Search results for "quantum gravity"

showing 10 items of 126 documents

From Big Bang to Asymptotic de Sitter: Complete Cosmologies in a Quantum Gravity Framework

2005

Using the Einstein-Hilbert approximation of asymptotically safe quantum gravity we present a consistent renormalization group based framework for the inclusion of quantum gravitational effects into the cosmological field equations. Relating the renormalization group scale to cosmological time via a dynamical cutoff identification this framework applies to all stages of the cosmological evolution. The very early universe is found to contain a period of ``oscillatory inflation'' with an infinite sequence of time intervals during which the expansion alternates between acceleration and deceleration. For asymptotically late times we identify a mechanism which prevents the universe from leaving t…

High Energy Physics - TheoryBig BangInflation (cosmology)Physicsmedia_common.quotation_subjectAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsRenormalization groupAstrophysicsUniverseGravitationGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)De Sitter universeQuantum gravityQuantumMathematical physicsmedia_common
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Massless positivity in graviton exchange

2021

We formulate Positivity Bounds for scattering amplitudes including exchange of massless particles. We generalize the standard construction through dispersion relations to include the presence of a branch cut along the real axis in the complex plane for the Maldestam variable $s$. In general, validity of these bounds require the cancellation of divergences in the forward limit of the amplitude, proportional to $t^{-1}$ and $\log(t)$. We show that this is possible in the case of gravitons if one assumes a Regge behavior of the amplitude at high energies below the Planck scale, as previously suggested in the literature, and that the concrete UV behaviour of the amplitude is uniquely determined…

High Energy Physics - TheoryField (physics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)hiukkasfysiikkakosmologia01 natural sciencesGeneral Relativity and Quantum CosmologyGravitationeffective field theorycanonical quantum gravityDispersion relation0103 physical sciencessironta010306 general physicsquantum field theoryperturbation theoryMathematical physicsPhysics010308 nuclear & particles physicsGravitonFísicagravitaatioDark Energyalternative gravity theoriesBimetric Theoriesscattering amplitudesMassless particleScattering amplitudeAmplitudeHigh Energy Physics - Theory (hep-th)Complex planeGravitation
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Einstein, Planck and Vera Rubin: Relevant Encounters Between the Cosmological and the Quantum Worlds

2021

In Cosmology and in Fundamental Physics there is a crucial question like: where the elusive substance that we call Dark Matter is hidden in the Universe and what is it made of? that, even after 40 years from the Vera Rubin seminal discovery [1] does not have a proper answer. Actually, the more we have investigated, the more this issue has become strongly entangled with aspects that go beyond the established Quantum Physics, the Standard Model of Elementary particles and the General Relativity and related to processes like the Inflation, the accelerated expansion of the Universe and High Energy Phenomena around compact objects. Even Quantum Gravity and very exotic Dark Matter particle candid…

High Energy Physics - TheoryGeneral Physics and AstronomyNature of dark matter01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologyClassical vs quantum cosmologyHigh Energy Physics - Phenomenology (hep-ph)010303 astronomy & astrophysicsQuantumMathematical PhysicsQuantum gravity and cosmologyPhysicsModification of general relativityChaplygin Gaslcsh:QC1-999CosmologyHigh Energy Physics - PhenomenologyExpansion of the UniversesymbolsGeneral RelativityGeneral relativityMaterials Science (miscellaneous)BiophysicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Metric expansion of spacesymbols.namesakeTheory of relativitySettore FIS/05 - Astronomia e Astrofisica0103 physical sciencesDark matterddc:530Cosmological ModelsPhysical and Theoretical ChemistryPlanckEinsteindark matter; galaxies; nature of dark matter; beyond standard model; modification of general relativity; quantum gravity and cosmology; expansion of the Universe010308 nuclear & particles physicsFísicaGalaxiesAstrophysics - Astrophysics of GalaxiesCosmosEpistemologyHigh Energy Physics - Theory (hep-th)quantum gravityAstrophysics of Galaxies (astro-ph.GA)Quantum gravityBeyond standard modellcsh:Physics
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Do we Observe Quantum Gravity Effects at Galactic Scales?

2005

The nonperturbative renormalization group flow of Quantum Einstein Gravity (QEG) is reviewed. It is argued that there could be strong renormalization effects at large distances, in particular a scale dependent Newton constant, which mimic the presence of dark matter at galactic and cosmological scales.

High Energy Physics - TheoryGravity (chemistry)High Energy Physics::LatticeDark matterFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsGeneral Relativity and Quantum CosmologyRenormalizationsymbols.namesakeGeneral Relativity and Quantum CosmologyEinsteinQuantumPhysicsAstrophysics (astro-ph)General EngineeringAstronomy and AstrophysicsHigh Energy Physics - Theory (hep-th)Space and Planetary ScienceQuantum electrodynamicsScale dependentsymbolsQuantum gravityConstant (mathematics)
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Palatini actions and quantum gravity phenomenology

2011

We show that an invariant an universal length scale can be consistently introduced in a generally covariant theory through the gravitational sector using the Palatini approach. The resulting theory is able to capture different aspects of quantum gravity phenomenology in a single framework. In particular, it is found that in this theory field excitations propagating with different energy-densities perceive different background metrics, which is a fundamental characteristic of the DSR and Rainbow Gravity approaches. We illustrate these properties with a particular gravitational model and explicitly show how the soccer ball problem is avoided in this framework. The isotropic and anisotropic cosmol…

High Energy Physics - TheoryLength scalePhysicsFOS: Physical sciencesAstronomy and AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (physics)General Relativity and Quantum CosmologyGravitationTheoretical physicsGeneral Relativity and Quantum CosmologySingularityHigh Energy Physics - Theory (hep-th)Quantum gravityCovariant transformationPhenomenology (particle physics)Big Bounce
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A minimal length from the cutoff modes in asymptotically safe quantum gravity

2005

Within asymptotically safe Quantum Einstein Gravity (QEG), the quantum 4-sphere is discussed as a specific example of a fractal spacetime manifold. The relation between the infrared cutoff built into the effective average action and the corresponding coarse graining scale is investigated. Analyzing the properties of the pertinent cutoff modes, the possibility that QEG generates a minimal length scale dynamically is explored. While there exists no minimal proper length, the QEG sphere appears to be "fuzzy" in the sense that there is a minimal angular separation below which two points cannot be resolved by the cutoff modes.

