Search results for "Metric tensor"

showing 10 items of 26 documents

A programming guide for tensor networks with global SU(2) symmetry

2020

Abstract This paper is a manual with tips and tricks for programming tensor network algorithms with global S U ( 2 ) symmetry. We focus on practical details that are many times overlooked when it comes to implementing the basic building blocks of codes, such as useful data structures to store the tensors, practical ways of manipulating them, and adapting typical functions for symmetric tensors. Here we do not restrict ourselves to any specific tensor network method, but keep always in mind that the implementation should scale well for simulations of higher-dimensional systems using, e.g., Projected Entangled Pair States, where tensors with many indices may show up. To this end, the structur…

PhysicsFibonacci number010308 nuclear & particles physicsAlgebraic specificationGeneral Physics and AstronomyData structure01 natural sciencesTopological quantum computerAlgebraFusion tree0103 physical sciencesSymmetric tensorTensorSymmetry (geometry)010306 general physicsAnnals of Physics
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An intrinsic characterization of the Schwarzschild metric

1998

An intrinsic algorithm that exclusively involves conditions on the metric tensor and its differential concomitants is presented to identify every type-D static vacuum solution. In particular, the necessary and sufficient explicit and intrinsic conditions are given for a Lorentzian metric to be the Schwarzschild solution.

PhysicsGeneral Relativity and Quantum CosmologyPhysics and Astronomy (miscellaneous)Schwarzschild coordinatesMetric signatureSchwarzschild geodesicsKerr metricSchwarzschild metricDeriving the Schwarzschild solutionMetric tensor (general relativity)Mathematical physicsIntrinsic metricClassical and Quantum Gravity
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Kaluza-Klein origin for the superstring tension

1992

The natural configuration space of a string in a background antisymmetric tensor potential is not loop space, but a principal U(1) bundle over loop space. This allows a Kaluza-Klein--like interpretation of the string tension as momentum along the U(1) fiber, and a similar interpretation is possible for a {ital p}-dimensional object. The higher-dimensional'' action incorporating this momentum as a dynamical variable is given for a {ital p}-dimensional supersymmetric extended object, in a general supergravity background. Its relevance, for a flat background, to classical anomalies'' in the supersymmetry algebra is explained.

PhysicsHigh Energy Physics::TheoryClassical mechanicsAntisymmetric tensorSupergravityLoop spaceKaluza–Klein theorySuperstring theorySupersymmetryString (physics)Supersymmetry algebraMathematical physicsPhysical Review D
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Labeling spherically symmetric spacetimes with the Ricci tensor

2017

We complete the intrinsic characterization of spherically symmetric solutions partially accomplished in a previous paper [Class.Quant.Grav. (2010) 27 205024]. In this approach we consider every compatible algebraic type of the Ricci tensor, and we analyze specifically the conformally flat case for perfect fluid and Einstein-Maxwell solutions. As a direct application we obtain the {\em ideal} labeling (exclusively involving explicit concomitants of the metric tensor) of the Schwarzschild interior metric and the Vaidya solution. The Stephani universes and some significative subfamilies are also characterized.

PhysicsIdeal (set theory)Physics and Astronomy (miscellaneous)010308 nuclear & particles physicsFOS: Physical sciencesPerfect fluidGeneral Relativity and Quantum Cosmology (gr-qc)Type (model theory)01 natural sciencesGeneral Relativity and Quantum Cosmology0103 physical sciencesMetric (mathematics)Metric tensor (general relativity)Algebraic number010306 general physicsSchwarzschild radiusRicci curvatureMathematical physics
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Implications of nonsymmetric metric theories for particle physics. New interpretation of the Pauli coupling

2014

In this work, we provide a possible geometrical interpretation of the spin of elementary particles. In particular, it is investigated how the wave equations of matter are altered by the addition of an antisymmetric contribution to the metric tensor. In this scenario, the explicit form of the matter wave equations is investigated in a general curved spacetime, and then the equations are particularized to the flat case. Unlike traditional approaches of Nonsymmetric Gravitational Theories (NGT), in which the gravitational field is responsible for breaking the symmetry of the flat Minkowski metric, we find more natural to consider that, in general, the metric of the spacetime could be nonsymme…

