Search results for "Lamb"

showing 10 items of 745 documents

Hidden-charm pentaquark state inΛb0→J/ψpπ−decay

2016

We study here the ${\mathrm{\ensuremath{\Lambda}}}_{b}^{0}\ensuremath{\rightarrow}J/\ensuremath{\psi}p{\ensuremath{\pi}}^{\ensuremath{-}}$ reaction in analogy to the ${\mathrm{\ensuremath{\Lambda}}}_{b}^{0}\ensuremath{\rightarrow}J/\ensuremath{\psi}p{K}^{\ensuremath{-}}$ one, and we note that in both decays there is a sharp structure (dip or peak) in the $J/\ensuremath{\psi}p$ mass distribution around 4450 MeV, which is associated in the ${\mathrm{\ensuremath{\Lambda}}}_{b}^{0}\ensuremath{\rightarrow}J/\ensuremath{\psi}p{K}^{\ensuremath{-}}$ experiment to an exotic pentaquark baryonic state, although in ${\mathrm{\ensuremath{\Lambda}}}_{b}^{0}\ensuremath{\rightarrow}J/\ensuremath{\psi}p{\en…

BaryonPhysicsParticle physicsMeson010308 nuclear & particles physicsQuantum mechanicsPartial wave analysis0103 physical sciencesState (functional analysis)010306 general physicsLambda01 natural sciencesPentaquarkPhysical Review D
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Λb and Λc baryon decays at finite values of heavy quark masses

2000

Semileptonic decays of Lambda_b and Lambda_c baryons are studied within the Relativistic Three-Quark Model using finite heavy quark mass values. Employing the same parameters as have been used previously for the description of exclusive decays of heavy baryons in the heavy quark limit we calculate the six form factors of the process and the corresponding decay rates. Our calculation shows that the ``finite mass'' corrections are important in heavy-to-light transitions and are not negligible in heavy-to-heavy transitions.

BaryonPhysicsQuarkNuclear and High Energy PhysicsParticle physicsHigh Energy Physics::LatticeNuclear TheoryHigh Energy Physics::PhenomenologyHigh Energy Physics::ExperimentLimit (mathematics)Nuclear ExperimentLambdaPhysics Letters B
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Resonances in chiral unitary approaches

2008

The extension of chiral theories to the description of resonances, via the incorporation of unitarity in coupled channels, has provided us with a new theoretical perspective on the nature of some of the observed excited hadrons. In this contribution some of the early achievements in the field of baryonic resonances are reviewed, the recent evidence of the two-pole nature of the Lambda(1405) is discussed and results on charmed baryon resonances are presented.

BaryonPhysicsTheoretical physicsField (physics)UnitarityExcited stateHigh Energy Physics::PhenomenologyHadronNuclear ExperimentLambdaUnitary state
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Cosmic Dark Radiation and Neutrinos

2013

New measurements of the cosmic microwave background (CMB) by the Planck mission have greatly increased our knowledge about the universe. Dark radiation, a weakly interacting component of radiation, is one of the important ingredients in our cosmological model which is testable by Planck and other observational probes. At the moment, the possible existence of dark radiation is an unsolved question. For instance, the discrepancy between the value of the Hubble constant, H-0, inferred from the Planck data and local measurements of H-0 can to some extent be alleviated by enlarging the minimal ACDM model to include additional relativistic degrees of freedom. From a fundamental physics point of v…

Big BangNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Article SubjectAge of the universeDark matterFOS: Physical sciencesLambda-CDM modelAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesBayron acoustic-Oscillationssymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Analytic approach0103 physical sciencesPlanck010306 general physicsPhysicsAstrophysics - Cosmology and Extragalactic Astrophysics010308 nuclear & particles physicsHot dark matterFísicalcsh:QC1-999High Energy Physics - Phenomenology13. Climate actionDark radiationDark energysymbolslcsh:PhysicsAstrophysics - Cosmology and Nongalactic AstrophysicsAdvances in High Energy Physics
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Uncertainty on w from large-scale structure

2012

We find that if we live at the center of an inhomogeneity with total density contrast of roughly 0.1, dark energy is not a cosmological constant at 95% confidence level. Observational constraints on the equation of state of dark energy, w, depend strongly on the local matter density around the observer. We model the local inhomogeneity with an exact spherically symmetric solution which features a pressureless matter component and a dark-energy fluid with constant equation of state and negligible sound speed, that reaches a homogeneous solution at finite radius. We fit this model to observations of the local expansion rate, distant supernovae and the cosmic microwave background. We conclude …

Big BangPhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)ta114010308 nuclear & particles physicsEquation of state (cosmology)Scalar field dark matterFOS: Physical sciencesAstronomy and AstrophysicsLambda-CDM modelGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyComputational physicsThermodynamics of the universeSpace and Planetary ScienceQuantum mechanics0103 physical sciencesDark energy010303 astronomy & astrophysicsDark fluidAstrophysics - Cosmology and Nongalactic Astrophysics
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Genetic analysis of early lamb survival in extensively reared lambs

2005

In sheep production, lamb survival is an important economic trait (Conington et al., 2004). Therefore, this trait has been studied by many scientists, especially in countries with an extensive husbandry system. In the United Kingdom, the number of lambs dying before weaning has been estimated ranging from 5 to 40% (Eales et al., 1983).

