Search results for "Diagram"

showing 10 items of 795 documents

Phase behaviour of heteronuclear dimers in three-dimensional systems—a Monte Carlo study

2008

Monte Carlo simulation in the grand canonical ensemble, the histogram reweighting technique and finite size scaling are used to study the phase behaviour of dimers in three-dimensional systems. A single molecule is composed of two segments A and B, and the bond between them cannot be broken. The phase diagrams have been estimated for a set of model systems. Different structures formed by heteronuclear dimers have been found. The results show a great variety of vapour–liquid coexistence behaviour depending on the strength of the interactions between segments.

Grand canonical ensembleHeteronuclear moleculeChemistryHistogramPhase (matter)Monte Carlo methodMoleculeGeneral Materials ScienceStatistical physicsCondensed Matter PhysicsScalingPhase diagramJournal of Physics: Condensed Matter
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Transformation of UML models to CSP : a case study for graph transformation tools

2008

Graph transformation provides an intuitive mechanism for capturing model transformations. In the current paper, we investigate and compare various graph transformation tools using a compact practical model transformation case study carried out as part of the AGTIVE 2007 Tool Contest [22]. The aim of this case study is to generate formal CSP processes from high-level UML activity diagrams, which enables to carry out mathematical analysis of the system under design.

Graph rewritingTransformation (function)Current (mathematics)Unified Modeling LanguageProgramming languageCarry (arithmetic)Model transformationActivity diagramcomputer.software_genrecomputerAlgorithmcomputer.programming_languageMathematicsProceedrings of the third international symposium on Applications of Graph Transformations with Industrial Relevance (AGTIVE 2007), October 10-12, 2007, Kassel, Germany
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Ābolskābes enantiomēru veidoto cieto šķīdumu eksperimentālie un teorētiskie pētijumi

2017

Ābolskābes enantiomēru veidoto cieto šķīdumu eksperimentālie un teorētiskie pētījumi. Sala E., darba vadītājs Dr. Chem. Bērziņš A., zinātniskais konsultants Mg. Chem. Rēķis T. Maģistra darbs, 40 lappuses, 24 attēli, 7 tabulas, 58 literatūras avoti. Latviešu valodā. Darbā konstruēta ābolskābes enantiomēru divkomponentu fāžu diagramma, kā arī pētīta ābolskābes skalēmisku maisījumu fāžu dažādība, izmantojot diferenciāli skenējošo kalorimetriju un pulvera rentgendifraktometriju. Izmatojot aprēķinu ķīmiju pētīti un aprakstīti ābolskābes cieto šķīdumu veidošanās strukturālie un enerģētiskie aspekti.

HIRĀLI SAVIENOJUMIDIVKOMPONENTU FĀŽU DIAGRAMMAAPRĒĶINU ĶĪMIJAĀBOLSKĀBECIETIE ŠĶĪDUMIĶīmija
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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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Advanced Stochastic Petri Net Modeling with the Mercury Scripting Language

2017

Formal models are widely used in performance and dependability studies of computational systems. Graphical modeling tools allow users to compose such models with ease, but they complicate the creation of models with a dynamic/complex structure, the hierarchical arrangement of different models, and the automatic execution of models with different parameter configurations. To overcome this problem, we created a scripting language for the Mercury tool that supports the combination of different modeling approaches (e.g., Stochastic Petri Nets and Reliability Block Diagrams) in a single project. In this paper, we focus on the extensions developed to improve the capabilities of Generalized Stocha…

Hierarchical modelingProgramming languageComputer science020206 networking & telecommunicationsReliability block diagram02 engineering and technologycomputer.software_genreScripting language0202 electrical engineering electronic engineering information engineeringStochastic Petri netDependability020201 artificial intelligence & image processingPhase-type distributionMercury (programming language)Discrete event simulationcomputercomputer.programming_languageProceedings of the 11th EAI International Conference on Performance Evaluation Methodologies and Tools
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Matter Dependence of the Four-Loop Cusp Anomalous Dimension

2019

We compute analytically the matter-dependent contributions to the quartic Casimir term of the four-loop light-like cusp anomalous dimension in QCD, with $n_f$ fermion and $n_s$ scalar flavours. The result is extracted from the double pole of a scalar form factor. We adopt a new strategy for the choice of master integrals with simple analytic and infrared properties, which significantly simplifies our calculation. To this end we first identify a set of integrals whose integrands have a dlog form, and are hence expected to have uniform transcendental weight. We then perform a systematic analysis of the soft and collinear regions of loop integration and build linear combinations of integrals w…

