Search results for "Spacetime"

showing 9 items of 159 documents

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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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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A Numbers-Based Approach to a Free Particle's Spacetime

2020

A possibility is proposed to define the proper spacetime of a free nonzerorest- mass m_0 particle based on the connection of its lasting proper time to an open sequence of natural numbers counting de Broglie time periods (h/c^2)(m^(-1)_ 0 ) [see R. Ferber, A Missing Link: What is Behind de Broglie's" Periodic Phenomenon"?, Foundations of Physics Letters 9, 575 (1996)]. It is suggested to define a set of twodirectional intervals of the particle's proper space (proper distances) following the construction of positive and negative integers from the ordered pairs of the natural numbers, which belong to the sequence 1, 2, ..., n defining the elapsed interval of de Broglie time t_n. Corresponding…

de Broglie proper timeproper spaceproper spacetime:NATURAL SCIENCES::Physics [Research Subject Categories]proper timeconstruction of integersenergy of proper space
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Handling of Small Scale Structures of the Irradiance Field for Solar Energy System Analysis – A Review

2016

Abstract Satellite derived irradiance information currently approaches a status as standard input for solar energy system analysis. Due to intrinsic limitations in spatial and temporal resolution, these data fail to give information of the full dynamics of the irradiance field in space and time. The analysis of systems with sensibility to details of the temporal evolution of the irradiance field and systems with sensibility to the spatial inhomogeneity of the field require knowledge of its fine-structured. Thus, methods for a respective enhancement of the satellite derived data are needed. This contribution presents various approaches discussed for setting up respective input data.

fine scale irradiance data010504 meteorology & atmospheric sciencesSpacetimeComputer sciencebusiness.industry020209 energyirradiance fieldIrradiance02 engineering and technologytemporal and spatial structureSolar energy01 natural sciencesField (geography)Energy(all)Temporal resolution0202 electrical engineering electronic engineering information engineeringSatellitebusinessScale (map)Derived Data0105 earth and related environmental sciencesRemote sensingEnergy Procedia
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Distributed n-player approachability via time and space average consensus

2012

Abstract In this paper we consider repeated coalitional games with transferable utilities (TU) over networks. Namely, we consider a set of n players that have to distribute among themselves a vector of rewards (one for each player). In our network version there is no coordinator allocating the rewards, but the agents have to agree on a common time-averaged vector by updating the local estimates of the reward vector. The common time-averaged reward vector has to approach a suitable constraint set, called core of the game, that guarantees that no agents benefit from quitting the grand coalition. We propose a doubly (over time and space) averaging distributed algorithm. At every iteration, eac…

game theoryComputer Science::Computer Science and Game TheoryMathematical optimizationSpacetimeReward-based selectionconsensus algorithmsGeneral Medicinecontrol optimization game theoryApproachabilitySet (abstract data type)Constraint (information theory)Core (game theory)Order (business)Distributed algorithmnetwork systemMathematicsIFAC Proceedings Volumes
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Quantum aspects originated by Gravitation: from cosmology to astrophysics

2018

El estudio de campos cuánticos que se propagan en espacio-tiempos clásicos, curvos y dinámicos, ofrece una primera manera de evaluar las consecuencias de la teoría cuántica cuando los fenómenos gravitatorios no son despreciables. Esta es una cuestión importante que debe ser abordada cuando un campo gravitatorio intenso juega un papel principal en la dinámica de un sistema físico, tal como ocurre durante el universo temprano (inflación cósmica) o en la formación de agujeros negros astrofísicos. Una de las características más sorprendentes de esta materia es quizás el hecho de que el cálculo de observables físicos, incluso para campos sin interacción, frecuentemente involucra operadores cuadr…

renormalization in curved spacetimeelectromagnetic field:FÍSICA [UNESCO]UNESCO::FÍSICAgeneral relativityclassical symmetriesinflationquantum anomaliesquantum field theorycosmology
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Pseudospectrum of Reissner-Nordström black holes: Quasinormal mode instability and universality

2021

Black hole spectroscopy is a powerful tool to probe the Kerr nature of astrophysical compact objects and their environment. The observation of multiple ringdown modes in gravitational waveforms could soon lead to high-precision gravitational spectroscopy, so it is critical to understand if the quasinormal mode spectrum is stable against perturbations. It was recently shown that the pseudospectrum can shed light on the spectral stability of black hole quasinormal modes. We study the pseudospectrum of Reissner-Nordstr\"om spacetimes and we find a spectral instability of scalar and gravitoelectric quasinormal modes in subextremal and extremal black holes, extending similar findings for the Sch…

star: compactspace-time: Schwarzschildblack hole: Reissner-NordstroemScalar (mathematics)[PHYS.MPHY]Physics [physics]/Mathematical Physics [math-ph]01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationGeneral Relativity and Quantum Cosmology0103 physical sciencesQuasinormal mode010306 general physicsperturbation: gravitationMathematical PhysicsMathematical physicsPseudospectrumPhysicsSpacetime010308 nuclear & particles physicsHorizonquasinormal modegravitational radiationblack hole: stabilityMathematics::Spectral Theorystabilityblack hole: quasinormal modequasinormal mode: spectrumBlack holeperturbation: scalarwave: model[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Schwarzschild radius
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Scattering of Co-Current Surface Waves on an Analogue Black Hole

2018

We report on what is to our knowledge the first scattering experiment of surface waves on an accelerating transcritical flow, which in the analogue gravity context is described by an effective spacetime with a black-hole horizon. This spacetime has been probed by an incident co-current wave, which partially scatters into an outgoing countercurrent wave on each side of the horizon. The measured scattering amplitudes are compatible with the predictions of the hydrodynamical theory, where the kinematical description in terms of the effective metric is exact.

surface: deformationGeneral Physics and AstronomyFOS: Physical sciencesContext (language use)General Relativity and Quantum Cosmology (gr-qc)black hole: horizonGravitation and Astrophysics01 natural sciences7. Clean energyGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical scienceswave: scatteringsurfaceeffect: Hawkingcorrelation function010306 general physicsPhysicsSpacetimeScatteringHorizonFluid Dynamics (physics.flu-dyn)Physics - Fluid Dynamics[PHYS.PHYS.PHYS-GEN-PH]Physics [physics]/Physics [physics]/General Physics [physics.gen-ph]Scattering amplitudeBlack holeFlow (mathematics)space-timeSurface waveQuantum electrodynamics[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]
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$$\mathscr {K}$$-Convergence of Finite Volume Solutions of the Euler Equations

2020

We review our recent results on the convergence of invariant domain-preserving finite volume solutions to the Euler equations of gas dynamics. If the classical solution exists we obtain strong convergence of numerical solutions to the classical one applying the weak-strong uniqueness principle. On the other hand, if the classical solution does not exist we adapt the well-known Prokhorov compactness theorem to space-time probability measures that are generated by the sequences of finite volume solutions and show how to obtain the strong convergence in space and time of observable quantities. This can be achieved even in the case of ill-posed Euler equations having possibly many oscillatory s…

symbols.namesakeFinite volume methodSpacetimeCompactness theoremsymbolsApplied mathematicsObservableUniquenessInvariant (physics)Euler equationsMathematicsProbability measure
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