Binary traitLive weightlive weightBiologyAnimal husbandryGenetic analysisbinary traitlamb survival binary trait genetic parameters live weightlamb survivalAnimal scienceSHEEPgenetic parametersTraitWeaningAnimal Science and Zoologylcsh:Animal culturelcsh:SF1-1100
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CODEX Weak Lensing Mass Catalogue and implications on the mass-richness relation

2021

The COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the largest flux limited sample of X-ray clusters at $0.35 = \alpha \mu + \beta$, with $\mu = \ln (M_{200c}/M_{\mathrm{piv}})$, and $M_{\mathrm{piv}} = 10^{14.81} M_{\odot}$. We find a slope $\alpha = 0.49^{+0.20}_{-0.15}$, normalization $ \exp(\beta) = 84.0^{+9.2}_{-14.8}$ and $\sigma_{\ln \lambda | \mu} = 0.17^{+0.13}_{-0.09}$ using CFHT richness estimates. In comparison to other weak lensing richness-mass relations, we find the normalization of the richness statistically agreeing with the normalization of other scaling relations from a broad redshift range ($0.0<z<0.65$) and with different cluster selection (X-ray, Sun…

COSMOLOGICAL CONSTRAINTSCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsLambdaPROFILE01 natural sciences114 Physical sciencesgravitational lensing: weakMAXBCGweak [gravitational lensing]0103 physical sciencesLARGE-SCALE STRUCTUREclusters: general [galaxies]PROBE010303 astronomy & astrophysicsWeak gravitational lensingGalaxy clusterLOCUSSPhysicsTEMPERATURE RELATION010308 nuclear & particles physicsAstronomy and Astrophysicsobservations [cosmology]RedshiftREDUCTIONSpace and Planetary Sciencegravitational lensing: weak; galaxies: clusters: general; cosmology: observationsgalaxies: clusters: generalcosmology: observationsGIANTSGALAXY CLUSTERS[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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A new assay for O6-alkylguanine-DNA-alkyltransferase to determine DNA repair capacities using lambda-phage DNA as substrate.

1990

One O6-methylguanine (O6-meG) was introduced into each BamHI site of lambda-phage DNA as a substrate for the determination of the DNA repair protein O6-alkylguanine-DNA-alkyltransferase. A new assay using as the detection group 32P-labeled phosphate introduced at the 3' position of the modified nucleoside by incorporation of 32P-labeled TTP in the 3'-neighboring position proved highly sensitive: 10(-16) mol of the DNA lesion was still easily detectable. This DNA, which has greater than 1000 bp represents a good model for cellular DNA and was used as a substrate to measure the individual repair capacities for O6-meG in human lymphocytes of 20 healthy male and female donors. There were great …

Cancer ResearchGuanineDNA RepairDNA repairMolecular Sequence DataBiologySubstrate Specificitychemistry.chemical_compoundO(6)-Methylguanine-DNA MethyltransferaseDNA Repair ProteinEscherichia coliHumansLymphocyteschemistry.chemical_classificationBase SequenceSubstrate (chemistry)General MedicineMethyltransferasesLambda phagebiology.organism_classificationBacteriophage lambdaIn vitroKineticsEnzymeBiochemistrychemistryDNA ViralBamHIDNACarcinogenesis
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Una ética de la excelencia: Cayetana de la Cerda y la circulación de Madame de Lambert en España

2015

En este artículo se sintetizan las líneas maestras del pensamiento de Anne-Thérèse Marguenat, marquesa de Lambert (1647-1733) y se profundiza en el eco que su obra tuvo en España, aclarando algunos episodios poco conocidos y arrojando luz sobre el contexto en el que se realizó y publicó finalmente la versión castellana de sus ensayos y sobre la personalidad intelectual y circunstancias sociales de su traductora, Cayetana de la Cerda y Vera, condesa de Lalaing (1755-1798). Se pretende así analizar las prácticas de transferencia y mediación cultural, interrogándonos sobre los significados con que su pensamiento y su figura pudieron ser investidos por parte de los sujetos implicados en su lect…

Cayetana de la Cerdapensamiento aristocráticolcsh:History (General) and history of Europefilosofíatransferencia culturalética de la excelenciadistinción socialescritura femenina.lcsh:DÈticalcsh:D204-475condesa de LalaingMme. de Lambertcultura cortesanatraducciónlcsh:Modern history 1453-
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Search for the decayB¯0→Λc+p¯pp¯

2014

We report a search for the decay B^0 → Λ^+_cppp. Using a data sample of 471×10^6 BB pairs collected with the BABAR detector at the PEP-II2 storage ring at SLAC, we find no events and set an upper limit on the branching fraction B(B^0 → Λ^+_cppp)×^(B(Λ^+_c→pK^−π^+))_(0.050) <2.8×10^(−6) at 90% C.L., where we have normalized B(Λ^+_c → pK^−π^+) to the world average value.

Charmed baryonsPhysicsNuclear physicsNuclear and High Energy PhysicsBranching fractionElectron–positron annihilationAnalytical chemistryLambdaBar (unit)Physical Review D
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