Search results for "General Relativity"

showing 10 items of 1057 documents

How to interpret black hole entropy?

1998

We consider a possibility that the entropy of a Schwarzschild black hole has two different interpretations: The black hole entropy can be understood either as an outcome of a huge degeneracy in the mass eigenstates of the hole, or as a consequence of the fact that the interior region of black hole spacetime is separated from the exterior region by a horizon. In the latter case, no degeneracy in the mass eigenstates needs to be assumed. Our investigation is based on calculations performed with Lorentzian partition functions obtained for a whole maximally extended Schwarzschild spacetime, and for its right-hand-side exterior region. To check the correctness of our analysis we reproduce, in th…

Physics::General PhysicsGeneral Relativity and Quantum CosmologyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum Cosmology
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Relativistic Positioning Systems: Numerical Simulations

2014

The motion of satellite constellations similar to GPS and Galileo is numerically simulated and, then, the region where bifurcation (double positioning) occurs is appropriately represented. In the cases of double positioning, the true location may be found using additional information (angles or times). The zone where the Jacobian, J, of the transformation from inertial to emission coordinates vanishes is also represented and interpreted. It is shown that the uncertainties in the satellite world lines produce positioning errors, which depend on the value of |J|. The smaller this quantity the greater the expected positioning errors. Among all the available 4-tuples of satellites, the most app…

Physics::Space PhysicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum Cosmology
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The galaxy power spectrum take on spatial curvature and cosmic concordance

2020

The concordance of the $\Lambda$CDM cosmological model in light of current observations has been the subject of an intense debate in recent months. The 2018 Planck Cosmic Microwave Background (CMB) temperature anisotropy power spectrum measurements appear at face value to favour a spatially closed Universe with curvature parameter $\Omega_K<0$. This preference disappears if Baryon Acoustic Oscillation (BAO) measurements are combined with Planck data to break the geometrical degeneracy, although the reliability of this combination has been questioned due to the strong tension present between the two datasets when assuming a curved Universe. Here, we approach this issue from yet another point…

Planckcosmological modelCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectCosmological parametersSpatial curvatureDark matterCosmic microwave backgroundCosmic background radiationFOS: Physical sciencesanisotropycosmic background radiationAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)power spectrumCurvature01 natural sciencesGeneral Relativity and Quantum Cosmologydark matterCosmologyacousticsymbols.namesake0103 physical sciencesPlanck010303 astronomy & astrophysicsmedia_commonPhysics[PHYS.GRQC] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]010308 nuclear & particles physicstemperatureAstronomy and AstrophysicsoscillationtensionUniverseGalaxybaryonCosmological tensionsSpace and Planetary Sciencecurvature[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]symbolsgalaxy[PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph][PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic AstrophysicsPhysics of the Dark Universe
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Correlation functions for a strongly coupled boson system and plane partitions.

2011

A quantum phase model is introduced as a limit for very strong interactions of a strongly correlated q -boson hopping model. The exact solution of the phase model is reviewed, and solutions are also provided for two correlation functions of the model. Explicit expressions, including both amplitude and scaling exponent, are derived for these correlation functions in the low temperature limit. The amplitudes were found to be related to the number of plane partitions contained in boxes of finite size.

Plane (geometry)General MathematicsMathematical analysisGeneral EngineeringGeneral Physics and AstronomyAmplitudeExact solutions in general relativityQuantum mechanicsExponentLimit (mathematics)ScalingQuantumBosonMathematicsPhilosophical transactions. Series A, Mathematical, physical, and engineering sciences
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Singularities of lightlike hypersurfaces in Minkowski four-space

2006

We classify singularities of lightlike hypersurfaces in Minkowski 4-space via the contact invariants for the corresponding spacelike surfaces and lightcones.

