Search results for "MINOS"

showing 10 items of 739 documents

Compatibility of Rhizobial Genotypes within Natural Populations of Rhizobium leguminosarum Biovar viciae for Nodulation of Host Legumes

2003

ABSTRACT Populations of Rhizobium leguminosarum biovar viciae were sampled from two bulk soils, rhizosphere, and nodules of host legumes, fava bean ( Vicia faba ) and pea ( Pisum sativum ) grown in the same soils. Additional populations nodulating peas, fava beans, and vetches ( Vicia sativa ) grown in other soils and fava bean-nodulating strains from various geographic sites were also analyzed. The rhizobia were characterized by repetitive extragenomic palindromic-PCR fingerprinting and/or PCR-restriction fragment length polymorphism (RFLP) of 16S-23S ribosomal DNA intergenic spacers as markers of the genomic background and PCR-RFLP of a nodulation gene region, nodD , as a marker of the sy…

GenotypeBulk soilBiologymedicine.disease_causeApplied Microbiology and BiotechnologyPlant RootsPolymerase Chain ReactionRhizobium leguminosarumRhizobiaPlant MicrobiologySymbiosisBacterial ProteinsNitrogen FixationBotanyGenotypemedicineSymbiosisSoil Microbiology[SDV.EE]Life Sciences [q-bio]/Ecology environmentRhizosphereRhizobium leguminosarumEcologyPeasfood and beveragesbiology.organism_classificationDNA FingerprintingVicia fabaVicia faba[SDV.EE] Life Sciences [q-bio]/Ecology environmentNitrogen fixationFood ScienceBiotechnologyPlasmids
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Ni-containing spinel aluminates glass-ceramic materials obtained from cordieritic bulk glasses

2003

Monolithic glasses with compositions 2MO � 2Al2O3 � 5SiO2, being M ¼ Ni and equimolar mixtures of Ni and Mg, were prepared at 1650 C by melting mixtures of raw materials. The crystallization of monoliths was produced by heattreatment at several temperatures up to 1200 C. The crystallization sequence was followed by differential thermal analysis (DTA), X-ray powder diffraction (XRD), field emission scanning electron microscopy (FESEM) and energy dispersive X-ray (EDX) and diffuse reflectance spectroscopies. Surprisingly, the only crystalline phase formed after heating up to 1100 C was a nickel-containing aluminate spinel for both compositions. The microstructural characterization indicated t…

Glass-ceramicMaterials scienceAluminateSpinelAnalytical chemistryMineralogyThermal treatmentengineering.materialCondensed Matter PhysicsElectronic Optical and Magnetic Materialslaw.inventionchemistry.chemical_compoundchemistryAluminosilicatelawDifferential thermal analysisMaterials ChemistryCeramics and CompositesengineeringCrystallizationPowder diffractionJournal of Non-Crystalline Solids
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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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Search for high-mass resonances decaying to dimuons at CDF.

2009

We present a search for high-mass neutral resonances using dimuon data corresponding to an integrated luminosity of 2.3 fb(-1) collected in pp collisions at s=1.96 TeV by the CDF II detector at the Fermilab Tevatron. No significant excess above the standard model expectation is observed in the dimuon invariant-mass spectrum. We set 95% confidence level upper limits on sigma BR(pp -> X ->mu mu), where X is a boson with spin-0, 1, or 2. Using these cross section limits, we determine lower mass limits on sneutrinos in R-parity-violating supersymmetric models, Z(') bosons, and Kaluza-Klein gravitons in the Randall-Sundrum model.

