Search results for "gravity"

showing 10 items of 537 documents

A class of nonlocal truncations in quantum Einstein gravity and its renormalization group behavior

2002

Motivated by the conjecture that the cosmological constant problem could be solved by strong quantum effects in the infrared we use the exact flow equation of Quantum Einstein Gravity to determine the renormalization group behavior of a class of nonlocal effective actions. They consist of the Einstein-Hilbert term and a general nonlinear function F(k, V) of the Euclidean space-time volume V. A partial differential equation governing its dependence on the scale k is derived and its fixed point is analyzed. For the more restrictive truncation of theory space where F(k, V) is of the form V+V ln V, V+V^2, and V+\sqrt{V}, respectively, the renormalization group equations for the running coupling…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsFOS: Physical sciencesOrder (ring theory)General Relativity and Quantum Cosmology (gr-qc)Cosmological constantRenormalization groupFixed pointSpace (mathematics)General Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum mechanicsQuantum gravityEffective actionCosmological constant problemPhysical Review D
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On selfdual spin-connections and asymptotic safety

2016

We explore Euclidean quantum gravity using the tetrad field together with a selfdual or anti-selfdual spin-connection as the basic field variables. Setting up a functional renormalization group (RG) equation of a new type which is particularly suitable for the corresponding theory space we determine the non-perturbative RG flow within a two-parameter truncation suggested by the Holst action. We find that the (anti-)selfdual theory is likely to be asymptotically safe. The existing evidence for its non-perturbative renormalizability is comparable to that of Einstein-Cartan gravity without the selfduality condition.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsField (physics)010308 nuclear & particles physicsMathematics::Analysis of PDEsAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Euclidean quantum gravitySpace (mathematics)01 natural sciencesGeneral Relativity and Quantum Cosmologylcsh:QC1-999Action (physics)High Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)Flow (mathematics)0103 physical sciencesFunctional renormalization groupMathematics::Differential Geometry010306 general physicsTetradlcsh:PhysicsMathematical physicsPhysics Letters B
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Space-Time Foam may Violate the Principle of Equivalence

2003

The interactions of different particle species with the foamy space-time fluctuations expected in quantum gravity theories may not be universal, in which case different types of energetic particles may violate Lorentz invariance by varying amounts, violating the equivalence principle. We illustrate this possibility in two different models of space-time foam based on D-particle fluctuations in either flat Minkowski space or a stack of intersecting D-branes. Both models suggest that Lorentz invariance could be violated for energetic particles that do not carry conserved charges, such as photons, whereas charged particles such electrons would propagate in a Lorentz-inavariant way. The D-brane …

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsGeneral Relativity and CosmologySpace timeAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsElectronGeneral Relativity and Quantum Cosmology (gr-qc)Lorentz covarianceAstrophysicsGeneral Relativity and Quantum CosmologyAtomic and Molecular Physics and OpticsCharged particleGluonHigh Energy Physics - PhenomenologyTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Minkowski spaceQuantum gravityPhenomenology (particle physics)
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Connections and geodesics in the space of metrics

2015

We argue that the exponential relation $g_{\mu\nu} = \bar{g}_{\mu\rho}\big(\mathrm{e}^h\big)^\rho{}_\nu$ is the most natural metric parametrization since it describes geodesics that follow from the basic structure of the space of metrics. The corresponding connection is derived, and its relation to the Levi-Civita connection and the Vilkovisky-DeWitt connection is discussed. We address the impact of this geometric formalism on quantum gravity applications. In particular, the exponential parametrization is appropriate for constructing covariant quantities like a reparametrization invariant effective action in a straightforward way. Furthermore, we reveal an important difference between Eucli…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsGeodesicFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Mathematical Physics (math-ph)General Relativity and Quantum CosmologyExponential functionCombinatoricsGeneral Relativity and Quantum CosmologyFormalism (philosophy of mathematics)High Energy Physics - Theory (hep-th)Quantum mechanicsEuclidean geometryQuantum gravityCovariant transformationEffective actionMathematical PhysicsPhysical Review D
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Cosmological waveguides for gravitational waves

