Search results for "RELATIVITY"

showing 10 items of 1213 documents

Gravity, Non-Commutative Geometry and the Wodzicki Residue

1993

We derive an action for gravity in the framework of non-commutative geometry by using the Wodzicki residue. We prove that for a Dirac operator $D$ on an $n$ dimensional compact Riemannian manifold with $n\geq 4$, $n$ even, the Wodzicki residue Res$(D^{-n+2})$ is the integral of the second coefficient of the heat kernel expansion of $D^{2}$. We use this result to derive a gravity action for commutative geometry which is the usual Einstein Hilbert action and we also apply our results to a non-commutative extension which, is given by the tensor product of the algebra of smooth functions on a manifold and a finite dimensional matrix algebra. In this case we obtain gravity with a cosmological co…

High Energy Physics - TheoryPhysicsResidue (complex analysis)General Physics and AstronomyFOS: Physical sciencesGeometryCosmological constantGeneral Relativity and Quantum Cosmology (gr-qc)Riemannian manifoldDirac operatorGeneral Relativity and Quantum Cosmologysymbols.namesakeGeneral Relativity and Quantum CosmologyTensor productHigh Energy Physics - Theory (hep-th)Einstein–Hilbert actionsymbolsGeometry and TopologyCommutative propertyMathematical PhysicsHeat kernel
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Generalized Slow Roll in the Unified Effective Field Theory of Inflation

2017

We provide a compact and unified treatment of power spectrum observables for the effective field theory (EFT) of inflation with the complete set of operators that lead to second-order equations of motion in metric perturbations in both space and time derivatives, including Horndeski and GLPV theories. We relate the EFT operators in ADM form to the four additional free functions of time in the scalar and tensor equations. Using the generalized slow roll formalism, we show that each power spectrum can be described by an integral over a single source that is a function of its respective sound horizon. With this correspondence, existing model independent constraints on the source function can b…

High Energy Physics - TheoryPhysicsSource functionCosmology and Nongalactic Astrophysics (astro-ph.CO)Slow rollSpacetime010308 nuclear & particles physicsScalar (mathematics)Spectral densityEquations of motionFOS: Physical sciencesObservableGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physicsClassical mechanicsHigh Energy Physics - Theory (hep-th)0103 physical sciencesEffective field theory010306 general physicsAstrophysics - Cosmology and Nongalactic Astrophysics
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Confronting the IR Fixed Point Cosmology with High Redshift Observations

2004

We use high-redshift type Ia supernova and compact radio source data in order to test the infrared (IR) fixed point model of the late Universe which was proposed recently. It describes a cosmology with a time dependent cosmological constant and Newton constant whose dynamics arises from an underlying renormalization group flow near an IR-attractive fixed point. Without any finetuning or quintessence field it yields $\Omega_{\rm M}=\Omega_{\Lambda}=1/2$. Its characteristic $t^{4/3}$-dependence of the scale factor leads to a distance-redshift relation whose predictions are compared both to the supernova and to the radio source data. According to the $\chi^2$ test, the fixed point model reprod…

High Energy Physics - TheoryPhysicsmedia_common.quotation_subjectAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsCosmological constantAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Type (model theory)Fixed pointAstrophysicsGeneral Relativity and Quantum CosmologyRedshiftUniverseCosmologyHigh Energy Physics - Theory (hep-th)Scale factor (cosmology)media_commonQuintessence
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Decoherent neutrino mixing, dark energy, and matter-antimatter asymmetry

2004

A CPT violating decoherence scenario can easily account for all the experimental evidence in the neutrino sector including LSND. In this work it is argued that this framework can also accommodate the Dark Energy content of the Universe, as well as the observed matter-antimatter asymmetry.

High Energy Physics - TheoryPhysics::General PhysicsNuclear and High Energy PhysicsParticle physicsPhysics::Instrumentation and DetectorsCPT symmetrymedia_common.quotation_subjectFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyCosmologyNuclear physicsHigh Energy Physics - Phenomenology (hep-ph)Neutrino oscillationComputer Science::Databasesmedia_commonPhysicsHigh Energy Physics::PhenomenologyFísicaUniverseHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Neutrino detectorAntimatterDark energyHigh Energy Physics::ExperimentNeutrinoPhysical Review D
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The Minkowski and conformal superspaces

2006

We define complex Minkowski superspace in 4 dimensions as the big cell inside a complex flag supermanifold. The complex conformal supergroup acts naturally on this super flag, allowing us to interpret it as the conformal compactification of complex Minkowski superspace. We then consider real Minkowski superspace as a suitable real form of the complex version. Our methods are group theoretic, based on the real conformal supergroup and its Lie superalgebra.

