Search results for "number"

showing 10 items of 3939 documents

On the existence of at least a solution for functional integral equations via measure of noncompactness

2017

In this article, we use fixed-point methods and measure of noncompactness theory to focus on the problem of establishing the existence of at least a solution for the following functional integral equation ¶ \[u(t)=g(t,u(t))+\int_{0}^{t}G(t,s,u(s))\,ds,\quad t\in{[0,+\infty[},\] in the space of all bounded and continuous real functions on $\mathbb{R}_{+}$ , under suitable assumptions on $g$ and $G$ . Also, we establish an extension of Darbo’s fixed-point theorem and discuss some consequences.

47H08Pure mathematicsBanach spaceAlgebra and Number Theory010102 general mathematicsMathematical analysisExtension (predicate logic)Space (mathematics)45N0501 natural sciencesMeasure (mathematics)Integral equation010101 applied mathematics54H25Settore MAT/05 - Analisi MatematicaBounded functionfunctional integral equationmeasure of noncompactnessSettore MAT/03 - Geometria0101 mathematicsAnalysisMathematicsBanach Journal of Mathematical Analysis
researchProduct

Wind accretion in the massive X-ray binary 4U 2206+54: abnormally slow wind and a moderately eccentric orbit

2006

Massive X-ray binaries are usually classified depending on the properties of the donor star in classical, supergiant and Be X-ray binaries. The massive X-ray binary 4U 2206+54 does not fit in any of these groups, and deserves a detailed study to understand how the transfer of matter and the accretion on to the compact object take place. To this end we study an IUE spectrum of the donor and obtain a wind terminal velocity (v_inf) of ~350 km/s, which is abnormally slow for its spectral type. We also analyse here more than 9 years of available RXTE/ASM data. We study the long-term X-ray variability of the source and find it to be similar to that observed in the wind-fed supergiant system Vela …

4U 2206+54X-ray binaryBinary numberFOS: Physical sciencesOutflows Emission-lineOrbital eccentricityAstrophysicsWindsCompact starUNESCO::ASTRONOMÍA Y ASTROFÍSICAVelaAstrophysicsIndividual starsPhysicsAstrophysics (astro-ph)BD +53◦2790BeAstronomy and AstrophysicsOrbital period:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Accretion (astrophysics)X-rays binariesX-rays individualsX-rays binaries ; X-rays individuals ; 4U 2206+54 ; Individual stars ; BD +53◦2790 ; Winds ; Outflows Emission-line ; BeSpace and Planetary ScienceUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaSupergiant:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
researchProduct

"Table 1" of "Measurement of the (anti-)$^{3}$He elliptic flow in Pb-Pb collisions at $\sqrt{s_{\rm{NN}}}$ = 5.02 TeV"

2020

Event-plane resolution $R_{\Psi_{2}}$ of the second harmonic as a function of the collision centrality.

5020.0PB PB --> 3HE XRESOLUTIONMathematics::Number TheoryMathematics::Classical Analysis and ODEsMathematics::Mathematical PhysicsR_Psi_2Mathematics::Spectral TheoryNuclear Experiment
researchProduct

Adaptive Number Knowledge in Secondary School Students: Profiles and Antecedents

2019

Cited By :1 Export Date: 10 February 2021 Correspondence Address: McMullen, J.; Department of Teacher EducationFinland; email: jake.mcmullen@utu.fi The present study aims to examine inter-individual differences in adaptive number knowledge in secondary school students. Adaptive number knowledge is defined as a well-connected network of knowledge of numerical characteristics and arithmetic relations. Substantial and relevant qualitative differences in the strategies and expression of adaptive number knowledge have been found in primary school students still in the process of learning arithmetic. We present a study involving 879 seventh-grade students that examines the structure of individual…

515 PsychologyProcess (engineering)yläkoululaisetlcsh:BF1-990Experimental and Cognitive Psychology050105 experimental psychologyFluencylatent profile analysisMathematics educationComputingMilieux_COMPUTERSANDEDUCATIONmatemaattiset taidot0501 psychology and cognitive sciencesAlgebra over a fieldAdaptive expertiseindividual differencesStructure (mathematical logic)Numerical Analysis4. EducationApplied Mathematicslcsh:Mathematics05 social sciences050301 educationMixture modeladaptive number knowledgelcsh:QA1-939Expression (mathematics)lcsh:PsychologyFormal instructionadaptive expertisenumeerinen lukutaitoarithmetic developmentPsychology0503 educationJournal of Numerical Cognition
researchProduct

Existence de points fixes enlacés à une orbite périodique d'un homéomorphisme du plan

1992

Let f be an orientation-preserving homeomorphism of the plane such that f-Id is contracting. Under these hypotheses, we establish the existence, for every periodic orbit, of a fixed point which has nonzero linking number with this periodic orbit.

