicine.diseaseHealth SurveysQuality-adjusted life yearRENAL-DISEASELatin AmericaYears of potential life lostAfricaNorth AmericaHuman medicinebusinessRCKidney disease
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EFFICACY OF ARGENTUM-QUARTZ SOLUTION IN THE TREATMENT OF PERIANAL FISTULAS: A PRELIMINARY STUDY

2015

Objective: Nowadays, an optional and effective medical surgery remains the gold standard for perianal fistulas. Hereby we reported preliminary rsults in favor of using Argentum-Quartz solution for both primary and recurrent perianal fisrtulas. Methods: Three patients with intersphimncter and extrasphinteric fistulas were enrolled. Argentum-Quartz solution was administrated twice a week for sa period of 4 weeks, followed by a pause of 8 days and then another 4 weeks of treatment, totally 16 administrations. After treatment, all patients were monitored for 4-months follow-up. Results: Complete closures of 2 extrasphinteric fistulas and a partial closure with absence of inflammation and supera…

Settore MED/18 - Chirurgia GeneraleSettore BIO/06 - Anatomia Comparata E CitologiaPerianal fistulas alternative treatment argentum-quartz solution extrashpinteric fistulas
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Passive degassing at Nyiragongo (D.R. Congo) and Etna (Italy) volcanoes: the chemical characterization of the emissions and assessment of their uptak…

2014

Etna Nyiragongo trace elements emissions
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Relaxation phenomena in mixed isomeric alcohols by Mandelstam-Brillouin scattering

1991

Mandelstam-Brillouin scattering data in mixed isomeric alcohols n-pentanol (nPe-OH) and 2-methyl-2-butanol (2Me-2BuOH) are presented. The hypersonic velocity and normalized absorption are measured as a function of the scattering angle, in the temperature range from - 15-degrees-C to + 45-degrees-C, and as a function of n-PeOH molar fraction going from the pure n-PeOH to the pure 2Me-2BuOH. The experimental results confirm the existence of a shear relaxation phenomenon in the GHz region, that has been previously detected in pure liquids. The temperature dependence of the relaxation time tau-s and of the shear modulus G-infinity evaluated within viscoelastic liquid models, support the existen…

DYNAMICS2-METHYL-2-BUTANOLBiophysicsThermodynamicsN-PENTANOLViscoelasticityShear modulusOpticsRAMAN-SPECTROSCOPYBrillouin scatteringTEMPERATURESSUPERCOOLED WATERPhysical and Theoretical ChemistryMolecular BiologyBulk modulusChemistrybusiness.industryScatteringRelaxation (NMR)STATIC DIELECTRIC-CONSTANTCondensed Matter PhysicsLIGHT-SCATTERINGShear (sheet metal)Shear flowbusinessBONDVISCOSITYMolecular Physics
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Emergence of non-Markovianity in the emission process of an atom in a half-cavity

2014

We study quantum non-Markovianity in the early stage of the emission process of a two-level atom coupled to a semi-infinite waveguide, where the waveguide termination behaves as a perfect mirror. Specifically, we restrict to the analysis of the process for times shorter than twice the time delay t_d, where t_d is the duration of a round trip along the atom-mirror path. We show the emergence of a threshold in the parameters space separating the Markovian and non-Markovian regions.

PhysicsQuantum PhysicsProcess (computing)FOS: Physical sciencesAtom (order theory)Markov processopen quantum systemsParameter spacenon-Markovianity open quantum systems spontaneous emission waveguide QEDCondensed Matter Physicsnon-MarkovianityAtomic and Molecular Physics and Opticssymbols.namesakePerfect mirrorwaveguide QEDQuantum mechanicsPath (graph theory)symbolsWaveguide (acoustics)Quantum Physics (quant-ph)spontaneous emissionQuantumMathematical Physics
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Upper limits on the isotropic gravitational-wave background from Advanced LIGO and Advanced Virgo's third observing run

2021

We report results of a search for an isotropic gravitational-wave background (GWB) using data from Advanced LIGO's and Advanced Virgo's third observing run (O3) combined with upper limits from the earlier O1 and O2 runs. Unlike in previous observing runs in the advanced detector era, we include Virgo in the search for the GWB. The results are consistent with uncorrelated noise, and therefore we place upper limits on the strength of the GWB. We find that the dimensionless energy density $\Omega_{\rm GW}\leq 5.8\times 10^{-9}$ at the 95% credible level for a flat (frequency-independent) GWB, using a prior which is uniform in the log of the strength of the GWB, with 99% of the sensitivity comi…