HIGH MASS RESONANCEParticle physicsFermilab TevatronTevatronGeneral Physics and AstronomyFOS: Physical sciencesddc:500.2114 Physical sciencesResonance7. Clean energy01 natural sciencesHigh Energy Physics - ExperimentNuclear physicsTellurium compoundsHigh Energy Physics - Experiment (hep-ex)Integrated luminosities0103 physical sciences[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Fermilab010306 general physicsBosonsBosonPhysicsMuonMass spectrometryhep-ex010308 nuclear & particles physicsPhysicsInvariant-mass spectrum13.85.Rm 13.85.Qk 12.60.Cn 14.70.Pw 04.50.-hHigh Energy Physics::PhenomenologyConfidence levelsGravitonSupersymmetryUpper limitsSupersymmetric modelsCross sectionsRandall–Sundrum modelThe standard modelsMass spectrumCDFHigh Energy Physics::ExperimentPhysical review letters
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Searching for long-lived particles beyond the Standard Model at the Large Hadron Collider

2020

Particles beyond the Standard Model (SM) can generically have lifetimes that are long compared to SM particles at the weak scale. When produced at experiments such as the Large Hadron Collider (LHC) at CERN, these longlived particles (LLPs) can decay far from the interaction vertex of the primary proton–proton collision. Such LLP signatures are distinct from those of promptly decaying particles that are targeted by the majority of searches for new physics at the LHC, often requiring customized techniques to identify, for example, significantly displaced decay vertices, tracks with atypical properties, and short track segments. Given their non-standard nature, a comprehensive overview of LLP…

HIGH-ENERGYbeyond the Standard Modellarge hadron colliderPhysics::Instrumentation and DetectorsPROTON-PROTON COLLISIONSPhysics beyond the Standard Modelbeyond the standard model01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)high-luminosity lhcHigh Energy Physics - Phenomenology (hep-ph)MAGNETIC MONOPOLESlong-lived [particle]high-energy collider experimentsdecay: vertexscattering [p p][PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]long-lived particlesQCproposed [detector]Physicslifetimedark gauge forcesLarge Hadron ColliderCMSROOT-S=13 TEVroot-s=13 tevPhysicsnew physics: search forscale: electroweak interactionhep-phATLASelectroweak interaction [scale]vertex [decay]upgrade [detector]High Energy Physics - Experiment; High Energy Physics - Experiment; High Energy Physics - Phenomenologydetector: upgradeSettore FIS/02 - Fisica Teorica Modelli e Metodi Matematiciprimary [vertex]ddc:High Energy Physics - PhenomenologyCERN LHC CollLarge Hadron Colliderbaryon asymmetryvertex: primaryLHCcolliding beams [p p]exclusion limitspp collisionsParticle Physics - ExperimentsignatureNuclear and High Energy PhysicsParticle physicsp p: scatteringCERN LabPAIR PRODUCTIONcollider phenomenologyreviewFOS: Physical sciencesDARK GAUGE FORCES530search for [new physics]BARYON ASYMMETRY0103 physical sciencesddc:530010306 general physicsnumerical calculationsParticle Physics - PhenomenologyEXCLUSION LIMITSmagnetic monopolesPP COLLISIONS010308 nuclear & particles physicshep-exbackgroundbibliographyshowersMAJORANA NEUTRINOSCollisiontracksLHC-Bdetector: proposedhigh-luminosity LHCpair productionMATHUSLAPhysics and Astronomy[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]proton-proton collisionshigh-energymajorana neutrinosparticle: long-livedp p: colliding beamsPhysics BSMexperimental results
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Precision measurement of D meson mass differences

2013

Using three- and four-body decays of D mesons produced in semileptonic b-hadron decays, precision measurements of D meson mass differences are made together with a measurement of the D-0 mass. The measurements are based on a dataset corresponding to an integrated luminosity of 1.0 fb(-1) collected in pp collisions at 7 TeV. Using the decay D-0 -> K+K-K-pi(+), the D-0 mass is measured to be M(D-0) = 1864.75 +/- 0.15 (stat) +/- 0.11 (syst) MeV/c(2). The mass differences M(D+) - M(D-0) = 4.76 +/- 0.12 (stat) +/- 0.07 (syst) MeV/c(2), M(D-s(+)) - M(D+) = 98.68 +/- 0.03 (stat) +/- 0.04 (syst) MeV/c(2) are measured using the D-0 -> K+K-pi(+)pi(-) and D-(s)(+) -> K+K-pi(+) modes.

