Search results for "general relativity"

showing 10 items of 1057 documents

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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Advanced Virgo Status

2015

Abstract The detection of a gravitational wave signal in September 2015 by LIGO interferometers, announced jointly by LIGO collaboration and Virgo collaboration in February 2016, opened a new era in Astrophysics and brought to the whole community a new way to look at - or “listen” to - the Universe. In this regard, the next big step was the joint observation with at least three detectors at the same time. This configuration provides a twofold benefit: it increases the signal-to-noise ratio of the events by means of triple coincidence and allows a narrower pinpointing of GW sources, and, in turn, the search for Electromagnetic counterparts to GW signals. Advanced Virgo (AdV) is the second ge…

Triple coincidenceHistoryComputer sciencePhysics::Instrumentation and DetectorsAstronomy01 natural sciencesLIGO010303 astronomy & astrophysicsmedia_commonSettore FIS/01Detector/dk/atira/pure/sustainabledevelopmentgoals/partnershipsAstrophysics::Instrumentation and Methods for AstrophysicsDetectorsdetector: upgradeComputer Science ApplicationsInterferometryUpgrade[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]upgradeDetection rateAdvanced VirgoGWOrders of magnitude (power)Nuclear and High Energy PhysicsnoiseVIRGO: sensitivitydetector: performancemedia_common.quotation_subjectinterferometerJoint observationgravitational radiation: direct detectionAdvanced Virgo; GW; detectorsEducationelectromagnetic field: production[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wavesSDG 17 - Partnerships for the Goals0103 physical sciencesAerospace engineeringdetector: design010308 nuclear & particles physicsGravitational wavebusiness.industrygravitational radiationAstronomy and AstrophysicsLIGOUniversegravitational radiation detector* Automatic Keywords *VIRGODetectors; Gravitational waves; Nuclear and High Energy Physics; Astronomy and Astrophysicsgravitational radiation: emissionHigh Energy Physics::ExperimentTelecommunicationsbusiness[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Twin paradox in curved spacetime

2022

The twin paradox has played an important role in the history of special relativity (SR). A precise calculation would require the application of the general theory of relativity (GR) but, neglecting the acceleration phases of the traveling twin, even in SR it is possible to find the correct solution without logical contradictions. Nowadays it is well known that the twin thought experiment seems a paradox as a consequence of a naive application of time dilation and the principle of relativity. The twin who goes on space travel is the one who, returning to the twin at rest, finds the aged brother. Continuing in this pedagogical tradition, we want to add a further consideration. In fact, the ex…

Twin paradoxgeneral relativityGeneral Physics and Astronomygravitational time dilationEducation
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An Exact Solution for the Level-Crossing Rate of Shadow Fading Processes Modelled by Using the Sum-of-Sinusoids Principle

2008

Published version of an article in the journal: Wireless Personal Communications. The original publication is available at Springerlink. http://dx.doi.org/10.1007/s11277-008-9512-3 The focus of this paper is on the higher order statistics of spatial simulation models for shadowing processes. Such processes are generally assumed to follow the lognormal distribution. The proposed spatial simulation model is derived from a non-realizable lognormal reference model with given correlation properties by using Rice's sum-of-sinusoids. Both exact and approximate expressions are presented for the level-crossing rate (LCR) and the average duration of fades (ADF) of the simulation model. It is pointed …

VDP::Mathematics and natural science: 400::Information and communication science: 420::Communication and distributed systems: 423Spatial correlationComputer scienceEmphasis (telecommunications)Higher-order statisticsLevel crossingShadow fadingComputer Science ApplicationsExact solutions in general relativityVDP::Technology: 500::Information and communication technology: 550::Telecommunication: 552Log-normal distributionStatisticsApplied mathematicsElectrical and Electronic EngineeringFocus (optics)Wireless Personal Communications
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Observational constraints on inhomogeneous cosmological models without dark energy

2011

It has been proposed that the observed dark energy can be explained away by the effect of large-scale nonlinear inhomogeneities. In the present paper we discuss how observations constrain cosmological models featuring large voids. We start by considering Copernican models, in which the observer is not occupying a special position and homogeneity is preserved on a very large scale. We show how these models, at least in their current realizations, are constrained to give small, but perhaps not negligible in certain contexts, corrections to the cosmological observables. We then examine non-Copernican models, in which the observer is close to the center of a very large void. These models can gi…

Void (astronomy)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Physics and Astronomy (miscellaneous)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physics0103 physical sciencesHomogeneity (physics)98.62.Sb010303 astronomy & astrophysicsPhysics010308 nuclear & particles physics98.80.EsObservable95.36.+xCopernican principleNonlinear systemDark energysymbols[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]98.65.DxAstrophysics - Cosmology and Nongalactic AstrophysicsSpecial position
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Vacuum type I spacetimes and aligned Papapetrou fields: symmetries

2003

We analyze type I vacuum solutions admitting an isometry whose Killing 2--form is aligned with a principal bivector of the Weyl tensor, and we show that these solutions belong to a family of type I metrics which admit a group $G_3$ of isometries. We give a classification of this family and we study the Bianchi type for each class. The classes compatible with an aligned Killing 2--form are also determined. The Szekeres-Brans theorem is extended to non vacuum spacetimes with vanishing Cotton tensor.

Weyl tensorPhysicsClass (set theory)Physics and Astronomy (miscellaneous)Group (mathematics)Cotton tensorFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Type (model theory)General Relativity and Quantum Cosmologysymbols.namesakeGeneral Relativity and Quantum CosmologyHomogeneous spaceIsometrysymbolsMathematics::Differential GeometryBivectorMathematical physics
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On the classification of type D space–times

2002

We give a classification of the type D spacetimes based on the invariant differential properties of the Weyl principal structure. Our classification is established using tensorial invariants of the Weyl tensor and, consequently, besides its intrinsic nature, it is valid for the whole set of the type D metrics and it applies on both, vacuum and non-vacuum solutions. We consider the Cotton-zero type D metrics and we study the classes that are compatible with this condition. The subfamily of spacetimes with constant argument of the Weyl eigenvalue is analyzed in more detail by offering a canonical expression for the metric tensor and by giving a generalization of some results about the non-exi…

Weyl tensorPhysicsGeneral Relativity and Quantum Cosmologysymbols.namesakePure mathematicssymbolsFOS: Physical sciencesStatistical and Nonlinear PhysicsGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (mathematics)General Relativity and Quantum CosmologyMathematical PhysicsEigenvalues and eigenvectorsJournal of Mathematical Physics
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