High Energy Physics - Theory530 PhysicsHigh Energy Physics::LatticeScalar (mathematics)FOS: Physical sciencesGeneral Physics and Astronomy10192 Physics Institute01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Feynman diagrams Form factors Perturbation theory Perturbative QCD Quantum field theory Scattering amplitudes Supersymmetric field theoriesQuartic function0103 physical sciencesFeynman diagramQuantum field theory010306 general physicsLinear combinationMathematical physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsPropagatorPerturbative QCD3100 General Physics and AstronomyHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)symbolsPhysical Review Letters
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Weight Systems from Feynman Diagrams

1996

We find that the overall UV divergences of a renormalizable field theory with trivalent vertices fulfil a four-term relation. They thus come close to establish a weight system. This provides a first explanation of the recent successful association of renormalization theory with knot theory.

High Energy Physics - TheoryAlgebra and Number TheoryAssociation (object-oriented programming)FOS: Physical sciencesMathematics::Geometric TopologyKnot theoryRenormalizationTheoretical physicssymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Mathematics - Quantum AlgebrasymbolsFOS: MathematicsFeynman diagramQuantum Algebra (math.QA)Field theory (psychology)Relation (history of concept)Mathematics
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Differential equations for Feynman integrals beyond multiple polylogarithms

2017

Differential equations are a powerful tool to tackle Feynman integrals. In this talk we discuss recent progress, where the method of differential equations has been applied to Feynman integrals which are not expressible in terms of multiple polylogarithms.

High Energy Physics - TheoryDifferential equationFeynman integralRepresentation (systemics)FOS: Physical sciencesFeynman graphHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Transformation (function)High Energy Physics - Theory (hep-th)ComputingMethodologies_SYMBOLICANDALGEBRAICMANIPULATIONsymbolsFeynman diagramMathematical physicsMathematicsProceedings of 13th International Symposium on Radiative Corrections (Applications of Quantum Field Theory to Phenomenology) — PoS(RADCOR2017)
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JaxoDraw: A graphical user interface for drawing Feynman diagrams

2003

JaxoDraw is a Feynman graph plotting tool written in Java. It has a complete graphical user interface that allows all actions to be carried out via mouse click-and-drag operations in a WYSIWYG fashion. Graphs may be exported to postscript/EPS format and can be saved in XML files to be used in later sessions. One of the main features of JaxoDraw is the possibility to produce LaTeX code that may be used to generate graphics output, thus combining the powers of TeX/LaTeX with those of a modern day drawing program. With JaxoDraw it becomes possible to draw even complicated Feynman diagrams with just a few mouse clicks, without the knowledge of any programming language.

High Energy Physics - TheoryJavacomputer.internet_protocolComputer scienceFOS: Physical sciencesGeneral Physics and Astronomycomputer.software_genreComputer graphicssymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Code (cryptography)Feynman diagramGraphicscomputer.programming_languageGraphical user interfaceProgramming languagebusiness.industryWYSIWYGHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Hardware and ArchitectureComputingMethodologies_DOCUMENTANDTEXTPROCESSINGsymbolsbusinesscomputerXMLComputer Physics Communications
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Efficient resummation of high post-Newtonian contributions to the binding energy

2021

A factorisation property of Feynman diagrams in the context the Effective Field Theory approach to the compact binary problem has been recently employed to efficiently determine the static sector of the potential at fifth post-Newtonian (5PN) order. We extend this procedure to the case of non-static diagrams and we use it to fix, by means of elementary algebraic manipulations, the value of more than one thousand diagrams at 5PN order, that is a substantial fraction of the diagrams needed to fully determine the dynamics at 5PN. This procedure addresses the redundancy problem that plagues the computation of the binding energy with respect to more "efficient" observables like the scattering an…

High Energy Physics - TheoryNuclear and High Energy PhysicsBlack HolesComputationFOS: Physical sciencesBinary numberContext (language use)General Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesake0103 physical sciencesEffective field theoryFeynman diagramlcsh:Nuclear and particle physics. Atomic energy. RadioactivityStatistical physicsAlgebraic numberResummation010306 general physicsPhysics010308 nuclear & particles physicsEffective Field TheoriesObservableHigh Energy Physics - Theory (hep-th)symbolslcsh:QC770-798Classical Theories of GravityJournal of High Energy Physics
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