coalescencePhysics and Astronomy (miscellaneous)gravitation: modelAstronomypopulationAstrophysicspower spectrum01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsGravitational wave backgroundbackground: magneticenergy: densitycorrelation functionLIGOQCPOPULATIONQBPhysicsSettore FIS/01education.field_of_studySpectral indexPhysicsstar-formation ratestatistical analysis: BayesianIsotropicSTAR-FORMATION RATE; BLACK-HOLE; MASS; COALESCENCE; POPULATION; EVOLUTION; RADIATION; PROSPECTSCOALESCENCEPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]LIGO; Virgo; isotropic gravitational-wave backgroundIsotropic gravitational wave backgrounds with LIGO and VirgoAstrophysics - Cosmology and Nongalactic Astrophysicsgravitational radiation: polarizationdata analysis methodCosmology and Nongalactic Astrophysics (astro-ph.CO)black-holePopulationFOS: Physical sciencesGravitational Waves LIGO Virgo Stochastic Background IsotropicGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsMASSSTAR-FORMATION RATEBinary black holebinary: coalescence0103 physical sciencesevolutionddc:530SDG 7 - Affordable and Clean Energy2ND010306 general physicseducationGravitational Waves/dk/atira/pure/sustainabledevelopmentgoals/affordable_and_clean_energyScience & Technology010308 nuclear & particles physicsGravitational waveVirgogravitational radiation: backgroundSpectral densityprospectsbinary: compactnoise: magneticLIGOEVOLUTIONisotropic gravitational-wave backgroundBlack holeradiationdetector: sensitivityPROSPECTSVIRGOpolarization: scalarblack hole: binaryGravitation Cosmology AstrophysicsBLACK-HOLEpolarization: vectorRADIATIONmassStochastic BackgroundDewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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FOLLOW-UP DI SVILUPPO NEUROPSICOMOTORIO E CORRELAZIONI CON IL PONDERAL INDEX IN UN CAMPIONE DI NEONATI LATE PRETERM

2015

late preterm, sviluppo neuropsicomotorio, ponderal index

Settore MED/38 - Pediatria Generale E Specialisticalate preterm sviluppo neuropsicomotorio ponderal index
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Constraints on Cosmic Strings Using Data from the Third Advanced LIGO–Virgo Observing Run

2021

We search for gravitational-wave signals produced by cosmic strings in the Advanced LIGO and Virgo full O3 data set. Search results are presented for gravitational waves produced by cosmic string loop features such as cusps, kinks and, for the first time, kink-kink collisions.cA template-based search for short-duration transient signals does not yield a detection. We also use the stochastic gravitational-wave background energy density upper limits derived from the O3 data to constrain the cosmic string tension, $G\mu$, as a function of the number of kinks, or the number of cusps, for two cosmic string loop distribution models.cAdditionally, we develop and test a third model which interpolat…

High Energy Physics - TheoryDewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftengravitational radiation: stochasticAstronomyCosmic stringsWAVESGeneral Physics and Astronomy01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologyGravitation Cosmology & AstrophysicsGravitationLIMITSCosmic strings & domain wallCosmology & Astrophysicsddc:550Distribution modelsTransient signalenergy: densityLIGOQCstochastic modelLIGO Scientific CollaborationShort durationsCosmic strings & domain walls; Gravitational waves; Gravitation Cosmology & AstrophysicsQBPhysicsCosmic strings & domain wallskinkSettore FIS/03Stochastic systems[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thPhysicsGravitational effectsarticleGRAVITATIONAL-RADIATION; LIMITS; EVOLUTION; WAVEStensionGravitational-wave signalsCosmologyPhysical Sciencesastro-ph.COGrand unified theories[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational waveAstrophysics - Cosmology and Nongalactic AstrophysicsGravitational effects; Gravity waves; Stochastic models; Stochastic systems; Cosmic strings; Distribution models; Grand unified theories; Gravitational-wave signals; Orders of magnitude; Short durations; Template-based; Transient signalGravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)gr-qcPhysics MultidisciplinaryGRAVITATIONAL-RADIATIONO3FOS: Physical sciencesContext (language use)General Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsPhysics and Astronomy(all)Gravity wavesGravitation and AstrophysicsGravitational wavesTheoretical physicsGeneral Relativity and Quantum Cosmologystatistical analysis0103 physical sciencesTemplate-basedCosmic Strings O3 LIGO Virgoddc:530010306 general physicscosmic stringSTFCInflation (cosmology)Science & Technology010308 nuclear & particles physicsGravitational wavestring tensionVirgogravitational radiation: backgroundRCUKLIGOEVOLUTIONCosmic stringStochastic modelsOrders of magnitudeVIRGOHigh Energy Physics - Theory (hep-th)Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910

2021

We present a search for continuous gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and Virgo. The search is enabled by a contemporaneous timing ephemeris obtained using NICER data. The NICER ephemeris has also been extended through 2020 October and includes three new glitches. PSR J0537-6910 has the largest spin-down luminosity of any pulsar and is highly active with regards to glitches. Analyses of its long-term and inter-glitch braking indices provided intriguing evidence that its spin-down energy budget may include gravitational-wave emission from a time-varying mass quadrupole moment. Its 62 Hz …

