Search results for "GRAVITY"

showing 10 items of 537 documents

The two-loop five-particle amplitude in $\mathcal{N}=8$ supergravity

2019

We compute for the first time the two-loop five-particle amplitude in $\mathcal{N}=8$ supergravity. Starting from the known integrand, we perform an integration-by-parts reduction and express the answer in terms of uniform weight master integrals. The latter are known to evaluate to non-planar pentagon functions, described by a 31-letter symbol alphabet. We express the final result for the amplitude in terms of uniform weight four symbols, multiplied by a small set of rational factors. The amplitude satisfies the expected factorization properties when one external graviton becomes soft, and when two external gravitons become collinear. We verify that the soft divergences of the amplitude ex…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsPure mathematics010308 nuclear & particles physicsSupergravityFOS: Physical sciencesFunction (mathematics)01 natural sciencesSmall setScattering amplitudeAmplitudeFactorizationHigh Energy Physics - Theory (hep-th)0103 physical scienceslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityLimit (mathematics)010306 general physicsScattering AmplitudesSupergravity ModelsN=8 Supergravity
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Q7-branes and their coupling to IIB supergravity

2007

We show how, by making use of a new basis of the IIB supergravity axion-dilaton coset, SL(2,R)/SO(2), 7-branes that belong to different conjugacy classes of the duality group SL(2,R) naturally couple to IIB supergravity with appropriate source terms characterized by an SL(2,R) charge matrix Q. The conjugacy classes are determined by the value of the determinant of Q. The (p,q) 7-branes are the branes in the conjugacy class detQ = 0. The 7-branes in the conjugacy class detQ > 0 are labelled by three numbers (p,q,r) which parameterize the matrix Q and will be called Q7-branes. We construct the full bosonic Wess--Zumino term for the Q7-branes. In order to realize a gauge invariant coupling …

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsPure mathematicsSupergravityFOS: Physical sciencesMONOPOLESInvariant (physics)p-branesBRANESFIELDSINSTANTONSABELIAN BORN-INFELDConjugacy classDOMAIN-WALLSHigh Energy Physics - Theory (hep-th)DUALITYD-branesBrane cosmologyCoset6 DIMENSIONS
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Scale-dependent metric and causal structures in Quantum Einstein Gravity

2006

Within the asymptotic safety scenario for gravity various conceptual issues related to the scale dependence of the metric are analyzed. The running effective field equations implied by the effective average action of Quantum Einstein Gravity (QEG) and the resulting families of resolution dependent metrics are discussed. The status of scale dependent vs. scale independent diffeomorphisms is clarified, and the difference between isometries implemented by scale dependent and independent Killing vectors is explained. A concept of scale dependent causality is proposed and illustrated by various simple examples. The possibility of assigning an "intrinsic length" to objects in a QEG spacetime is a…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsScale (ratio)SpacetimeAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyAction (physics)Causality (physics)Theoretical physicssymbols.namesakeHigh Energy Physics - Theory (hep-th)Metric (mathematics)symbolsEinsteinQuantumJournal of High Energy Physics
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Renormalization group improved gravitational actions: A Brans-Dicke approach

2003

A new framework for exploiting information about the renormalization group (RG) behavior of gravity in a dynamical context is discussed. The Einstein-Hilbert action is RG-improved by replacing Newton's constant and the cosmological constant by scalar functions in the corresponding Lagrangian density. The position dependence of $G$ and $\Lambda$ is governed by a RG equation together with an appropriate identification of RG scales with points in spacetime. The dynamics of the fields $G$ and $\Lambda$ does not admit a Lagrangian description in general. Within the Lagrangian formalism for the gravitational field they have the status of externally prescribed ``background'' fields. The metric sat…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsSpacetimeScalar (mathematics)FOS: Physical sciencesEnergy–momentum relationGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantRenormalization groupGeneral Relativity and Quantum CosmologyGravitationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Gravitational fieldQuantum mechanicsQuantum gravityMathematical physicsPhysical Review D
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Fractal Spacetime Structure in Asymptotically Safe Gravity

2005

Four-dimensional Quantum Einstein Gravity (QEG) is likely to be an asymptotically safe theory which is applicable at arbitrarily small distance scales. On sub-Planckian distances it predicts that spacetime is a fractal with an effective dimensionality of 2. The original argument leading to this result was based upon the anomalous dimension of Newton's constant. In the present paper we demonstrate that also the spectral dimension equals 2 microscopically, while it is equal to 4 on macroscopic scales. This result is an exact consequence of asymptotic safety and does not rely on any truncation. Contact is made with recent Monte Carlo simulations.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsSpacetimeTruncationMonte Carlo methodAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum Cosmologysymbols.namesakeClassical mechanicsFractalHigh Energy Physics - Theory (hep-th)symbolsEinsteinConstant (mathematics)Quantum
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D=11massless superparticle covariant quantization, pure spinor BRST charge and hidden symmetries

