Search results for "relativity"

showing 10 items of 1213 documents

Homogeneous three-dimensional Riemannian spaces

2020

The necessary and sufficient conditions for a three-dimensional Riemannian metric to admit a transitive group of isometries are obtained. These conditions are Intrinsic, Deductive, Explicit and ALgorithmic, and they offer an IDEAL labeling of these geometries. It is shown that the transitive action of the group naturally falls into an unfolding of some of the ten types in the Bianchi-Behr classification. Explicit conditions, depending on the Ricci tensor, are obtained that characterize all these types.

PhysicsPure mathematicsIdeal (set theory)Physics and Astronomy (miscellaneous)010308 nuclear & particles physicsGroup (mathematics)Transitive actionFOS: Physical sciencesTransitive groupGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyHomogeneous0103 physical sciencesHomogeneous spaceMetric (mathematics)Mathematics::Differential Geometry010306 general physicsRicci curvature
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Dimension of the isometry group in three-dimensional Riemannian spaces

2021

The necessary and sufficient conditions for a three-dimensional Riemannian metric to admit a group of isometries of dimension $r$ acting on s-dimensional orbits are obtained. These conditions are Intrinsic, Deductive, Explicit and ALgorithmic and they offer an IDEAL labeling that improves previously known invariant studies.

PhysicsPure mathematicsIdeal (set theory)Physics and Astronomy (miscellaneous)Dimension (vector space)Group (mathematics)Computer Science::Information RetrievalMetric (mathematics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (mathematics)Isometry groupGeneral Relativity and Quantum CosmologyClassical and Quantum Gravity
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Coordinates and frames from the causal point of view

2006

Lorentzian frames may belong to one of the 199 causal classes. Of these numerous causal classes, people are essentially aware only of two of them. Nevertheless, other causal classes are present in some well-known solutions, or present a strong interest in the physical construction of coordinate systems. Here we show the unusual causal classes to which belong so familiar coordinate systems as those of Lema{\^{\i}}tre, those of Eddington-Finkelstein, or those of Bondi-Sachs. Also the causal classes associated to the Coll light coordinates (four congruences of real geodetic null lines) and to the Coll positioning systems (light signals broadcasted by four clocks) are analyzed. The role that th…

PhysicsPure mathematicsNull (mathematics)Coordinate systemFOS: Physical sciencesGeodetic datumPoint (geometry)General Relativity and Quantum Cosmology (gr-qc)Congruence relationGeneral Relativity and Quantum CosmologyAIP Conference Proceedings
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An intrinsic characterization of 2+2 warped spacetimes

2010

We give several equivalent conditions that characterize the 2+2 warped spacetimes: imposing the existence of a Killing-Yano tensor $A$ subject to complementary algebraic restrictions; in terms of the projector $v$ (or of the canonical 2-form $U$) associated with the 2-planes of the warped product. These planes are principal planes of the Weyl and/or Ricci tensors and can be explicitly obtained from them. Therefore, we obtain the necessary and sufficient (local) conditions for a metric tensor to be a 2+2 warped product. These conditions exclusively involve explicit concomitants of the Riemann tensor. We present a similar analysis for the conformally 2+2 product spacetimes and give an invaria…

PhysicsPure mathematicsRiemann curvature tensorPhysics and Astronomy (miscellaneous)Degenerate energy levelsFOS: Physical sciencesProduct metricGeneral Relativity and Quantum Cosmology (gr-qc)Fixed pointGeneral Relativity and Quantum Cosmologylaw.inventionsymbols.namesakeProjectorlawsymbolsTensorAlgebraic numberInvariant (mathematics)
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Maximal slicings in spherical symmetry: Local existence and construction

2011

We show that any spherically symmetric spacetime locally admits a maximal spacelike slicing and we give a procedure allowing its construction. The construction procedure that we have designed is based on purely geometrical arguments and, in practice, leads to solve a decoupled system of first order quasi-linear partial differential equations. We have explicitly built up maximal foliations in Minkowski and Friedmann spacetimes. Our approach admits further generalizations and efficient computational implementation. As by product, we suggest some applications of our work in the task of calibrating Numerical Relativity complex codes, usually written in Cartesian coordinates.

