Search results for "Relativity"

showing 10 items of 1213 documents

Electronic properties of graphene: A learning path for undergraduate students

2016

The purpose of this work is to present a learning path aimed at deepening student understanding of the fundamental concepts underlying the electronic properties of new materials, graphene in particular. To achieve this task, we propose a five-week long workshop where students may be introduced to fundamental concepts of advanced physics, rarely used in learning paths, such as the symmetry properties of the crystal lattice, the group theory , the features of the free electron wave functions and energy levels, the relativistic Dirac equation. Particular emphasis is given to the manner of introducing these concepts, since an essential knowledge of solid state physics, quantum physics and relat…

Theoretical computer scienceSolid-state physicsSettore FIS/08 - Didattica E Storia Della FisicaLattice theoryCrystal symmetryElectronSettore FIS/03 - Fisica Della MateriaTask (project management)EducationElectronic propertieRelativitysymbols.namesakeTheory of relativityMathematics educationLinear equationWave functionsPhysicsSequenceSymmetry (physics)Dirac equationQuantum theoryPath (graph theory)symbolsThe Conceptual FrameworkGroup theoryStudent
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The Mathematicians’ Happy Hunting Ground: Einstein’s General Theory of Relativity

2004

There is hardly any doubt that for physics special relativity theory is of much greater consequence than the general theory. The reverse situation prevails with respect to mathematics: there special relativity theory had comparatively little, general relativity theory very considerable, influence, above all upon the development of a general scheme for differential geometry. —Hermann Weyl, “Relativity as a Stimulus to Mathematical Research,” pp. 536–537.

Theoretical physicsTheory of relativityHistory and Philosophy of ScienceStatic interpretation of timeDoubly special relativityGeneral MathematicsQuantum mechanicsAbsolute time and spaceFour-forceTest theories of special relativityEmission theorySpecial relativity (alternative formulations)MathematicsThe Mathematical Intelligencer
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Seeing reality through Einstein's eyes: a teaching proposal for special relativity

2021

The teaching of Special Relativity is still a critical issue not only for students but also for teachers. In this paper, we describe the trial of a learning unit on the Special Relativity topic based on Minkowski's approach through spacetime diagrams, following the results in pedagogical researches in this field. The main innovation of our project consists of a mechanical instrument: it allows to physically and mechanically represent Lorentz’s transformations by hands, exploring the effects of a change of the reference frame. Teachers and students can deal “by eye” with unusual phenomena as the loss of simultaneity, time dilation, length contraction, relativistic addition of velocities and …

Theoretical physicssymbols.namesakespecial relativitySpecial Relativity spacetime didactics of Physics High Schools laboratory of Special Relativity.PhilosophySettore FIS/08 - Didattica E Storia Della FisicasymbolsEinsteinlaboratory of special relativityspacetimedidactics of physicsSpecial relativity (alternative formulations)high schools
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A quantum model of Schwarzschild black hole evaporation

1996

We construct a one-loop effective metric describing the evaporation phase of a Schwarzschild black hole in a spherically symmetric null-dust model. This is achieved by quantising the Vaidya solution and by chosing a time dependent quantum state. This state describes a black hole which is initially in thermal equilibrium and then the equilibrium is switched off, so that the black hole starts to evaporate, shrinking to a zero radius in a finite proper time. The naked singularity appears, and the Hawking flux diverges at the end-point. However, a static metric can be imposed in the future of the end-point. Although this end-state metric cannot be determined within our construction, we show tha…

Thermal equilibriumPhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsAstrophysics::High Energy Astrophysical PhenomenaNaked singularityFOS: Physical sciencesRadiusGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum stateQuantum mechanicsMetric (mathematics)Schwarzschild metricAstronomiaProper time
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Symmetries and solvable models for evaporating 2D black holes

1997

We study the evaporation process of a 2D black hole in thermal equilibrium when the ingoing radiation is suddenly switched off. We also introduce global symmetries of generic 2D dilaton gravity models which generalize the extra symmetry of the CGHS model. © Elsevier Science B.V

Thermal equilibriumPhysicsNuclear and High Energy PhysicsGravity (chemistry)CGHS modelEvaporationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Atomic and Molecular Physics and OpticsSymmetry (physics)General Relativity and Quantum CosmologyBlack holeTheoretical physicsHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHomogeneous spaceDilaton
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Relativistic kinematic approach to the classical ideal gas