Hadronic decays of charmed mesonsParticle physicsTeoria quàntica de campsGravitacióNuclear and High Energy PhysicsMesonHigh Energy Physics::LatticeNuclear TheoryFOS: Physical sciencesHadrons01 natural sciencesHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadrons; Leptonic semileptonic and radiative decays of bottom mesons; Charmed mesons (|C|>0 B=0); Hadronic decays of charmed mesonsPartícules (Física nuclear)Settore FIS/04 - Fisica Nucleare e SubnucleareLuminosityHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)0103 physical sciencesD mesonLeptonic semileptonic and radiative decays of bottom meson[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]TOOLTeoria quàntica010306 general physicsHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadronsNuclear ExperimentQCHadron-Hadron Scattering; Nuclear and High Energy PhysicsPhysicsHadron-Hadron Scattering010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyHadron-induced high- and super-high-energy interactions (energy > 10 GeV): Inclusive production with identified hadronRelativity (Physics)DecayRelativitat (Física)Quantum field theoryFIS/01 - FISICA SPERIMENTALEQuantum theoryLeptonic semileptonic and radiative decays of bottom mesonsDECAY; TOOLFísica nuclearHigh Energy Physics::ExperimentCharmed mesons (|C|>0 B=0)DECAYParticle Physics - ExperimentGravitationJournal of High Energy Physics
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Stereoselective Access to Fluorinated and Non-fluorinated Quaternary Piperidines: Synthesis of Pipecolic Acid and Iminosugar Derivatives

2012

The preparation of optically pure quaternary piperidines, both fluorinated and non-fluorinated, has been achieved from a chiral imino lactone derived from (R)-phenylglycinol. In the case of the fluorinated derivatives, the addition of (trifluoromethyl)trimethylsilane (TMSCF(3)) followed by iodoamination and migration of the CF(3) group allowed access to four derivatives of α-(trifluoromethyl)pipecolic acid. A theoretical study of the CF(3)-group rearrangement has been carried out to help establish the reaction mechanism of this uncommon transformation. Moreover, a route to trifluoromethyl-substituted iminosugars was also developed through the diastereoselective dihydroxylation of suitable s…

HalogenationStereochemistryIminosugarAlkylationCatalysischemistry.chemical_compoundPiperidinesfluorineiminosugarsPipecolic acidchemistry.chemical_classificationamino acidsTrifluoromethylMolecular StructureChemistryOrganic ChemistryHalogenationStereoisomerismGeneral ChemistryImino SugarsDihydroxylationPipecolic Acidsdensity functional calculationsquaternary stereocentersStereoselectivityLactone
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Measurement of hard double-parton interactions inW(???) + 2-jet events at $\sqrt{s}\,=7$ TeV with the ATLAS detector

2013

The production of W bosons in association with two jets in proton–proton collisions at a centre-of-mass energy of √s=7 TeV has been analysed for the presence of double-parton interactions using data corresponding to an integrated luminosity of 36 pb[superscript −1], collected with the ATLAS detector at the Large Hadron Collider. The fraction of events arising from double-parton interactions, f[superscript (D) over subscript DP], has been measured through the p[subscript T] balance between the two jets and amounts to f[superscript (D) over subscript DP] = 0.08 ± 0.01 (stat.) ± 0.02 (sys.) for jets with transverse momentum p[subscript T] > 20 GeV and rapidity |y| < 2.8. This corresponds to a …

