Search results for " relativity"

showing 10 items of 1158 documents

Quantum walk on a cylinder

2016

We consider the 2D alternate quantum walk on a cylinder. We concentrate on the study of the motion along the open dimension, in the spirit of looking at the closed coordinate as a small or "hidden" extra dimension. If one starts from localized initial conditions on the lattice, the dynamics of the quantum walk that is obtained after tracing out the small dimension shows the contribution of several components, which can be understood from the study of the dispersion relations for this problem. In fact, these components originate from the contribution of the possible values of the quasi-momentum in the closed dimension. In the continuous space-time limit, the different components manifest as …

High Energy Physics - Theorymass generationQuantum simulatorFOS: Physical sciencesQuantum entanglementGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmology010305 fluids & plasmassymbols.namesake[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesquantum walksQuantum walkBoundary value problem010306 general physicsEntropy (arrow of time)ComputingMilieux_MISCELLANEOUSquantum simulationPhysicsQuantum Physics[PHYS.HLAT]Physics [physics]/High Energy Physics - Lattice [hep-lat]Mass generationExtra dimensionsClassical mechanicsHigh Energy Physics - Theory (hep-th)Dirac equationsymbolsQuantum Physics (quant-ph)
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Pseudospectrum and Black Hole Quasinormal Mode Instability

2020

We study the stability of quasinormal modes (QNM) in asymptotically flat black hole spacetimes by means of a pseudospectrum analysis. The construction of the Schwarzschild QNM pseudospectrum reveals the following: (i) the stability of the slowest-decaying QNM under perturbations respecting the asymptotic structure, reassessing the instability of the fundamental QNM discussed by Nollert [H. P. Nollert, About the Significance of Quasinormal Modes of Black Holes, Phys. Rev. D 53, 4397 (1996)] as an "infrared" effect; (ii) the instability of all overtones under small-scale ("ultraviolet") perturbations of sufficiently high frequency, which migrate towards universal QNM branches along pseudospec…

High Energy Physics - TheoryperturbationcompactificationQC1-999[PHYS.MPHY]Physics [physics]/Mathematical Physics [math-ph]FOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesInstabilityStability (probability)General Relativity and Quantum Cosmologyoperator: spectrumGeneral Relativity and Quantum CosmologyTheoretical physics0103 physical sciencesQuasinormal modestructurenumerical calculations010306 general physicsMathematical PhysicsPseudospectrumPhysicsCompactification (physics)[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]010308 nuclear & particles physicsPhysicsOperator (physics)black hole: stabilityMathematical Physics (math-ph)Schwarzschildquasinormal mode: spectrumBlack holeHigh Energy Physics - Theory (hep-th)[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]spectralSchwarzschild radiusPhysical Review X
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Born–Infeld inspired modifications of gravity

2017

General Relativity has shown an outstanding observational success in the scales where it has been directly tested. However, modifications have been intensively explored in the regimes where it seems either incomplete or signals its own limit of validity. In particular, the breakdown of unitarity near the Planck scale strongly suggests that General Relativity needs to be modified at high energies and quantum gravity effects are expected to be important. This is related to the existence of spacetime singularities when the solutions of General Relativity are extrapolated to regimes where curvatures are large. In this sense, Born-Infeld inspired modifications of gravity have shown an extraordin…

High Energy Physics - Theorystar: compactcosmological model[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]space-time: black holeGeneral Physics and AstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]Gravitationquantum gravity: effectBorn–Infeld gravityPhysicsenergy: highBlack holes[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]formationCosmologyregularizationcurvaturewormhole[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational singularitySingularitiesAstrophysics - Cosmology and Nongalactic AstrophysicsGravity (chemistry)Cosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityEarly universegeneral relativity: solutionFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Theoretical physicsGeneral Relativity and Quantum Cosmologyspace-time: singularity0103 physical sciencesunitaritystructureWormholeinflation010306 general physicsCompact objectsSpacetime010308 nuclear & particles physicsscale: PlanckBlack holeBorn-Infeld modelHigh Energy Physics - Theory (hep-th)gravitationQuantum gravity[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Thermodynamical Properties of Horizons

2002

We show, by using Regge calculus, that the entropy of any finite part of a Rindler horizon is, in the semi-classical limit, one quarter of the area of that part. We argue that this result implies that the entropy associated with any horizon of spacetime is, in semi-classical limit, one quarter of its area. As an example, we derive the Bekenstein-Hawking entropy law for the Schwarzschild black hole.

High Energy Physics::TheoryGeneral Relativity and Quantum CosmologyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum Cosmology
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"Table 19" of "Search for heavy particles decaying into a top-quark pair in the fully hadronic final state in $pp$ collisions at $\sqrt{s} =13$ TeV w…

2020

Expected and observed upper limits on the cross-section times branching fraction of Kaluza-Klein graviton decaying into top-quark pair as a function of the graviton mass.

