Search results for "quantum gravity"

showing 10 items of 126 documents

T and CPT Symmetries in Entangled Neutral Meson Systems

2011

Genuine tests of an asymmetry under T and/or CPT transformations imply the interchange between in-states and out-states. I explain a methodology to perform model-indepedent separate measurements of the three CP, T and CPT symmetry violations for transitions involving the decay of the neutral meson systems in B- and {\Phi}-factories. It makes use of the quantum-mechanical entanglement only, for which the individual state of each neutral meson is not defined before the decay of its orthogonal partner. The final proof of the independence of the three asymmetries is that no other theoretical ingredient is involved and that the event sample corresponding to each case is different from the other …

High Energy Physics - TheoryPhysicsHistoryParticle physicsMesonCPT symmetrymedia_common.quotation_subjectFOS: Physical sciencesQuantum entanglementState (functional analysis)Function (mathematics)AsymmetryOmegaComputer Science ApplicationsEducationHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Quantum gravityHigh Energy Physics::Experimentmedia_common
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Bimetric truncations for quantum Einstein gravity and asymptotic safety

2010

In the average action approach to the quantization of gravity the fundamental requirement of "background independence" is met by actually introducing a background metric but leaving it completely arbitrary. The associated Wilsonian renormalization group defines a coarse graining flow on a theory space of functionals which, besides the dynamical metric, depend explicitly on the background metric. All solutions to the truncated flow equations known to date have a trivial background field dependence only, namely via the classical gauge fixing term. In this paper we analyze a number of conceptual issues related to the bimetric character of the gravitational average action and explore a first no…

High Energy Physics - TheoryPhysicsAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantGeneral Relativity and Quantum CosmologyRenormalizationGravitationHigh Energy Physics - Theory (hep-th)Quantum gravityBackground independenceCosmological constant problemMathematical physicsGauge fixingAnnals of Physics
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Asymptotic Safety in Quantum Einstein Gravity: Nonperturbative Renormalizability and Fractal Spacetime Structure

2007

The asymptotic safety scenario of Quantum Einstein Gravity, the quantum field theory of the spacetime metric, is reviewed and it is argued that the theory is likely to be nonperturbatively renormalizable. It is also shown that asymptotic safety implies that spacetime is a fractal in general, with a fractal dimension of 2 on sub-Planckian length scales.

PhysicsPhysics::General PhysicsQuantum field theory in curved spacetimeAsymptotic safety in quantum gravityCausal setsStationary spacetimeHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyClassical mechanicsLinearized gravityQuantum gravityBackground independenceMathematical physicsFractal cosmology
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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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Searches for Physics Beyond the Standard Model

2015

Despite its phenomenal success, the Standard Model is not expected to be a complete description of nature all the way up to the Planck scale where quantum gravity comes into play. As the collider at the current energy frontier, the LHC is in a unique position to look for signals of physics beyond the Standard Model. In this chapter, results from the first run of the LHC are surveyed that go beyond the supersymmetric extension of the Standard Model discussed in the previous chapter. At the time of writing, no evidence for new phenomena has been discovered. Instead, the LHC experiments have constrained the parameter space of conceivable models significantly. The most prominent results are on …

PhysicsGauge bosonParticle physicsExtra dimensionsLarge Hadron ColliderPhysics beyond the Standard ModelQuantum gravityLeptoquarkSupersymmetryStandard Model
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Standard and Z2-Regge theory in two dimensions

1998

Abstract We qualitatively compare two versions of quantum Regge calculus by means of Monte Carlo simulations. In Standard Regge Calculus the quadratic link lengths of the triangulation vary continuously, whereas in the Z2-Regge Model they are restricted to two possible values. The goal is to determine whether the computationally more easily accessible Z2 model retains the characteristics of standard Regge theory.

Nuclear and High Energy PhysicsHigh Energy Physics::LatticeHigh Energy Physics::PhenomenologyMonte Carlo methodTriangulation (social science)Regge calculusAtomic and Molecular Physics and OpticsRegge theoryHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyQuadratic equationQuantum electrodynamicsQuantum gravityHigh Energy Physics::ExperimentStatistical physicsLink (knot theory)QuantumMathematicsNuclear Physics B - Proceedings Supplements
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A new functional flow equation for Einstein-Cartan quantum gravity

2015

We construct a special-purpose functional flow equation which facilitates non-perturbative renormalization group (RG) studies on theory spaces involving a large number of independent field components that are prohibitively complicated using standard methods. Its main motivation are quantum gravity theories in which the gravitational degrees of freedom are carried by a complex system of tensor fields, a prime example being Einstein-Cartan theory, possibly coupled to matter. We describe a sequence of approximation steps leading from the functional RG equation of the Effective Average Action to the new flow equation which, as a consequence, is no longer fully exact on the untruncated theory sp…

PhysicsHigh Energy Physics - TheoryField (physics)Immirzi parameterAsymptotic safety in quantum gravityGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Action (physics)General Relativity and Quantum CosmologyTensor fieldFlow (mathematics)High Energy Physics - Theory (hep-th)Quantum gravityTensorMathematical physics
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Einstein-Cartan gravity, Asymptotic Safety, and the running Immirzi parameter

2013

In this paper we analyze the functional renormalization group flow of quantum gravity on the Einstein-Cartan theory space. The latter consists of all action functionals depending on the spin connection and the vielbein field (co-frame) which are invariant under both spacetime diffeomorphisms and local frame rotations. In the first part of the paper we develop a general methodology and corresponding calculational tools which can be used to analyze the flow equation for the pertinent effective average action for any truncation of this theory space. In the second part we apply it to a specific three-dimensional truncated theory space which is parametrized by Newton's constant, the cosmological…

PhysicsHigh Energy Physics - TheorySpacetimeImmirzi parameterAsymptotic safety in quantum gravityFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantRenormalization groupGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Quantum gravityFunctional renormalization groupSpin connection
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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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Insensitivity of Hawking radiation to an invariant Planck-scale cutoff

2009

A disturbing aspect of Hawking's derivation of black hole radiance is the need to invoke extreme conditions for the quantum field that originates the emitted quanta. It is widely argued that the derivation requires the validity of the conventional relativistic field theory to arbitrarily high, trans-Planckian scales. We stress in this note that this is not necessarily the case if the question is presented in a covariant way. We point out that Hawking radiation is immediately robust against an invariant Planck-scale cutoff. This important feature of Hawking radiation is relevant for a quantum gravity theory that preserves, in some way, the Lorentz symmetry.

PhysicsNuclear and High Energy PhysicsQuantum field theory in curved spacetime010308 nuclear & particles physicsBlack hole information paradoxFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Lorentz covariance01 natural sciencesGeneral Relativity and Quantum CosmologyPartícules (Física nuclear)Black holeTheoretical physicsHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyQuantum mechanics0103 physical sciencesQuantum gravityCovariant transformationFísica nuclearQuantum field theory010306 general physicsHawking radiation
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