Search results for "Mathematical physics"

showing 10 items of 2687 documents

Comparison between the fCCZ4 and BSSN formulations of Einstein equations in spherical polar coordinates

2015

Recently, we generalized a covariant and conformal version of the Z4 system of the Einstein equations using a reference metric approach, that we denote as fCCZ4. We successfully implemented and tested this approach in a 1D code that uses spherical coordinates and assumes spherical symmetry, obtaining from one to three orders of magnitude reduction of the Hamiltonian constraint violations with respect to the BSSN formulation in tests involving neutron star spacetimes. In this work, we show preliminary results obtained with the 3D implementation of the fCCZ4 formulation in a fully 3D code using spherical polar coordinates.

PhysicsHistoryLog-polar coordinatesSpherical coordinate systemAction-angle coordinatesSymmetry (physics)Computer Science ApplicationsEducationClassical mechanicsGeneralized coordinatesHamiltonian constraintEinstein field equationsCovariant transformationMathematical physicsJournal of Physics: Conference Series
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On the local existence of maximal slicings in spherically symmetric spacetimes

2010

In this talk we show that any spherically symmetric spacetime admits locally a maximal spacelike slicing. The above condition is reduced to solve a decoupled system of first order quasi-linear partial differential equations. The solution may be accomplished analytical or numerically. We provide a general procedure to construct such maximal slicings.

PhysicsHistoryPartial differential equationFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)First orderSpherically symmetric spacetimeGeneral Relativity and Quantum CosmologyComputer Science ApplicationsEducationMathematical physics
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Appell Functions and the Scalar One-Loop Three-point Integrals in Feynman Diagrams

2002

The scalar three-point function appearing in one-loop Feynman diagrams is compactly expressed in terms of a generalized hypergeometric function of two variables. Use is made of the connection between such Appell function and dilogarithms coming from a previous investigation. Special cases are obtained for particular values of internal masses and external momenta.

PhysicsHistoryParticle physicsScalar (mathematics)Mathematics::Classical Analysis and ODEsFOS: Physical sciencesGeneralized hypergeometric functionComputer Science ApplicationsEducationHigh Energy Physics - Phenomenologysymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)symbolsFeynman diagramMathematical physics
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Group-Theoretic analysis of the mixing angle in the electroweak gauge group

1996

In this paper the authors provide strong mathematical support for the idea that the experimentally measured magnitude 1 - M{sub W}{sup 2}/M{sub Z}{sup 2} associated with sin{sup 2}{theta}{sub w} in the standard model of electroweak interactions cannot be simultaneously identified with the squared quotient of the electric charge by the SU(2) charge, e{sup 2}/g{sup 2}. In fact, the natural, mathematical requirement that the Weinberg rotation between the gauge fields associated with the third component of the {open_quotes}weak isospin{close_quotes} (T{sub 3}) and the hypercharge (Y) proceeds from a global Lie-group homomorphism of the SU(2) {circle_times} U(1){sub y} gauge group in some locall…

PhysicsHyperchargeParticle physicsPhysics and Astronomy (miscellaneous)Gauge groupGeneral MathematicsLie algebraElectroweak interactionLie groupGrand Unified TheoryCharge (physics)Weinberg angleMathematical physicsInternational Journal of Theoretical Physics
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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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Cosmology of the Planck Era from a Renormalization Group for Quantum Gravity

2001

Homogeneous and isotropic cosmologies of the Planck era before the classical Einstein equations become valid are studied taking quantum gravitational effects into account. The cosmological evolution equations are renormalization group improved by including the scale dependence of Newton's constant and of the cosmological constant as it is given by the flow equation of the effective average action for gravity. It is argued that the Planck regime can be treated reliably in this framework because gravity is found to become asymptotically free at short distances. The epoch immediately after the initial singularity of the Universe is described by an attractor solution of the improved equations w…

PhysicsInflation (cosmology)High Energy Physics - TheoryNuclear and High Energy PhysicsAstrophysics (astro-ph)FOS: Physical sciencesHierarchy problemGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Planck timeQuantum cosmologyFlatness problemMathematical physicsPlanck lengthLoop quantum cosmology
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Inflation, renormalization, and CMB anisotropies

2010

5 páginas.-- Trabajo presentado al Spanish Relativity Meeting (ERE 2009).-- El PDF es la versión pre-print (arXiv:1002.3914v1).

PhysicsInflation (cosmology)History010308 nuclear & particles physicsCosmic microwave backgroundScalar (mathematics)FOS: Physical sciencesObservableGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyComputer Science ApplicationsEducationMetric expansion of spaceRenormalizationRegularization (physics)0103 physical sciencesQuantum field theory010306 general physicsMathematical physics
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Spiral Inflation with Coleman-Weinberg Potential

2015

We apply the idea of spiral inflation to Coleman-Weinberg potential, and show that inflation matching well observations is allowed for a symmetry-breaking scale ranging from an intermediate scale to GUT scale even if the quartic coupling $\lambda$ is of $\mathcal{O}(0.1)$. The tensor-to-scalar ratio can be of $\mathcal{O}(0.01)$ in case of GUT scale symmetry-breaking.

PhysicsInflation (cosmology)Nuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Scale (ratio)010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFísicaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsLambdaCoupling (probability)01 natural sciencesHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)Quantum mechanicsQuartic function0103 physical sciencesColeman–Weinberg potentialGrand Unified TheorySymmetry breaking010306 general physicsMathematical physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Instantons and theΔI=1/2Rule

2001

The instanton-induced interaction leads to a significant enhancement of the Ao weak amplitude determining the DeltaI = 1/2 rule, through the contribution of operators with dimension d = 9, as we show in the weak K--> pi(pi) decay.

PhysicsInstantonAmplitudeDimension (vector space)General Physics and AstronomyMathematical physicsPhysical Review Letters
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Relaxation of periodic and nonstandard growth integrals by means of two-scale convergence

2019

An integral representation result is obtained for the variational limit of the family functionals $\int_{\Omega}f\left(\frac{x}{\varepsilon}, Du\right)dx$, as $\varepsilon \to 0$, when the integrand $f = f (x,v)$ is a Carath\'eodory function, periodic in $x$, convex in $v$ and with nonstandard growth.

PhysicsIntegral representationRegular polygonScale (descriptive set theory)homomgenizationFunction (mathematics)two scale convergencehomomgenization; two scale convergencehomomgenization two scale convergenceMathematics - Analysis of PDEsConvergence (routing)FOS: MathematicsRelaxation (physics)Limit (mathematics)Analysis of PDEs (math.AP)Mathematical physics
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