Hard-partonCiencias FísicasGeneral Physics and AstronomyParton7. Clean energy01 natural sciencesHigh Energy Physics - Experimentlaw.inventionVector bosonScattering//purl.org/becyt/ford/1 [https]law[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]w bosonNuclear ExperimentQCBosonddc:539PhysicsLuminosity (scattering theory)Large Hadron ColliderSettore FIS/01 - Fisica SperimentaleATLAShard double-parton interactions; ATLAS detectorProbemedicine.anatomical_structureHadronic CollisionsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGLHCCIENCIAS NATURALES Y EXACTASParticle Physics - ExperimentParticle physicsMultiparton InteractionsCiências Naturais::Ciências Físicas530 PhysicsAstrophysics::High Energy Astrophysical Phenomena:Ciências Físicas [Ciências Naturais]ddc:500.25304-Jet EventsNuclear physicsAtlas (anatomy)0103 physical sciencesmedicineddc:530RapidityHigh Energy Physics010306 general physicsColliderCiencias ExactasCalorimeterScience & TechnologyATLAS detector010308 nuclear & particles physicsMeasurementsHigh Energy Physics::PhenomenologyFísica//purl.org/becyt/ford/1.3 [https]QCDAstronomíaHADRON-HADRON COLLISIONSExperimental High Energy Physicsproton-proton collisionsHigh Energy Physics::ExperimentCollider
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VLTI/AMBER spectro-interferometry of the late-type supergiants V766 Cen (=HR 5171 A), σ Oph, BM Sco, and HD 206859

2017

Aims. We add four warmer late-type supergiants to our previous spectro-interferometric studies of red giants and supergiants. Methods. We measure the near-continuum angular diameter, derive fundamental parameters, discuss the evolutionary stage, and study extended atmospheric atomic and molecular layers. Results. V766 Cen (=HR 5171 A) is found to be a high-luminosity (log L/L = 5.8 ± 0.4) source of effective temperature 4290 ± 760 K and radius 1490 ± 540 R, located in the Hertzsprung-Russell (HR) diagram close to both the Hayashi limit and Eddington limit; this source is consistent with a 40 M evolutionary track without rotation and current mass 27-36 M. V766 Cen exhibits Na i in emission a…

Hertzsprung–Russell diagramindividual: BM Sco [Stars]FOS: Physical sciencesAstrophysics01 natural sciencesLuminositysymbols.namesake0103 physical sciencesStars: individual: BM ScoRed supergiantStars: mass-lossYellow hypergiantatmospheres [Stars]010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Physicsmass-loss [Stars]010308 nuclear & particles physicsAstronomy and AstrophysicsEffective temperatureStars: individual: V766 CenAstrophysics - Solar and Stellar AstrophysicsSupergiantsSpace and Planetary ScienceEddington luminosityTechniques: interferometricsymbolsCircumstellar dustinterferometric [Techniques]individual: V766 Cen [Stars]Stars: atmospheresSupergiant
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Millimeter-VLBI observations of low-luminosity active galactic nuclei with source-frequency phase-referencing

2021

We report millimeter-VLBI results of low-luminosity active galactic nuclei (M 84 and M 87) up to 88 GHz with source-frequency phase-referencing observations. We detected the weak VLBI core and obtained the first image of M 84 at 88 GHz. The derived brightness temperature of M 84 core was about 7.2$\times$10$^9$ K, which could serve as a lower limit as the core down to 30 Schwarzschild radii was still un-resolved in our 88 GHz observations. We successfully determined the core-shifts of M 87 at 22-44 GHz and 44-88 GHz through source-frequency phase-referencing technique. The jet apex of M 87 could be deduced at about 46 $\mu$as upstream of the 43 GHz core from core-shift measurements. The est…

High Energy Astrophysical Phenomena (astro-ph.HE)Event Horizon TelescopePhysicsAstrofísicaActive galactic nucleusEvent horizonFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics - Astrophysics of GalaxiesLuminositySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Brightness temperatureVery-long-baseline interferometryMagnitude (astronomy)AstronomiaMillimeterAstrophysics - High Energy Astrophysical Phenomena
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