PhysicsNuclear and High Energy PhysicsAntisymmetric relationScalar (physics)General Physics and AstronomyAstronomy and AstrophysicsSymmetry (physics)General Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyTheoretical physicssymbols.namesakePauli exclusion principleMetric (mathematics)Minkowski spacesymbolsMetric tensor (general relativity)Spin-½
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An intrinsic characterization of spherically symmetric spacetimes

2010

We give the necessary and sufficient (local) conditions for a metric tensor to be a non conformally flat spherically symmetric solution. These conditions exclusively involve explicit concomitants of the Riemann tensor. As a direct application we obtain the {\em ideal} labeling of the Schwarzschild, Reissner-Nordstr\"om and Lema\^itre-Tolman-Bondi solutions.

PhysicsRiemann curvature tensorIdeal (set theory)Physics and Astronomy (miscellaneous)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Characterization (mathematics)General Relativity and Quantum CosmologyPhysics::History of PhysicsGeneral Relativity and Quantum Cosmologysymbols.namesakesymbolsSymmetric solutionMetric tensor (general relativity)Schwarzschild radiusMathematical physicsClassical and Quantum Gravity
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An intrinsic characterization of the Kerr metric

2009

We give the necessary and sufficient (local) conditions for a metric tensor to be the Kerr solution. These conditions exclusively involve explicit concomitants of the Riemann tensor.

PhysicsRiemann curvature tensorsymbols.namesakePhysics and Astronomy (miscellaneous)Kerr metricsymbolsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Characterization (mathematics)Metric tensor (general relativity)General Relativity and Quantum CosmologyMathematical physics
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On distinguished polynomials and their projections

2012

We study projections and injections between projective tensor products spaces or spaces of polynomials and we show that the example of a polynomial constructed in (4), that is neither p-dominated nor compact, can be identified with the projection map of the symmetric tensor product onto the space. Also we give a characterization of the weak and quasi approximation properties on symmetric tensor products.

Pure mathematicsTensor productTensor product of algebrasPower sum symmetric polynomialGeneral MathematicsTopological tensor productMathematical analysisTensor product of Hilbert spacesSymmetric tensorElementary symmetric polynomialTensor densityMathematicsAnnales Academiae Scientiarum Fennicae Mathematica
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Odd-intrinsic-parity processes within the Resonance Effective Theory of QCD

2003

19 páginas, 4 figuras.-- arXiv:hep-ph/0306157v1

Quantum chromodynamicsPhysicsNuclear and High Energy PhysicsParticle physicsMesonHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyNuclear TheoryFísicaFOS: Physical sciencesVector meson dominance1/N ExpansionIntrinsic parityQCDPseudoscalarHigh Energy Physics - PhenomenologyPionGlobal symmetriesHigh Energy Physics - Phenomenology (hep-ph)Antisymmetric tensorEffective field theoryHigh Energy Physics::ExperimentChiral lagrangians
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The classical two-dimensional Heisenberg model revisited: An $SU(2)$-symmetric tensor network study

2021

The classical Heisenberg model in two spatial dimensions constitutes one of the most paradigmatic spin models, taking an important role in statistical and condensed matter physics to understand magnetism. Still, despite its paradigmatic character and the widely accepted ban of a (continuous) spontaneous symmetry breaking, controversies remain whether the model exhibits a phase transition at finite temperature. Importantly, the model can be interpreted as a lattice discretization of the $O(3)$ non-linear sigma model in $1+1$ dimensions, one of the simplest quantum field theories encompassing crucial features of celebrated higher-dimensional ones (like quantum chromodynamics in $3+1$ dimensio…

Sigma modelSpontaneous symmetry breakingQC1-999Lattice (group)General Physics and AstronomyFOS: Physical sciencesClassical Heisenberg modelQuantum Materials53001 natural sciences010305 fluids & plasmasTheoretical physicsHigh Energy Physics - Lattice0103 physical sciencesSymmetric tensorTensorQuantum field theory010306 general physicsclassical Heisenberg modelCondensed Matter - Statistical MechanicsPhysicsQuantum PhysicsStatistical Mechanics (cond-mat.stat-mech)Heisenberg modelPhysics500 Naturwissenschaften und Mathematik::530 Physik::530 PhysikHigh Energy Physics - Lattice (hep-lat)magnetismstatistical and condensed matter physicsQuantum Physics (quant-ph)
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