2019

he necessary and sufficient conditions for a unit time-like vector field to be the unit velocity of a classical ideal gas are obtained. In a recent paper [Coll, Ferrando and S\'aez, Phys. Rev D {\bf 99} (2019)] we have offered a purely hydrodynamic description of a classical ideal gas. Here we take one more step in reducing the number of variables necessary to characterize these media by showing that a plainly kinematic description can be obtained. We apply the results to obtain test solutions to the hydrodynamic equation that model the evolution in local thermal equilibrium of a classical ideal gas. \end{abstract}

Thermal equilibriumPhysicsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsMathematical analysisFOS: Physical sciencesKinematicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyIdeal gas0103 physical sciencesVector field010306 general physicsUnit (ring theory)
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Thermodynamic class II Szekeres-Szafron solutions. Singular models

2019

A family of parabolic Szekeres-Szafron class II solutions in local thermal equilibrium is studied and their associated thermodynamics are obtained. The subfamily with the hydrodynamic behavior of a generic ideal gas (defined by the equation of state $p = k n \Theta$) results to be an inhomogeneous generalization of flat FLRW $\gamma$-law models. Three significative interpretations that follow on from the choice of three specific thermodynamic schemes are analyzed in depth. First, the generic ideal gas in local thermal equilibrium; this interpretation leads to an inhomogeneous temperature $\Theta$. Second, the thermodynamics with homogeneous temperature considered by Lima and Tiomno (CQG 6 1…

Thermal equilibriumPhysicsPhysics and Astronomy (miscellaneous)Spacetime010308 nuclear & particles physicsEquation of state (cosmology)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesIdeal gasGeneral Relativity and Quantum CosmologyInterpretation (model theory)symbols.namesakeFriedmann–Lemaître–Robertson–Walker metric0103 physical sciencesCompressibilitysymbolsLimit (mathematics)010306 general physicsMathematical physics
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Local thermal equilibrium and ideal gas Stephani universes

2005

The Stephani universes that can be interpreted as an ideal gas evolving in local thermal equilibrium are determined. Five classes of thermodynamic schemes are admissible, which give rise to five classes of regular models and three classes of singular models. No Stephani universes exist representing an exact solution to a classical ideal gas (one for which the internal energy is proportional to the temperature). But some Stephani universes may approximate a classical ideal gas at first order in the temperature: all of them are obtained. Finally, some features about the physical behavior of the models are pointed out.

Thermal equilibriumPhysicsTheoretical physicsExact solutions in general relativityPhysics and Astronomy (miscellaneous)Internal energyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]First orderIdeal gasGeneral Relativity and Quantum Cosmology
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Unified theory for analysis of curved thin-walled girders with open and closed cross section through HSA method

2016

Abstract The behaviour of thin-walled structures is deeply influenced by non-uniform torsion and cross section distortion. In this paper the extension of the Hamiltonian Structural Analysis (HSA) Method to thin-walled straight and curved beams is presented. The proposed method solves the structural elastic problem of thin-walled beams through the definition of a Hamiltonian system composed of 1st order differential equations. The method allows engineers to solve the elastic problem by introducing the degrees of freedom and the corresponding compatibility equations, founding equilibrium equations in the variational form. The methodology is explained in the framework of the so-called Generali…

Timoshenko beam theoryCurved beamDifferential equationThin-walled structuresTorsion (mechanics)020101 civil engineeringDistortion02 engineering and technologyElastic foundation0201 civil engineeringHamiltonian systemTransfer matricesSettore ICAR/09 - Tecnica Delle Costruzioni020303 mechanical engineering & transportsClassical mechanicsExact solutions in general relativity0203 mechanical engineeringHamiltonian structural analysisGirderBeam on elastic foundation analogyUnified field theoryBeam (structure)Civil and Structural EngineeringMathematicsGeneral beam theory
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LEM for twisted re-entrant angle sections

2014

In this paper an innovative numerical method named as line element-less method, LEM, for finding solution of torsion problem has been extended to all shaped sections, including sections possessing re-entrant angles at their boundary. The response solution in terms of shear stress field or Prandtl function or warping function in all domain and for any kind of domain with arbitrary contour, may be performed quickly, calculating line integrals only. The method takes full advantage of the theory of analytic complex function and is robust in the sense that returns exact solution if this exists. Numerical implementation of LEM has been developed using Mathematica software without resorting to any…

TorsionRe-entrant angleDiscretizationMechanical EngineeringNumerical analysisMathematical analysisPrandtl numberLine integralTorsion (mechanics)GeometryStress fieldComputer Science ApplicationsStress fieldsymbols.namesakeExact solutions in general relativityModeling and SimulationShear stresssymbolsComplex potential functionGeneral Materials ScienceCivil and Structural EngineeringMathematicsComputers & Structures
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