55M20 54H20Surfaces homeomorphismsPlane (geometry)Applied MathematicsGeneral Mathematics010102 general mathematics[ MATH.MATH-DS ] Mathematics [math]/Dynamical Systems [math.DS][MATH.MATH-DS]Mathematics [math]/Dynamical Systems [math.DS]Linking numberFixed pointLinking numbers01 natural sciencesHomeomorphism010101 applied mathematicsCombinatoricssymbols.namesakesymbolsPeriodic orbitsPeriodic orbitsAstrophysics::Earth and Planetary AstrophysicsMathematics - Dynamical Systems0101 mathematicsMSC : 55M20 54H20Mathematics
researchProduct

Low-lying electric dipole gamma-continuum for the unstable Fe-62,64 nuclei : Strength evolution with neutron number

2020

6 pags., 4 figs.

62Nuclear and High Energy Physics64PhononAstrophysics::High Energy Astrophysical PhenomenaBinding energyNuclear TheoryCoulomb excitation[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]7. Clean energy01 natural sciences64Fe530Dipole excitation around neutron threshold62FeSubatomär fysik0103 physical sciencesSubatomic Physicsddc:530NeutronNuclear Physics - ExperimentNuclear structure010306 general physicsNuclear ExperimentPhysics010308 nuclear & particles physics62 Fe62; Fe; 64; Fe; Dipole excitation around neutron threshold; Nuclear structureNuclear structure64 FeFelcsh:QC1-999DipoleFe-64Neutron numberFe-62AGATAAtomic physicslcsh:Physics
researchProduct

Uncertainty quantification on a spatial Markov-chain model for the progression of skin cancer

2019

AbstractA spatial Markov-chain model is formulated for the progression of skin cancer. The model is based on the division of the computational domain into nodal points, that can be in a binary state: either in ‘cancer state’ or in ‘non-cancer state’. The model assigns probabilities for the non-reversible transition from ‘non-cancer’ state to the ‘cancer state’ that depend on the states of the neighbouring nodes. The likelihood of transition further depends on the life burden intensity of the UV-rays that the skin is exposed to. The probabilistic nature of the process and the uncertainty in the input data is assessed by the use of Monte Carlo simulations. A good fit between experiments on mi…

65C05Skin NeoplasmsComputer scienceQuantitative Biology::Tissues and OrgansMarkovin ketjut0206 medical engineeringMonte Carlo methodPhysics::Medical PhysicsBinary number02 engineering and technologyArticleihosyöpä03 medical and health sciencesMicemedicineAnimalsHumansComputer SimulationStatistical physicsUncertainty quantification60J20stokastiset prosessit030304 developmental biologyProbability0303 health sciencesMarkov chainApplied MathematicsProbabilistic logicUncertaintyState (functional analysis)medicine.disease020601 biomedical engineeringAgricultural and Biological Sciences (miscellaneous)Markov ChainsCardinal pointModeling and Simulation65C40Disease Progressionmatemaattiset mallitSkin cancerMonte Carlo MethodJournal of Mathematical Biology
researchProduct

"Table 6" of "Measurement of matter-antimatter differences in beauty baryon decays"

2017

Fig2b. The invariant mass distributions for $\Lambda^0_b\to \pi^- K^+ K^-$ decays. Uncertainties on the data points are statistical only and represent one standard deviations, calculated assuming Poisson-distributed entries.

8000.0Number of candidateNumber of candidatesP P --> LAMBDA/B0 X7000.0
researchProduct

"Table 5" of "Measurement of matter-antimatter differences in beauty baryon decays"

2017

Fig2a. The invariant mass distributions for $\Lambda^0_b\to p\pi^-\pi^+\pi^-$ decays. Uncertainties on the data points are statistical only and represent one standard deviations, calculated assuming Poisson-distributed entries.

8000.0Number of candidatesNumber of candidateP P --> LAMBDA/B0 X7000.0
researchProduct

"Table 2" of "Photon Events with Missing Energy at sqrt(s) = 183 to 189 GeV"

2003

Combined result.

9.150E+019.450E+01182.7E+ E- ScatteringExclusiveE+ E- --> NU NUBAR GAMMA (GAMMAS)NC=NUMBER OF NEUTRINOS
researchProduct