Search results for "EXPANSION"

showing 10 items of 630 documents

Muscleblind isoforms are functionally distinct and regulate α-actinin splicing

2007

Drosophila Muscleblind (Mbl) proteins control terminal muscle and neural differentiation, but their molecular function has not been experimentally addressed. Such an analysis is relevant as the human Muscleblind-like homologs (MBNL1-3) are implicated in the pathogenesis of the inherited muscular developmental and degenerative disease myotonic dystrophy. The Drosophila muscleblind gene expresses four protein coding splice forms (mblA to mblD) that are differentially expressed during the Drosophila life cycle, and which vary markedly in their ability to rescue the embryonic lethal phenotype of muscleblind mutant flies. Analysis of muscleblind mutant embryos reveals misregulated alternative sp…

Gene isoformCancer ResearchMolecular Sequence DataBiologyKidneyChlorocebus aethiopsAnimalsDrosophila ProteinsHumansProtein IsoformsActininMuscle Skeletal3' Untranslated RegionsMolecular BiologyGeneCells CulturedCell NucleusGeneticsBase SequenceAlternative splicingGene Expression Regulation DevelopmentalNuclear ProteinsRNA-Binding ProteinsRNAKidney metabolismCell BiologyAlternative SplicingDrosophila melanogasterCOS CellsMutationRNA splicingTrinucleotide Repeat ExpansionTrinucleotide repeat expansionDevelopmental BiologyMinigeneDifferentiation
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Phase Transitions of BiVO4 under High Pressure and High Temperature

2022

We have studied the occurrence of phase transitions in two polymorphs of BiVO4 under high-pressure and high-temperature conditions by means of X-ray diffraction measurements. The fergusonite polymorph undergoes a phase transition at 1.5(1) GPa and room temperature into a tetragonal scheelite-type structure. The same transition takes place at 523(1) K and ambient pressure. A second phase transition takes place at room temperature under compression at 16(1) GPa. The transition is from the tetragonal scheelite structure to a monoclinic structure (space group P21/c). All observed phase transitions are reversible. The zircon polymorph counterpart also transforms under compression into the scheel…

General Energychemical structurecompressibilitydiffractionPhysical and Theoretical ChemistryUNESCO::CIENCIAS TECNOLÓGICASSurfaces Coatings and FilmsElectronic Optical and Magnetic Materialsphase transitionsthermal expansion
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Bochner-Riesz means of functions in weak-L p

1993

The Bochner-Riesz means of order delta greater-than-or-equal-to 0 for suitable test functions on R(N) are defined via the Fourier transform by (S(R)(delta)f)(xi) = (1 - \xi\2/R2)+(delta)f(xi). We show that the means of the critical index delta = N/P - N + 1/2, 1 + infinity, to f(x) in norm and for almost every x in R(N). We also observe that the means of the function absolute value of x-N/p, which belongs to L(p,infinity) (R(N)) but not to the closure of test functions, converge for no x

General MathematicsMathematical analysisFourier-Hankel expansionweak-$L\sp p$test functionBochner-Riesz meanradial functionCombinatoricssymbols.namesakeFourier transformLorentz spacesNorm (mathematics)Fourier transformsymbolsCritical indexFourier-Bessel expansionMAT/05 - ANALISI MATEMATICAMathematicsMonatshefte f�r Mathematik
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Violation of the equivalence principle from light scalar dark matter

2018

In this paper, we study the local observational consequences of a violation of the Einstein Equivalence Principle induced by models of light scalar Dark Matter (DM). We focus on two different models where the scalar field couples linearly or quadratically to the standard model of matter fields. For both these cases, we derive the solutions of the scalar field. We also derive from first principles the expressions for two types of observables: (i) the local comparison of two atomic sensors that are differently sensitive to the constants of Nature and (ii) the local differential acceleration between two test-masses with different compositions. For the linear coupling, we recover that the signa…

General relativityAtomic Physics (physics.atom-ph)Dark matteralternative theories of gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)local position invariance01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics - Atomic Physicsspace-time: oscillationdark matter: couplingGravitationTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)Gravitational field0103 physical sciencesDark Matteruniversalityequivalence principle: violationdark matter: scalarEquivalence principle010306 general physicsmodified gravityPhysics010308 nuclear & particles physicsScalar (physics)Yukawa potentialtorsioncoupling: linearuniversality of free fall[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]field theory: scalarHigh Energy Physics - Phenomenologypotential: YukawaGeneral relativitytests of gravitygravitation[SDU]Sciences of the Universe [physics][PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph][PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]expansion: accelerationScalar field
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Isolation and characterization of 10 highly polymorphic di- and trinucleotide microsatellite markers in the mayfly Ameletus inopinatus (Ephemeroptera…

2008

We describe the isolation of ten polymorphic microsatellite loci from the mayfly Ameletus inopinatus. Loci had di- or trinucleotide repeat motifs and were highly variable with three to 17 alleles (mean = 7.15). Observed heterozygosity ranged from 0.143 to 0.905. One locus (Ami_202) showed significant deviation from Hardy–Weinberg equilibrium in one population, but no evidence for null alleles. One locus (Ami_73) was significantly linked with three other loci. The remaining nine loci should prove highly informative for population genetic studies.

