Search results for "Theoretical models"

showing 10 items of 79 documents

Cold fusion of heavy ions paving the way to superheavy elements

2001

Abstract Significant progress has been made approaching superheavy elements. A shell-stabilized region near hassium has been discovered. Element 112 has been synthesized. Recently evidence for the creation of elements 114, 116, and 118 has been reported. The way to these superheavy nuclei was paved by the cold fusion of heavy ions. In this paper experimental methods for heavy-element research, which is essentially physics with single atoms, are presented together with recent experimental results. The observed nuclear properties are discussed in the framework of theoretical models. New instrumental developments including accelerators and radioactive beams are be addressed.

Nuclear physicsPhysicsNuclear and High Energy PhysicschemistryTheoretical modelschemistry.chemical_elementSuperheavy ElementsAtomic physicsExperimental methodsHassiumCold fusionIonNuclear Physics A
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Experimental realization of a new type of crystalline undulator.

2014

A new scheme of making crystalline undulators was recently proposed and investigated theoretically by Andriy Kostyuk, concluding that a new type of crystalline undulator would be not only viable, but better than the previous scheme. This article describes the first experimental measurement of such a crystalline undulator, produced by using Si(1-x)Ge(x)-graded composition and measured at the Mainzer Microtron facility at beam energies of 600 and 855 MeV. We also present theoretical models developed to compare with the experimental data.

OpticsMaterials sciencebusiness.industryTheoretical modelsGeneral Physics and AstronomyType (model theory)UndulatorbusinessMicrotronRealization (systems)Beam (structure)Physical review letters
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Bet-hedging in diapausing egg hatching of temporary rotifer populations - A review of models and new insights

2014

Habitat unpredictability is a local adaptation factor shaping life-history traits in rotifer populations. It may select for the evolution of bet-hedging through risk-spreading strategies in diapausing egg hatching. This means that a fraction of diapausing eggs in wild populations do not hatch even when the conditions are favorable for population growth. Thus, there is a remaining fraction of viable diapausing eggs standing in the sediments for longer periods. According to theory, it is expected that the incidence of bet-hedging strategies for diapausing egg hatching will be higher in more uncertain habitats. Here, we review the major predictions derived from theoretical models applied to th…

Phenotypic plasticityHatchingEcologyTheoretical modelsRotiferAquatic ScienceBiologybiology.organism_classificationHabitatembryonic structuresGenetic variationPredictabilityEcology Evolution Behavior and SystematicsLocal adaptationInternational Review of Hydrobiology
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Numerical Simulations of Jets from Active Galactic Nuclei

2019

Numerical simulations have been playing a crucial role in the understanding of jets from active galactic nuclei (AGN) since the advent of the first theoretical models for the inflation of giant double radio galaxies by continuous injection in the late 1970s. In the almost four decades of numerical jet research, the complexity and physical detail of simulations, based mainly on a hydrodynamical/magneto-hydrodynamical description of the jet plasma, have been increasing with the pace of the advance in theoretical models, computational tools and numerical methods. The present review summarizes the status of the numerical simulations of jets from AGNs, from the formation region in the neighborho…

PhysicsActive galactic nucleus010308 nuclear & particles physicsRadio galaxyplasma physicslcsh:AstronomyNumerical analysisAstrophysics::High Energy Astrophysical PhenomenaTheoretical modelsAstronomy and AstrophysicsAstrophysicsPlasmaAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslcsh:QB1-991Astrophysical jetmagneto-hydrodynamics0103 physical sciencesactive galactic nucleinumerical methodsMagnetohydrodynamics010303 astronomy & astrophysicsPhenomenology (particle physics)Astrophysics::Galaxy Astrophysicsrelativistic jetsGalaxies
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Measurement of the Absolute Branching Fraction forΛc+→Λe+νe

2015

We report the first measurement of the absolute branching fraction for Lambda(+)(c) -> Lambda e(+)nu(e). This measurement is based on 567 pb(-1) of e(+)e(-) annihilation data produced at root s = 4.599 GeV, which is just above the Lambda(+)(c)Lambda(-)(c) threshold. The data were collected with the BESIII detector at the BEPCII storage rings. The branching fraction is determined to be B(Lambda(+)(c) -> Lambda e(+)nu(e)) = [3.63 +/- 0.38(stat) +/- 0.20(syst)] %, representing a significant improvement in precision over the current indirect determination. As the branching fraction for Lambda(+)(c) -> Lambda e(+)nu(e) is the benchmark for those of other Lambda(+)(c) semileptonic channels, our r…