1997

We study the linearized equations describing the propagation of gravitational waves through dust. In the leading order of the WKB approximation, dust behaves as a non-dispersive, non-dissipative medium. Taking advantage of these features, we explore the possibility that a gravitational wave from a distant source gets trapped by the gravitational field of a long filament of galaxies of the kind seen in the large scale structure of the Universe. Such a waveguiding effect may lead to a huge magnification of the radiation from distant sources, thus lowering the sensitivity required for a successful detection of gravitational waves by detectors like VIRGO, LIGO and LISA.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsGravitational-wave observatoryGravitational waveSpeed of gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGravitational accelerationGeneral Relativity and Quantum CosmologyLIGOGravitational energyGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Gravitational fieldGravitational redshiftPhysical Review D
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Born-Infeld Gravity: Constraints from Light-by-Light Scattering and an Effective Field Theory Perspective

2021

By using a novel technique that establishes a correspondence between general relativity and metric-affine theories based on the Ricci tensor, we are able to set stringent constraints on the free parameter of Born-Infeld gravity from the ones recently obtained for Born-Infeld electrodynamics by using light-by-light scattering data from ATLAS. We also discuss how these gravity theories plus matter fit within an effective field theory framework.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsGravity (chemistry)010308 nuclear & particles physicsGeneral relativityScatteringAtlas (topology)PhysicsQC1-999FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyLight scatteringTheoretical physicsHigh Energy Physics - Theory (hep-th)0103 physical sciencesEffective field theory010306 general physicsRicci curvatureFree parameter
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Gauging of flat groups in four dimensional supergravity

2002

We show that N=8 spontaneously broken supergravity in four dimensions obtained by Scherk-Schwarz generalized dimensional reduction can be obtained from a pure four dimensional perspective by gauging a suitable electric subgroup of E_{7,7}. Owing to the fact that there are non isomorphic choices of maximal electric subgroups of the U-duality group their gaugings give rise to inequivalent theories. This in particular shows that the Scherk-Schwarz gaugings do not fall in previous classifications of possible gauged N=8 supergravities. Gauging of flat groups appear in many examples of string compactifications in presence of brane fluxes.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsGroup (mathematics)SupergravityHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyFísicaFOS: Physical sciencesString (physics)Theoretical physicsHigh Energy Physics::TheoryPerspective (geometry)High Energy Physics - Theory (hep-th)Dimensional reductionBraneParticle Physics - Theory
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Renormalization group flow of the Holst action

2010

The renormalization group (RG) properties of quantum gravity are explored, using the vielbein and the spin connection as the fundamental field variables. The scale dependent effective action is required to be invariant both under space time diffeomorphisms and local frame rotations. The nonperturbative RG equation is solved explicitly on the truncated theory 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, probably inequivalent to metric quantum gravity constructed in the same way.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsImmirzi parameterAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Renormalization groupGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Functional renormalization groupQuantum gravitySpin connectionEffective actionGauge fixingMathematical physicsPhysics Letters B
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Aspects of D-brane Dynamics in Supergravity Backgrounds with Fluxes, Kappa-symmetry and Equations of Motion. Part IIB

2006

We derive and carry out a detailed analysis of the equations of motion of the type IIB D branes in generic supergravity backgrounds with fluxes making account of the worldvolume Born-Infeld gauge field and putting a special emphasis on the structure of the Dirac equation for Dp brane fermionic modes. We present an explicit form of the worldvolume field equations for each of the Dp branes (p=1,3,5,7,9) in the cases in which the Neveu-Schwarz flux and the Ramond-Ramond p-form flux along the Dp-brane worldvolume are zero and the supergravity backgrounds do not necessarily induce the worldvolume Born-Infeld flux. We then give several examples of D3, D5 and D7 brane configurations in which the w…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsInstantonCompactification (physics)SupergravityEquations of motionFOS: Physical sciencessymbols.namesakeHigh Energy Physics::TheoryClassical mechanicsHigh Energy Physics - Theory (hep-th)Mathematics::K-Theory and HomologyDirac equationsymbolsBrane cosmologyGauge theoryD-braneMathematical physics
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Planck scale physics and topology change through an exactly solvable model

2014

We consider the collapse of a charged radiation fluid in a Planck-suppressed quadratic extension of General Relativity (GR) formulated à la Palatini. We obtain exact analytical solutions that extend the charged Vaidya-type solution of GR, which allows to explore in detail new physics at the Planck scale. Starting from Minkowski space, we find that the collapsing fluid generates wormholes supported by the electric field. We discuss the relevance of our findings in relation to the quantum foam structure of space–time and the meaning of curvature divergences in this theory.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsModified gravityPlanck scaleTopology changeLibrary scienceFOS: Physical sciencesPlanck-scale physicsGeneral Relativity and Quantum Cosmology (gr-qc)Palatini formalismGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Dynamical Vaidya solutionsResearch councilFísica AplicadasymbolsPartial support
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