Pure mathematicsLightlike hypersurfaceGeneral MathematicsMathematical analysisspacelike surfacelightconePhysics::Classical PhysicsSpace (mathematics)53A3541458C27Computer Science::OtherLorentzian distance-squared functionGeneral Relativity and Quantum CosmologyMinkowski spaceGravitational singularityMathematics::Differential GeometryMathematicsTohoku Mathematical Journal
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Supermanifolds, Symplectic Geometry and Curvature

2016

We present a survey of some results and questions related to the notion of scalar curvature in the setting of symplectic supermanifolds.

Pure mathematicsMathematical analysisSymplectic representationGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheorySymplectic vector spaceMathematics::Differential GeometrySymplectomorphismMathematics::Symplectic GeometryMoment mapGeometry and topologyScalar curvatureSymplectic geometrySymplectic manifoldMathematics
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Flat lightlike hypersurfaces in Lorentz–Minkowski 4-space

2009

Abstract The lightlike hypersurfaces in Lorentz–Minkowski space are of special interest in Relativity Theory. In particular, the singularities of these hypersurfaces provide good models for the study of different horizon types. We introduce the notion of flatness for these hypersurfaces and study their singularities. The classification result asserts that a generic classification of flat lightlike hypersurfaces is quite different from that of generic lightlike hypersurfaces.

Pure mathematicsMathematics::Complex VariablesLorentz transformationMathematical analysisGeneral Physics and AstronomySpace (mathematics)General Relativity and Quantum Cosmologysymbols.namesakeMathematics::Algebraic GeometryTheory of relativityClassification resultMinkowski spaceHorizon (general relativity)symbolsGravitational singularityMathematics::Differential GeometryGeometry and TopologyMathematical PhysicsFlatness (mathematics)MathematicsJournal of Geometry and Physics
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Global properties of codimension two spacelike submanifolds in Minkowski space

2009

Abstract We consider codimension two spacelike submanifolds with a parallel normal field (i.e. vanishing normal curvature) in Minkowski space. We use the analysis of their contacts with hyperplanes and hyperquadrics in order to get some global information on them. As a consequence we obtain new versions of Carathéodory's and Loewner's conjectures on spacelike surfaces in 4-dimensional Minkowski space and 4-flattenings theorems for closed spacelike curves in 3-dimensional Minkowski space.

Pure mathematicseducationMinkowski's theoremMathematical analysisNormal curvatureOrder (ring theory)CodimensionNormal fieldGlobal informationGeneral Relativity and Quantum CosmologyHyperplaneMinkowski spaceMathematics::Differential GeometryGeometry and TopologyMathematicsadvg
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Comments on `A new efficient method for calculating perturbation energies using functions which are not quadratically integrable'

1996

The recently proposed method of calculating perturbation energies using a non-normalizable wavefunction by Skala and Cizek is analysed and rigorously proved.

Quadratic growthGeneral Relativity and Quantum CosmologyClassical mechanicsIntegrable systemGeneral Physics and AstronomyPerturbation (astronomy)Statistical and Nonlinear PhysicsWave functionMathematical PhysicsMathematicsJournal of Physics A: Mathematical and General
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New approach to describe two coupled spins in a variable magnetic field

2021

We propose a method to describe the evolution of two spins coupled by hyperfine i nteraction in an external time- dependent magnetic field. We apply the approach to the case of hyperfine interaction with axial symmetry, which can be solved exactly in a constant, appropriately oriented magnetic field. In order to t reat t he n onstationary d ynamical p roblem, we modify the time-dependent Schrödinger equation through a change of representation that, by exploiting an instantaneous (adiabatic) basis makes the time-dependent Hamiltonian diagonal at any time instant. The solution of the transformed time-dependent Schrödinger FRVBUJPO in the form of chronologically ordered exponents with transpar…

Quantum ComputationPhysicsQuantum PhysicsGeometric PhaseSpinsQuantum Physics; Quantum PhysicsFOS: Physical sciencesSchrödinger equationMagnetic fieldsymbols.namesakeExact solutions in general relativityQuantum mechanicssymbolsHamiltonian (quantum mechanics)Adiabatic processAxial symmetryQuantum Physics (quant-ph)QubitsHyperfine structure
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