PhysicsPure mathematicsWork (thermodynamics)Partial differential equationFOS: Physical sciencesStatistical and Nonlinear PhysicsGeneral Relativity and Quantum Cosmology (gr-qc)First orderSpherically symmetric spacetimeGeneral Relativity and Quantum Cosmologylaw.inventionGeneral Relativity and Quantum CosmologyNumerical relativitylawMinkowski spaceCartesian coordinate systemCircular symmetryMathematical PhysicsComputingMethodologies_COMPUTERGRAPHICSJournal of Mathematical Physics
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Exact solutions for the mutual inductance of circular coils and elliptic coils

2012

An exact solution is presented for the mutual inductance between general noncoaxial thin circular and elliptic coils with parallel axes. The thin coil solution is given as an angular integral of an elliptic integral expression. In addition, for the coaxial case, an exact solution is given for the mutual inductance of a thick circular coil and a thick elliptic coil. The elliptic coil is such that the coil thickness is the same along both elliptic semi-axes. The thick coil solution is given as an integral of an expression involving Bessel and Struve functions. Extensive numerical results for sample geometries are given for both solutions, which are cross checked against each other in the limi…

PhysicsQuantitative Biology::BiomoleculesPhysics::Medical PhysicsMathematical analysisElectronic Optical and Magnetic MaterialsMagnetic fieldInductancesymbols.namesakeExact solutions in general relativityElectromagnetic coilStruve functionsymbolsElliptic integralElectrical and Electronic EngineeringCoaxialBessel functionIEEE Transactions on Magnetics
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The Geometry of Space-Time and Its Deformations from a Physical Perspective

2007

We start with an epistemological introduction on the evolution of the concepts of space and time and more generally of physical concepts in the context of the relation between mathematics and physics from the point of view of deformation theory. The concepts of relativity, including anti de Sitter space-time, and of quantization, are important paradigms; we briefly present these and some consequences. The importance of symmetries and of space-time in fundamental physical theories is stressed. The last section deals with “composite elementary particles” in anti de Sitter space-time and ends with speculative ideas around possible quantized anti de Sitter structures in some parts of the univer…

PhysicsQuantization (physics)Theoretical physicsTheory of relativitySpacetimeSpace timeDeformation theoryHomogeneous spaceElementary particleGeometryAnti-de Sitter space
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Resonance interaction energy between two accelerated identical atoms in a coaccelerated frame and the Unruh effect

2016

We investigate the resonance interaction energy between two uniformly accelerated identical atoms, interacting with the scalar field or the electromagnetic field in the vacuum state, in the reference frame coaccelerating with the atoms. We assume that one atom is excited and the other in the ground state, and that they are prepared in their correlated symmetric or antisymmetric state. Using perturbation theory, we separate, at the second order in the atom-field coupling, the contributions of vacuum fluctuations and radiation reaction field to the energy shift of the interacting system. We show that only the radiation reaction term contributes to the resonance interaction between the two ato…

PhysicsQuantum PhysicsField (physics)010308 nuclear & particles physicsVacuum stateFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Interaction energy01 natural sciencesResonance (particle physics)General Relativity and Quantum CosmologyLamb shiftresonance interactionUnruh effectExcited state0103 physical sciencesUnruh effectquantum field theory in curved spaceAtomic physicsQuantum Physics (quant-ph)010306 general physicsGround statePhysical Review D
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Thermal and non-thermal signatures of the Unruh effect in Casimir-Polder forces

2014

We show that Casimir-Polder forces between two relativistic uniformly accelerated atoms exhibit a transition from the short distance thermal-like behavior predicted by the Unruh effect, to a long distance non-thermal behavior, associated with the breakdown of a local inertial description of the system. This phenomenology extends the Unruh thermal response detected by a single accelerated observer to an accelerated spatially extended system of two particles, and we identify the characteristic length scale for this crossover with the inverse of the proper acceleration of the two atoms. Our results are derived separating at fourth order in perturbation theory the contributions of vacuum fluctu…

PhysicsQuantum PhysicsInertial frame of referenceCharacteristic lengthVacuum stateGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Casimir-Polder forceGeneral Relativity and Quantum CosmologyCasimir effectCondensed Matter - Other Condensed MatterUnruh effectClassical mechanicsVacuum FluctuationsUnruh EffectProper accelerationQuantum Physics (quant-ph)Scalar fieldQuantum fluctuationOther Condensed Matter (cond-mat.other)
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Collision-model-based approach to non-Markovian quantum dynamics

2013

We present a theoretical framework to tackle quantum non-Markovian dynamics based on a microscopic collision model (CM), where the bath consists of a large collection of initially uncorrelated ancillas. Unlike standard memoryless CMs, we endow the bath with memory by introducing inter-ancillary collisions between next system-ancilla interactions. Our model interpolates between a fully Markovian dynamics and the continuous interaction of the system with a single ancilla, i.e., a strongly non-Markovian process. We show that in the continuos limit one can derive a general master equation, which while keeping such features is guaranteed to describe an unconditionally completely positive and tra…

PhysicsQuantum PhysicsQuantum decoherenceQuantum dynamicsMarkov processFOS: Physical sciencesAtomic and Molecular Physics and Opticssymbols.namesakeExact solutions in general relativityClassical mechanicsSPINNon-Markovian open quantum systems collision modelsMaster equationDissipative systemsymbolsStatistical physicsQuantum informationQuantum Physics (quant-ph)Quantum
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