Geneticseducation.field_of_studyPopulationLocus (genetics)Biologybiology.organism_classificationNull alleleLoss of heterozygosityMayflyGeneticsMicrosatelliteeducationTrinucleotide repeat expansionMicrosatellite enrichmentEcology Evolution Behavior and SystematicsBiotechnologyMolecular ecology resources
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Why Magnus expansion

2021

A short story about the origins of Magnus Expansion, why we got involved and how it led us to meet Geometric Integration. We present a biographical draft of Wilhelm Magnus, a sketchy discussion of ...

Geometric integrationComputational Theory and MathematicsApplied MathematicsMagnus expansionCalculusComputer Science ApplicationsMathematicsInternational Journal of Computer Mathematics
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1.6 GHz VLBI observations of SN 1979C: almost-free expansion

2009

We report on 1.6 GHz Very-Long-Baseline-Interferometry (VLBI) observations of supernova SN 1979C made on 18 November 2002. We derive a model-dependent supernova size. We also present a reanalysis of VLBI observations made by us on June 1999 and by other authors on February 2005. We conclude that, contrary to our earlier claim of strong deceleration in the expansion, SN 1979C has been undergoing almost-free expansion ($m = 0.91\pm0.09$; $R \propto t^m$) for over 25 years.

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Continuum (measurement)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsSupernovaSpace and Planetary ScienceVery-long-baseline interferometryFree expansionBasso continuoAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Cosmology and Nongalactic AstrophysicsAstronomy & Astrophysics
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Spontaneous Scalarization of Charged Black Holes

2018

Extended scalar-tensor-Gauss-Bonnet (eSTGB) gravity has been recently argued to exhibit spontaneous scalarisation of vacuum black holes (BHs). A similar phenomenon can be expected in a larger class of models, which includes e.g. Einstein-Maxwell-scalar (EMS) models, where spontaneous scalarisation of electrovacuum BHs should occur. EMS models have no higher curvature corrections, a technical simplification over eSTGB models that allows us to investigate, fully non-linearly, BH scalarisation in two novel directions. Firstly, numerical simulations in spherical symmetry show, dynamically, that Reissner-Nordstr\"om (RN) BHs evolve into a perturbatively stable scalarised BH. Secondly, we compute…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsHigh Energy Physics - Theory010308 nuclear & particles physicsHorizonScalar (mathematics)FOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Curvature01 natural sciencesStability (probability)General Relativity and Quantum CosmologyGravitationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)0103 physical sciencesIsometryCircular symmetry010306 general physicsMultipole expansionAstrophysics - High Energy Astrophysical PhenomenaMathematical physicsPhysical Review Letters
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Hadron structure in tau -> KK pi nu_tau decays

2009

We analyze the hadronization structure of both vector and axial-vector currents leading to tau -> KK pi nu(tau) decays. At leading order in the 1/N-C expansion, and considering only the contribution of the lightest resonances, we work out, within the framework of the resonance chiral Lagrangian, the structure of the local vertices involved in those processes. The couplings in the resonance theory are constrained by imposing the asymptotic behavior of vector and axial-vector spectral functions ruled by QCD. In this way we predict the hadron spectra and conclude that, contrary to previous assertions, the vector contribution dominates by far over the axial-vector one in all KK pi charge channe…

High Energy Physics - PhenomenologyHadron tau decays[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]High Energy Physics::Phenomenology[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Física1/N ExpansionHigh Energy Physics::ExperimentChiral lagrangiansQCDHigh Energy Physics - Experiment
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tau -> pi pi pi nu(tau) decays and the a(1)(1260) off-shell width revisited

2009

The tau -> pi pi pi nu(tau) decay is driven by the hadronization of the axial-vector current. Within the resonance chiral theory, and considering the large-N-C expansion, this process has been studied in Ref. [1] (D. Gomez Dumm, A. Pich, J. Portoles, 2004). In the light of later developments we revise here this previous work by including a new off-shell width for the lightest a(1) resonance that provides a good description of the tau -> pi pi pi nu(tau) spectrum and branching ratio. We also consider the role of the rho(1450) resonance in these observables. Thus we bring in an overall description of the tau -> pi pi pi nu(tau) process in excellent agreement with our present experimental know…

High Energy Physics - Phenomenology[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]Hadron tau decays[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Física1/N ExpansionHigh Energy Physics::ExperimentChiral lagrangiansQCDHigh Energy Physics - Experiment
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