High Energy Physics::TheoryGeneral Relativity and Quantum CosmologyPhysics::General Physicstop-quark pair13000.0Proton-Proton Scatteringp p --> t tbarHigh Energy Physics::Experimenttop
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Einstein's Washington Manuscript on Unified Field Theory

2020

In this note, we point attention to and briefly discuss a curious manuscript of Einstein, composed in 1938 and entitled "Unified Field Theory," the only such writing, published or unpublished, carrying this title without any further specification. Apparently never intended for publication, the manuscript sheds light both on Einstein's modus operandi as well as on the public role of Einstein's later work on a unified field theory of gravitation and electromagnetism.

History530 PhysicsAlbert EinsteinElias Avery LowePhysics - History and Philosophy of PhysicsFOS: Physical sciences050905 science studiesComputer Science::Digital LibrariesUnpublished ManuscriptGravitationsymbols.namesakeGeneral Relativity and Quantum Cosmology510 MathematicsHistory and Philosophy of ScienceLibrary of congressElectromagnetismPublic roleHistory and Philosophy of Physics (physics.hist-ph)0601 history and archaeologyEinsteinUnified field theoryCondensed Matter::Quantum GasesBeitragKaluza TheoryPhilosophy05 social sciences510 Mathematik06 humanities and the arts530 PhysikPhysics::History of PhysicsEpistemologyLibrary of CongressPeter BergmannUnified Field Theory060105 history of science technology & medicinesymbols0509 other social sciencesBeiträge
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Václav Hlavatý on intuition in Riemannian space

2019

Abstract We present a historical commentary together with an English translation of a mathematical-philosophical paper by the Czech differential geometer and later proponent of a geometrized unified field theory Vaclav Hlavatý (1894–1969). The paper was published in 1924 at the height of interpretational debates about recent advancements in differential geometry triggered by the advent of Einstein's general theory of relativity. In the paper he argued against a naive generalization of analogical reasoning valid for curves and surfaces in three-dimensional Euclidean space to the case of higher-dimensional curved Riemannian spaces. Instead, he claimed, the only secure ground to arrive at resu…

HistoryGeneral relativityEuclidean spaceGeneral MathematicsPhilosophy06 humanities and the artsRiemannian geometrysymbols.namesake060105 history of science technology & medicineDifferential geometryArgumentsymbolsCalculus0601 history and archaeologyEinsteinDifferential (infinitesimal)Unified field theoryHistoria Mathematica
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Progresses in 3D integral imaging with optical processing

2008

Integral imaging is a promising technique for the acquisition and auto-stereoscopic display of 3D scenes with full parallax and without the need of any additional devices like special glasses. First suggested by Lippmann in the beginning of the 20th century, integral imaging is based in the intersection of ray cones emitted by a collection of 2D elemental images which store the 3D information of the scene. This paper is devoted to the study, from the ray optics point of view, of the optical effects and interaction with the observer of integral imaging systems.

HistoryIntegral imagingbusiness.industryComputer scienceOptical processingObserver (special relativity)RayComputer Science ApplicationsEducationOpticsComputer visionImaging scienceArtificial intelligencebusinessParallaxJournal of Physics: Conference Series
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Flat synchronizations in spherically symmetric space-times

2010

It is well known that the Schwarzschild space-time admits a spacelike slicing by flat instants and that the metric is regular at the horizon in the associated adapted coordinates (Painleve-Gullstrand metric form). We consider this type of flat slicings in an arbitrary spherically symmetric space-time. The condition ensuring its existence is analyzed, and then, we prove that, for any spherically symmetric flat slicing, the densities of the Weinberg momenta vanish. Finally, we deduce the Schwarzschild solution in the extended Painleve-Gullstrand-Lemaitre metric form by considering the coordinate decomposition of the vacuum Einstein equations with respect to a flat spacelike slicing.

HistoryKerr metricMathematical analysisSpherically symmetric spacetimeComputer Science ApplicationsEducationGeneral Relativity and Quantum CosmologySchwarzschild coordinatesSymmetric spaceMetric (mathematics)Schwarzschild metricDeriving the Schwarzschild solutionSchwarzschild radiusMathematicsJournal of Physics: Conference Series
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Effect of the milling conditions on the degree of amorphization of selenium by milling in a planetary ball mill

2007

The effect of the milling parameters (rotation speed of the milling device and duration of milling) on the phase composition of the products of milling of fully crystalline selenium has been investigated. The milling was conducted using a planetary micromill and the phase composition of the milling products was determined by differential thermal analysis. It has been found that ball milling leads to the partial amorphization of the starting crystalline material. The content of amorphous phase in the milling products depends, in a rather complicated way, on the milling parameters. At the milling parameters adopted in the present study, the milling product was never fully amorphous. The compl…

HistoryMaterials scienceHigh Energy Physics::LatticeMetallurgychemistry.chemical_elementCondensed Matter::Disordered Systems and Neural NetworksComputer Science ApplicationsEducationAmorphous solidlaw.inventionDegree (temperature)Condensed Matter::Materials ScienceGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheorychemistrylawPhase compositionDifferential thermal analysisDeformation (engineering)CrystallizationBall millSeleniumJournal of Physics: Conference Series
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