Search results for "gravity"

showing 10 items of 537 documents

First-order flows and stabilisation equations for non-BPS extremal black holes

2011

28 páginas.-- This article is distributed under the terms of the Creative Commons Attribution Noncommercial License.

PhysicsHigh Energy Physics - TheorySupergravity modelsNuclear and High Energy Physics010308 nuclear & particles physicsSupergravityFOS: Physical sciencesCharge (physics)Black holes in string theoryFirst order01 natural sciencesGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryHigh Energy Physics - Theory (hep-th)Flow (mathematics)Harmonic functionPhysics::Plasma Physics0103 physical sciences010306 general physicsMathematical physicsAnsatzJournal of High Energy Physics
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Finite Quantum Gravity Amplitudes: No Strings Attached

2020

We study the gravity-mediated scattering of scalar fields based on a parameterisation of the Lorentzian quantum effective action. We demonstrate that the interplay of infinite towers of spin zero and spin two poles at imaginary squared momentum leads to scattering amplitudes that are compatible with unitarity bounds, causal, and scale-free at trans-Planckian energy. Our construction avoids introducing non-localities or the massive higher-spin particles that are characteristic in string theory.

PhysicsHigh Energy Physics - TheoryUnitarityScatteringScalar (physics)General Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)String theory01 natural sciencesGeneral Relativity and Quantum CosmologyScattering amplitudeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum mechanics0103 physical sciencesQuantum gravityHigh Energy Physics010306 general physicsQuantumEffective actionPhysical Review Letters
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RG flows of Quantum Einstein Gravity in the linear-geometric approximation

2014

We construct a novel Wetterich-type functional renormalization group equation for gravity which encodes the gravitational degrees of freedom in terms of gauge-invariant fluctuation fields. Applying a linear-geometric approximation the structure of the new flow equation is considerably simpler than the standard Quantum Einstein Gravity construction since only transverse-traceless and trace part of the metric fluctuations propagate in loops. The geometric flow reproduces the phase-diagram of the Einstein-Hilbert truncation including the non-Gaussian fixed point essential for Asymptotic Safety. Extending the analysis to the polynomial $f(R)$-approximation establishes that this fixed point come…

PhysicsHigh Energy Physics - Theory; High Energy Physics - Theory; General Relativity and Quantum CosmologyHigh Energy Physics - TheoryEntropic gravityGeneral relativityAsymptotic safety in quantum gravityGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Euclidean quantum gravityGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyClassical mechanicsHigh Energy Physics - Theory (hep-th)Linearized gravityTheoretical High Energy PhysicsComputingMethodologies_DOCUMENTANDTEXTPROCESSINGQuantum gravitySemiclassical gravityf(R) gravityAnnals of Physics
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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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Remarks on the reduced phase space of -dimensional gravity on a torus in the Ashtekar formulation

1998

We examine the reduced phase space of the Barbero-Varadarajan solutions of the Ashtekar formulation of (2 + 1)-dimensional general relativity on a torus. We show that it is a finite-dimensional space due to the existence of an infinite-dimensional residual gauge invariance which reduces the infinite-dimensional space of solutions to a finite-dimensional space of gauge-inequivalent solutions. This is in agreement with general arguments which imply that the number of physical degrees of freedom for (2 + 1)-dimensional Ashtekar gravity on a torus is finite.

PhysicsHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyGravity (chemistry)Physics and Astronomy (miscellaneous)General relativityPhase spaceDegrees of freedom (physics and chemistry)TorusGauge theorySpace (mathematics)ResidualMathematical physicsClassical and Quantum Gravity
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Gravitational waves in Fully Constrained Formulation in a dynamical spacetime with matter content

2011

We analyze numerically the behaviour of the hyperbolic sector of the Fully Constrained Formulation (FCF) (Bonazzola et al. 2004). The numerical experiments allow us to be confident in the performances of the upgraded version of the CoCoNuT code (Dimmelmeier et al. 2005) by replacing the Conformally Flat Condition (CFC), an approximation of Einstein equations, by FCF. First gravitational waves in FCF in a dynamical spacetime with matter content will be shown.