2007

We consider the covariant quantization of the D=11 massless superparticle (M0-brane) in the spinor moving frame or twistor-like Lorentz harmonics formulation. The action involves the set of 16 constrained 32 component Majorana spinors, the spinor Lorentz harmonics parametrizing (as homogeneous coordinates, modulo gauge symmetries) the celestial sphere S9. There presence allows us to separate covariantly the first and the second class constraints of the model. After taking into account the second class constraints by means of Dirac brackets and after further reducing the first class constraints algebra, the system is described in terms of a simple BRST charge associated to the d=1, n=16 supe…

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsSpinorPure spinorSupergravityFOS: Physical sciencesBRST quantizationCohomologyTwistor theoryHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)Quantum mechanicsCovariant transformationSupersymmetry algebraMathematical physicsNuclear Physics B
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Fluid membranes and2dquantum gravity

2011

We study the RG flow of two dimensional (fluid) membranes embedded in Euclidean D-dimensional space using functional RG methods based on the effective average action. By considering a truncation ansatz for the effective average action with both extrinsic and intrinsic curvature terms we derive a system of beta functions for the running surface tension, bending rigidity and Gaussian rigidity. We look for non-trivial fixed points but we find no evidence for a crumpling transition at $T\neq0$. Finally, we propose to identify the $D\rightarrow 0$ limit of the theory with two dimensional quantum gravity. In this limit we derive new beta functions for both cosmological and Newton's constants.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsStatistical Mechanics (cond-mat.stat-mech)GaussianAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Fixed pointGeneral Relativity and Quantum CosmologyRenormalizationSurface tensionsymbols.namesakePhysics - Statistical MechanicsHigh Energy Physics - Theory (hep-th)Quantum mechanicsEuclidean geometrysymbolsQuantum gravityHigh Energy Physics - Theory; High Energy Physics - Theory; Physics - Statistical Mechanics; General Relativity and Quantum CosmologyCondensed Matter - Statistical MechanicsAnsatzPhysical Review D
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Duality and Spontaneously Broken Supergravity in Flat Backgrounds

2002

It is shown that the super Higgs mechanism that occurs in a wide class of models with vanishing cosmological constant (at the classical level) is obtained by the gauging of a flat group which must be an electric subgroup of the duality group. If the residual massive gravitinos which occur in the partial supersymmetry breaking are BPS saturated, then the flat group is non abelian. This is so for all the models obtained by a Scherk-Schwarz supersymmetry breaking mechanism. If gravitinos occur in long multiplets, then the flat groups may be abelian. This is the case of supersymmetry breaking by string compactifications on an orientifold T^6/Z_2 with non trivial brane fluxes.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsSupergravityHigh Energy Physics::PhenomenologyFísicaDuality (optimization)FOS: Physical sciencesSupersymmetry breakingsymbols.namesakeTheoretical physicsHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)OrientifoldsymbolsGravitinoAbelian groupBraneHiggs mechanismParticle Physics - Theory
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N=2 Super-Higgs, N=1 Poincare' Vacua and Quaternionic Geometry

2002

In the context of N=2 supergravity we explain the occurrence of partial super-Higgs with vanishing vacuum energy and moduli stabilization in a model suggested by superstring compactifications on type IIB orientifolds with 3-form fluxes. The gauging of axion symmetries of the quaternionic manifold, together with the use of degenerate symplectic sections for special geometry, are the essential ingredients of the construction.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsSupergravityHigh Energy Physics::PhenomenologySuperstring theoryFOS: Physical sciencesContext (language use)Partícules (Física nuclear)ModuliHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)Homogeneous spaceHiggs bosonAxionMathematics::Symplectic GeometryParticle Physics - TheorySymplectic geometryMathematical physics
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Flow equation of quantum Einstein gravity in a higher-derivative truncation

2002

Motivated by recent evidence indicating that Quantum Einstein Gravity (QEG) might be nonperturbatively renormalizable, the exact renormalization group equation of QEG is evaluated in a truncation of theory space which generalizes the Einstein-Hilbert truncation by the inclusion of a higher-derivative term $(R^2)$. The beta-functions describing the renormalization group flow of the cosmological constant, Newton's constant, and the $R^2$-coupling are computed explicitly. The fixed point (FP) properties of the 3-dimensional flow are investigated, and they are confronted with those of the 2-dimensional Einstein-Hilbert flow. The non-Gaussian FP predicted by the latter is found to generalize to …

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsTruncationAsymptotic safety in quantum gravityFOS: Physical sciencesOrder (ring theory)Gaussian fixed pointGeneral Relativity and Quantum Cosmology (gr-qc)Fixed pointRenormalization groupCoupling (probability)General Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum gravityMathematical physicsPhysical Review D
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