PhysicsAnnihilation010308 nuclear & particles physicsBranching fractionElectron–positron annihilationTheoretical modelsAnalytical chemistryGeneral Physics and AstronomyLambda baryonLambda01 natural sciencesNuclear physicsBaryonCharmed baryons0103 physical sciencesHigh Energy Physics::Experiment010306 general physicsPhysical Review Letters
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Microcalorimeter/EBIT measurements of X-ray spectra of highly charged ions

2001

Spectra of highly charged Ar, Kr, Xe and Fe ions, produced in an Electron Beam Ion Trap (EBIT), have been recorded in a broad X-ray energy band (0.2 keV to 10 keV) with a microcalorimeter detector. The first analysis of the Kr spectra has been completed and most of the spectral lines have been identified as transitions of B- to Al-like Kr. Line intensity ratios of Fe XVII have been measured and compared with theoretical models.

PhysicsAtomic and Molecular Physics and OpticPhysics::Instrumentation and DetectorsDetectorTheoretical modelsCondensed Matter PhysicsAtomic and Molecular Physics and OpticsSpectral lineIonSettore FIS/05 - Astronomia E AstrofisicaMathematical PhysicAtomic physicsElectronic band structureX ray spectraMathematical PhysicsLine (formation)Electron beam ion trap
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Superparamagnetism in Ising Clusters

1992

Recent experiments on small ferromagnetic clusters have inspired introduction of a number of seemingly quite different theoretical models. We shall argue that all these models show superparamagnetic behaviour above the blocking temperature but below the Curie temperature. In particular, we shall show that Ising clusters display superparamagnetism and introduce a simple correction to the usual tank behaviour of magnetisation which has to be included for very small clusters. We also discuss the dependence of magnetisation on coordination number.

PhysicsCondensed Matter::Materials ScienceMagnetizationCondensed matter physicsFerromagnetismCoordination numberTheoretical modelsCurie temperatureCondensed Matter::Strongly Correlated ElectronsIsing modelSuperparamagnetism
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Total free energy of a spin-crossover molecular system

2004

The free energy of spin-crossover molecular systems studied so far deal with the inner degrees of freedom of the spin-crossover molecules and a variety of interaction schemes between the molecules in the high spin (HS) and low spin (LS) states. Different types of transition curves, gradual, abrupt, hysteresis, and also two step transitions have been simulated or even satisfactorily fitted to experimental data. However, in the last decade spin transition curves were measured, especially under pressure, which could not be explained within these theoretical models. In this contribution the total free energy of an anharmonic lattice incorporating spin-crossover molecules which have a certain mi…

PhysicsCondensed matter physicsSpin crossoverLattice (order)IsotropyAnharmonicitySpin transitionTheoretical modelsMoleculeCondensed Matter PhysicsCrystallographic defectElectronic Optical and Magnetic MaterialsPhysical Review B
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The discovery of an expanding X-ray source in the HH 154 protostellar jet

2006

We have performed, in October 2005, a deep Chandra X-ray observation of HH 154. Comparison with the previous (2001) Chandra observation allows to detect proper motion down to the level predicted by models of X-ray emitting shocks in the jet. The 2005 Chandra observation of HH 154 shows unexpected morphological changes of the X-ray emission in comparison with the 2001 data. Two components are present: a stronger, point-like component with no detectable motion and a weaker component which has expanded in size by approximately 300 AU over the 4 years time base of the two observations. This expansion corresponds to approximately 500 km/s, very close to the velocity of the X-ray emitting shock i…

PhysicsJet (fluid)Proper motionShock (fluid dynamics)Astrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)X-rayTheoretical modelsFOS: Physical sciencesAstronomy and AstrophysicsMedium densityAstrophysicsAstrophysicsL1551-IRS-5Space and Planetary ScienceEMISSIONAstronomy & Astrophysics
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Observation of the decay KLO→ e+e−ep+e−

1991

Abstract Two events with the characteristic of the decay K L O → e + e − e − have been observed with a negligible expected background from which a branching ratio of (4±3)×10 −8 is derived. This result is consistent with values estimated from theoretical models based on the double internal conventional of the decay K L O → γγ .

PhysicsNuclear and High Energy PhysicsBranching fractionTheoretical modelsAtomic physicsPhysics Letters B
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