PhysicsHistoryCode (set theory)Hyperbolic sectorSpacetime010308 nuclear & particles physicsGravitational wave01 natural sciencesComputer Science ApplicationsEducationClassical mechanicsLinearized gravity0103 physical sciencesContent (measure theory)Einstein equations010303 astronomy & astrophysicsJournal of Physics: Conference Series, 314, id. 012078 (2011).
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Loop quantum gravity and Planck-size black hole entropy

2007

The Loop Quantum Gravity (LQG) program is briefly reviewed and one of its main applications, namely the counting of black hole entropy within the framework is considered. In particular, recent results for Planck size black holes are reviewed. These results are consistent with an asymptotic linear relation (that fixes uniquely a free parameter of the theory) and a logarithmic correction with a coefficient equal to -1/2. The account is tailored as an introduction to the subject for non-experts.

PhysicsHistoryLogarithmFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Loop quantum gravityLinear-quadratic-Gaussian controlGeneral Relativity and Quantum CosmologyComputer Science ApplicationsEducationsymbols.namesakeTheoretical physicsGeneral Relativity and Quantum CosmologysymbolsLinear relationPlanckBlack hole thermodynamicsFree parameter
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Dynamics for a simple graph using the U(N) framework for loop quantum gravity

2012

The implementation of the dynamics in loop quantum gravity (LQG) is still an open problem. Here, we discuss a tentative dynamics for the simplest class of graphs in LQG: Two vertices linked with an arbitrary number of edges. We find an interesting global U(N) symmetry in this model that selects the homogeneous/isotropic sector. Then, we propose a quantum Hamiltonian operator for this reduced sector. Finally, we introduce the spinor representation for LQG in order to propose a classical effective dynamics for this model.

PhysicsHistorySpinorOpen problemFOS: Physical sciencesLoop quantum gravityGeneral Relativity and Quantum Cosmology (gr-qc)Linear-quadratic-Gaussian controlGeneral Relativity and Quantum CosmologySymmetry (physics)Computer Science ApplicationsEducationTheoretical physicsComputer Science::Systems and ControlQuantum gravityddc:530Representation (mathematics)Quantum
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BARYOGENESIS IN SUPERGRAVITY INFLATIONARY MODELS

1985

Abstract Realistic N=1 supergravity theories with a gravitino mass of order 1 TeV require a period of inflation to dilute the gravitino abundance. Moreover, if the gravitino is unstable the reheat temperature is bounded to be no greater than O(108 GeV). We show that such models may still have acceptable rates of baryosynthesis and discuss possible mechanisms.

PhysicsInflation (cosmology)Nuclear and High Energy PhysicsParticle physicsSupergravityAstrophysics::High Energy Astrophysical PhenomenaHigh Energy Physics::PhenomenologyFísicaFeynman graphBaryogenesisGeneral Relativity and Quantum CosmologyBounded functionCP violationGravitinoHigh Energy Physics::ExperimentGeneral Theoretical Physics
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Black hole state counting in loop quantum gravity: a number-theoretical approach

2008

4 pages, 1 figure.-- PACS nrs.: 04.70.Dy, 04.60.Pp.-- ArXiv pre-print available at: http://arxiv.org/abs/0802.4077

PhysicsMatemáticasAstrophysics::High Energy Astrophysical PhenomenaImmirzi parameterGeneral Physics and AstronomyFOS: Physical sciencesFísicaLoop quantum gravityGeneral Relativity and Quantum Cosmology (gr-qc)Mathematical Physics (math-ph)General Relativity and Quantum CosmologyBlack holeTheoretical physicsMicro black holeGeneral Relativity and Quantum CosmologyClassical mechanicsExtremal black hole[PACS] Quantum aspects of black holes evaporation thermodynamicsVirtual black holeBlack hole thermodynamics[PACS] Loop quantum gravity quantum geometry spin foamsMathematical PhysicsBlack hole complementarity
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