High Energy Physics - TheoryPure mathematicsFOS: Physical sciencesReal formFísicaStatistical and Nonlinear PhysicsConformal mapLie superalgebraMathematical Physics (math-ph)Mathematics - Rings and AlgebrasSuperspaceHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Rings and Algebras (math.RA)Mathematics::Quantum AlgebraMinkowski spaceSupermanifoldFOS: MathematicsCompactification (mathematics)Mathematics::Representation TheorySupergroupMathematical PhysicsMathematics
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Quantum groups and deformed special relativity

1994

The structure and properties of possible $q$-Minkowski spaces is discussed, and the corresponding non-commutative differential calculi are developed in detail and compared with already existing proposals. This is done by stressing its covariance properties as described by appropriate reflection equations. Some isomorphisms among the space-time and derivative algebras are demonstrated, and their representations are described briefly. Finally, some physical consequences and open problems are discussed.

High Energy Physics - TheoryPure mathematicsLorentz transformationStructure (category theory)FOS: Physical sciencesCovariancesymbols.namesakeReflection (mathematics)High Energy Physics - Theory (hep-th)Doubly special relativitysymbolsDifferential (infinitesimal)QuantumMathematics
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Critical reflections on asymptotically safe gravity

2020

Asymptotic safety is a theoretical proposal for the ultraviolet completion of quantum field theories, in particular for quantum gravity. Significant progress on this program has led to a first characterization of the Reuter fixed point. Further advancement in our understanding of the nature of quantum spacetime requires addressing a number of open questions and challenges. Here, we aim at providing a critical reflection on the state of the art in the asymptotic safety program, specifying and elaborating on open questions of both technical and conceptual nature. We also point out systematic pathways, in various stages of practical implementation, towards answering them. Finally, we also take…

High Energy Physics - TheoryReflection (computer programming)Computer scienceEffective field theoryMaterials Science (miscellaneous)Asymptotic safety in quantum gravityBiophysicsGeneral Physics and AstronomyUnitarityFixed pointQuantum spacetime01 natural sciences530General Relativity and Quantum CosmologyTheoretical High Energy Physics0103 physical sciencesCalculusddc:530High Energy PhysicsQuantum gravitationQuantum field theoryPhysical and Theoretical Chemistry010306 general physicsRunning couplingsMathematical PhysicsStructure (mathematical logic)ObservablesObservablelcsh:QC1-999Asymptotic safetySettore FIS/02 - Fisica Teorica Modelli e Metodi MatematiciQuantum gravityRenormalization grouplcsh:Physics
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Adiabatic expansions for Dirac fields, renormalization, and anomalies

2018

11 pags.

High Energy Physics - TheoryRenormalizationConformal anomalyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyRenormalizationGeneral Relativity and Quantum CosmologyDirac fieldFriedmann-Lemaître-Robertson-Walker spacetime0103 physical sciencesMinkowski spaceRenormalization; anomalies010306 general physicsAdiabatic processYukawa couplingMathematical physicsPhysicsMaterialesSpacetime010308 nuclear & particles physicsYukawa potentialAdiabatic expansionCosmologyHigh Energy Physics - Theory (hep-th)Regularization (physics)anomaliesScalar fieldPhysical Review D
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Running Immirzi Parameter and Asymptotic Safety

2011

We explore the renormalization group (RG) properties of quantum gravity, using the vielbein and the spin connection as the fundamental field variables. We require the effective action to be invariant under the semidirect product of spacetime diffeomorphisms and local frame rotations. Starting from the corresponding functional integral we review the construction of an appropriate theory space and an exact funtional RG equation operating on it. We then solve this equation on a truncated space defined by a three parameter family of Holst-type actions which involve a running Immirzi parameter. We find evidence for the existence of an asymptotically safe fundamental theory. It is probably inequi…

High Energy Physics - TheorySemidirect productSpacetimeImmirzi parameterAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Renormalization groupGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum gravitySpin connectionEffective actionMathematical physicsMathematics
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Sterile Neutrinos, Black Hole Vacuum and Holographic Principle

2021

We construct an effective field theory (EFT) model that describes matter field interactions with Schwarzschild mini-black-holes (SBH's), treated as a scalar field, $B_0(x)$. Fermion interactions with SBH's require a random complex spurion field, $\theta_{ij}$, which we interpret as the EFT description of "holographic information," which is correlated with the SBH as a composite system. We consider Hawking's virtual black hole vacuum (VBH) as a Higgs phase, $\langle B_0 \rangle =V$. Integrating sterile neutrino loops, the field $\theta_{ij}$ is promoted to a dynamical field, necessarily developing a tachyonic instability and acquiring a VEV of order the Planck scale. For $N$ sterile neutrino…

High Energy Physics - TheorySterile neutrinoParticle physicsPhysics and Astronomy (miscellaneous)FOS: Physical scienceslcsh:AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:QB460-466Effective field theorylcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsVirtual black holeEngineering (miscellaneous)Physics010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyOrder (ring theory)Higgs phaseBlack holeHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)lcsh:QC770-798Scalar fieldSchwarzschild radius
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