High Energy Physics - TheoryLength scalePhysicsNuclear and High Energy PhysicsSpacetimeFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyManifoldAction (physics)Proper lengthClassical mechanicsHigh Energy Physics - Theory (hep-th)Quantum gravityCutoffQuantumJournal of High Energy Physics
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Quantum gravitational decoherence from fluctuating minimal length and deformation parameter at the Planck scale

2020

Schemes of gravitationally induced decoherence are being actively investigated as possible mechanisms for the quantum-to-classical transition. Here, we introduce a decoherence process due to quantum gravity effects. We assume a foamy quantum spacetime with a fluctuating minimal length coinciding on average with the Planck scale. Considering deformed canonical commutation relations with a fluctuating deformation parameter, we derive a Lindblad master equation that yields localization in energy space and decoherence times consistent with the currently available observational evidence. Compared to other schemes of gravitational decoherence, we find that the decoherence rate predicted by our mo…

High Energy Physics - TheoryLength scaleQuantum decoherenceScienceQuantum physicsGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Quantum spacetime01 natural sciencesGeneral Relativity and Quantum CosmologyArticleGeneral Biochemistry Genetics and Molecular BiologyGravitation0103 physical sciencesMaster equation010306 general physicsQuantumCondensed Matter - Statistical MechanicsPhysicsMesoscopic physicsMultidisciplinaryStatistical Mechanics (cond-mat.stat-mech)010308 nuclear & particles physicsQGeneral ChemistryClassical mechanicsHigh Energy Physics - Theory (hep-th)Quantum gravityQuantum Physics (quant-ph)Theoretical physics
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Born-Infeld f(R) gravity

2014

Motivated by the properties of matter quantum fields in curved space-times, we work out a gravity theory that combines the Born-Infeld gravity Lagrangian with an $f(R)$ piece. To avoid ghost-like instabilities, the theory is formulated within the Palatini approach. This construction provides more freedom to address a number of important questions such as the dynamics of the early universe and the cosmic accelerated expansion, among others. In particular, we consider the effect that adding an $f(R)=a R^2$ term has on the early-time cosmology. We find that bouncing solutions are robust against these modifications of the Lagrangian whereas the solutions with {\it loitering} behavior of the ori…

High Energy Physics - TheoryNuclear and High Energy PhysicsGravity (chemistry)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Борна-Инфельда теория гравитации модифицированнаяmedia_common.quotation_subjectFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyCosmologyкосмологияGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)De Sitter universeBorn–Infeld modelmedia_commonPhysicsквантовая гравитацияFunction (mathematics)UniverseHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Quantum gravityf(R) gravityF(R)-гравитацияквантовые поляAstrophysics - Cosmology and Nongalactic Astrophysics
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U(N) tools for loop quantum gravity: the return of the spinor

2011

We explore the classical setting for the U(N) framework for SU(2) intertwiners for loop quantum gravity (LQG) and describe the corresponding phase space in terms of spinors with appropriate constraints. We show how its quantization leads back to the standard Hilbert space of intertwiner states defined as holomorphic functionals. We then explain how to glue these intertwiners states in order to construct spin network states as wave-functions on the spinor phase space. In particular, we translate the usual loop gravity holonomy observables to our classical framework. Finally, we propose how to derive our phase space structure from an action principle which induces non-trivial dynamics for the…

High Energy Physics - TheoryPhysics and Astronomy (miscellaneous)FOS: Physical sciencesLoop quantum gravityGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesake0103 physical sciences010306 general physicsWave functionMathematical PhysicsMathematical physicsPhysicsSpinor010308 nuclear & particles physicsHilbert spaceObservableMathematical Physics (math-ph)High Energy Physics - Theory (hep-th)Phase spacePhysical Sciencessymbols[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Quantum gravitySpin network
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The metric on field space, functional renormalization, and metric-torsion quantum gravity

2015

Searching for new non-perturbatively renormalizable quantum gravity theories, functional renormalization group (RG) flows are studied on a theory space of action functionals depending on the metric and the torsion tensor, the latter parameterized by three irreducible component fields. A detailed comparison with Quantum Einstein-Cartan Gravity (QECG), Quantum Einstein Gravity (QEG), and "tetrad-only" gravity, all based on different theory spaces, is performed. It is demonstrated that, over a generic theory space, the construction of a functional RG equation (FRGE) for the effective average action requires the specification of a metric on the infinite-dimensional field manifold as an addition…

High Energy Physics - TheoryPhysics010308 nuclear & particles physicsAsymptotic safety in quantum gravityGeneral Physics and AstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Renormalization group01 natural sciencesGeneral Relativity and Quantum CosmologyRenormalizationGeneral Relativity and Quantum CosmologyTorsion tensorHigh Energy Physics - Theory (hep-th)0103 physical sciencesQuantum gravityFunctional renormalization group010306 general physicsQuantumIrreducible componentMathematical physics
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