010504 meteorology & atmospheric sciencesAstronomyAstrophysicsEP/ T017325/101 natural sciencesrotationGeneral Relativity and Quantum CosmologyPSR J0537−6910neutron starsLuminosityGravitatational Waves PSR J0537−6910 LIGO VirgoHISTORYLIGOSupernova remnantneutron star010303 astronomy & astrophysicsgravitational waveQCQBpulsarPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/03N157BPhysics/dk/atira/pure/sustainabledevelopmentgoals/partnershipsGravitational waves neutron stars pulsarEPSRCPhysical Sciencesmoment: multipole[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Astrophysics - High Energy Astrophysical PhenomenaGravitational wavedata analysis methodPSR J0537-6910Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & AstrophysicsEphemeris1ST SEARCHGravitational wavesX-raySDG 17 - Partnerships for the GoalsPulsar0103 physical sciences/dk/atira/pure/subjectarea/asjc/1900/1912X-ray: emissiongravitational waves; pulsars; PSR J0537-6910; neutron starsSTFCAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesScience & TechnologyNeutron Star Interior Composition ExplorerR-MODEGravitational waveVirgopulsar: rotationRCUKAstronomy and AstrophysicsLIGONeutron starVIRGOSUPERNOVA REMNANTSpace and Planetary Sciencegravitational radiation: emissionpulsars/dk/atira/pure/subjectarea/asjc/3100/3103Gravitatational Waves[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Electroweak measurements in electron-positron collisions at W-boson-pair energies at LEP

2013

The ALEPH, DELPHI, L3, OPAL collaborations and LEP Electroweak Working Group.-- arXiv:1302.3415

Top quarkPARTICLE PHYSICS; LARGE ELECTRON POSITRON COLLIDER; ALEPH; DELPHI; L3; OPALElectron–positron annihilationPrecision measurements at W-pair energiesWW bosonGeneral Physics and AstronomyCOLOR DIPOLE MODEL01 natural sciences7. Clean energyZZ bosonMathematical SciencesHigh Energy Physics - Experimentelectroweak interactionsHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)electron-positron physics[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]FERMION-LOOP SCHEMEANOMALOUS MAGNETIC-MOMENTOF-MASS ENERGIES; TOP-QUARK MASS; CARLO EVENT GENERATOR; HADRONIC Z-DECAYS; INVARIANT YFS EXPONENTIATION; ANOMALOUS MAGNETIC-MOMENT; (UN)STABLE W+W-PRODUCTION; FERMION-LOOP SCHEME; COLOR DIPOLE MODEL; LEADING ORDER QCDeffective coupling constantsBosonPhysicsOPALPhysicsElectroweak interactionSettore FIS/01 - Fisica Sperimentalehep-phPrecision measurements at WW-pair energiesRadiative correctionsALEPHNuclear & Particles PhysicsLARGE ELECTRON POSITRON COLLIDER3. Good healthRadiative correctionHigh Energy Physics - PhenomenologyOF-MASS ENERGIESDecays of heavy intermediate gauge bosonsINVARIANT YFS EXPONENTIATIONPrecision measurements at W-pair energieFermion-antifermion productionL3Physical SciencesComputingMethodologies_DOCUMENTANDTEXTPROCESSINGPARTICLE PHYSICSFísica nuclearProduction (computer science)decays of heavy intermediate gauge bosons; neutral weak current; w boson; tests of the standard model; precision measurements at w-pair energies; fermion-antifermion production; top quark; electron-positron physics; electroweak interactions; effective coupling constants; higgs boson; z boson; radiative correctionsFermion–antifermion productionELECTROWEAK INTERACTIONTests of the Standard ModelParticle Physics - ExperimentParticle physicsZ bosonElectron-positron physicElectroweak interactionsLEADING ORDER QCDHiggs boson(UN)STABLE W+W-PRODUCTIONFOS: Physical sciencesdecays of heavy intermediate gauge bosonsddc:500.2Decays of heavy intermediate gauge bosonEffective coupling constantPartícules (Física nuclear)Standard ModelNuclear physicsPhysics and Astronomy (all)Neutral weak current0103 physical sciencesddc:530010306 general physicsTOP-QUARK MASSEffective coupling constantsDELPHIElectron–positron physicshep-ex010308 nuclear & particles physicsBranching fractionHigh Energy Physics::PhenomenologyCARLO EVENT GENERATORTop quarkradiative correctionsElectron-positron physics; Electroweak interactions; Decays of heavy intermediate gauge bosons; Fermion-antifermion production; Precision measurements at W-pair energies; Tests of the Standard Model; Radiative corrections; Effective coupling constants; Neutral weak current; Z boson; W boson; Top quark; Higgs bosonHADRONIC Z-DECAYSCol·lisions (Física nuclear)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Experimental High Energy PhysicsLarge Electron–Positron ColliderW bosonHigh Energy Physics::ExperimentElectron-positron physics
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Dealing with interruptions in text-based chat sessions

2010

Running a teaching session that achieves its aims and objectives requires organised and structured dialogue between teacher and students that leaves room for a clear line of instructions. However, participants can disrupt the flow and prevent the achievement of these objectives through constant interruption (via questions or comments). The interruptions mentioned here include any discursive interaction that halts the flow of the argument and causes distraction for teacher and students.

chat disruption interaction
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