Search results for "normalization"

showing 10 items of 632 documents

Entropy Production during Asymptotically Safe Inflation

2011

The Asymptotic Safety scenario predicts that the deep ultraviolet of Quantum Einstein Gravity is governed by a nontrivial renormalization group fixed point. Analyzing its implications for cosmology using renormalization group improved Einstein equations we find that it can give rise to a phase of inflationary expansion in the early Universe. Inflation is a pure quantum effect here and requires no inflaton field. It is driven by the cosmological constant and ends automatically when the renormalization group evolution has reduced the vacuum energy to the level of the matter energy density. The quantum gravity effects also provide a natural mechanism for the generation of entropy. It could eas…

High Energy Physics - TheoryAsymptotic safety in quantum gravityGeneral Physics and AstronomyFOS: Physical scienceslcsh:AstrophysicsCosmological constantAstrophysics::Cosmology and Extragalactic AstrophysicsTheoretical physicsGeneral Relativity and Quantum CosmologyVacuum energylcsh:QB460-466inflationlcsh:ScienceEntropy (arrow of time)PhysicsEntropy productionquantum gravity; Asymptotic Safety; inflationInflatonRenormalization grouplcsh:QC1-999High Energy Physics - Theory (hep-th)quantum gravityAsymptotic SafetyQuantum gravitylcsh:Qlcsh:PhysicsEntropy; Volume 13; Issue 1; Pages: 274-292
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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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Pair creation in electric fields, anomalies, and renormalization of the electric current

2018

We investigate the Schwinger pair production phenomena in spatially homogeneous strong electric fields. We first consider scalar QED in four-dimensions and discuss the potential ambiguity in the adiabatic order assignment for the electromagnetic potential required to fix the renormalization subtractions. We argue that this ambiguity can be solved by invoking the conformal anomaly when both electric and gravitational backgrounds are present. We also extend the adiabatic regularization method for spinor QED in two-dimensions and find consistency with the chiral anomaly. We focus on the issue of the renormalization of the electric current $\langle j^\mu \rangle$ generated by the created pairs.…

High Energy Physics - TheoryChiral anomalyPhysicsSpinor010308 nuclear & particles physicsHigh Energy Physics::LatticeConformal anomalyHigh Energy Physics::PhenomenologyFOS: Physical sciencesComputer Science::Digital Libraries01 natural sciencesRenormalizationTheoretical physicsPair productionHigh Energy Physics - Theory (hep-th)Regularization (physics)Electric field0103 physical sciences010306 general physicsAdiabatic processPhysical Review D
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The 1-loop effective potential for the Standard Model in curved spacetime

2018

The renormalisation group improved Standard Model effective potential in an arbitrary curved spacetime is computed to one loop order in perturbation theory. The loop corrections are computed in the ultraviolet limit, which makes them independent of the choice of the vacuum state and allows the derivation of the complete set of $\beta$-functions. The potential depends on the spacetime curvature through the direct non-minimal Higgs-curvature coupling, curvature contributions to the loop diagrams, and through the curvature dependence of the renormalisation scale. Together, these lead to significant curvature dependence, which needs to be taken into account in cosmological applications, which i…

High Energy Physics - TheoryDe Sitter spaceVacuum stateUNIVERSEfield theories in higher dimensionskosmologia01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & FieldsHigh Energy Physics - Phenomenology (hep-ph)INFLATIONRADIATIVE-CORRECTIONSGauge theoryELECTROWEAK VACUUMMathematical physicsPhysics02 Physical SciencesPhysicshep-thhiukkasfysiikan standardimalliRENORMALIZATION-GROUP EQUATIONShep-phSPONTANEOUS SYMMETRY-BREAKINGNuclear & Particles PhysicsHigh Energy Physics - PhenomenologyHIGGS MASSPhysical SciencesGAUGE-THEORIESMathematics::Differential GeometryNuclear and High Energy Physicsgr-qcFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Curvatureclassical theories of gravityGeneral Relativity and Quantum Cosmology0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivityfield theories in lower dimensions010306 general physics01 Mathematical SciencesInflation (cosmology)Science & TechnologySpacetimeSTABILITYta114010308 nuclear & particles physicsgravitaatioLoop (topology)High Energy Physics - Theory (hep-th)INTERACTING SCALAR FIELDlcsh:QC770-798Perturbation theory (quantum mechanics)Journal of High Energy 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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Tensor bounds on the hidden universe

2018

During single clock inflation, hidden fields (i.e. fields coupled to the inflaton only gravitationally) in their adiabatic vacua can ordinarily only affect observables through virtual effects. After renormalizing background quantities (fixed by observations at some pivot scale), all that remains are logarithmic runnings in correlation functions that are both Planck and slow roll suppressed. In this paper we show how a large number of hidden fields can partially compensate this suppression and generate a potentially observable running in the tensor two point function, consistently inferable courtesy of a large $N$ resummation. We detour to address certain subtleties regarding loop correction…

High Energy Physics - TheoryNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectCosmic microwave backgroundFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)ddc:500.201 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityTensorPlanck010306 general physicsmedia_commonPhysicsInflation (cosmology)Slow roll010308 nuclear & particles physicsScalar (physics)InflatonCosmology of Theories beyond the SMUniverseHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)symbolslcsh:QC770-798Renormalization Regularization and RenormalonsAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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Derivation of spontaneously broken gauge symmetry from the consistency of effective field theory I: Massive vector bosons coupled to a scalar field

2018

We revisit the problem of deriving local gauge invariance with spontaneous symmetry breaking in the context of an effective field theory. Previous derivations were based on the condition of tree-order unitarity. However, the modern point of view considers the Standard Model as the leading order approximation to an effective field theory. As tree-order unitarity is in any case violated by higher-order terms in an effective field theory, it is instructive to investigate a formalism which can be also applied to analyze higher-order interactions. In the current work we consider an effective field theory of massive vector bosons interacting with a massive scalar field. We impose the conditions o…

High Energy Physics - TheoryNuclear and High Energy PhysicsNuclear TheorySpontaneous symmetry breakingFOS: Physical sciences53001 natural sciencesRenormalizationNuclear Theory (nucl-th)Theoretical physicsHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)0103 physical sciencesEffective field theoryddc:530Gauge theory010306 general physicsGauge symmetryPhysicsCoupling constantUnitarity010308 nuclear & particles physicsHigh Energy Physics - Lattice (hep-lat)lcsh:QC1-999High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Scalar fieldlcsh:Physics
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Non-supersymmetric AdS6 and the swampland

2021

We discuss infinite families of non-supersymmetric AdS$_6$ solutions in Type IIB string theory. They are siblings of supersymmetric solutions which are associated with $(p,q)$ 5-brane webs and holographically dual to 5d SCFTs engineered by those brane webs. The non-supersymmetric backgrounds carry identical 5-brane charges and are connected to the supersymmetric ones by RG flows. We study the stability of the non-supersymmetric solutions, identifying perturbative and non-perturbative decay channels for all the backgrounds explicitly available. We also identify likely decay mechanisms for solutions that have not been constructed explicitly but may be expected to exist based on brane web cons…

High Energy Physics - TheoryNuclear and High Energy PhysicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciSuperstring VacuaFOS: Physical sciencesQC770-798domain wallAdS-CFT Correspondencestring model: Type IIB01 natural sciencesGauge-gravity correspondenceHigh Energy Physics::TheoryNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciences010306 general physicsAdS-CFT Correspondence Gauge-gravity correspondence Superstring Vacua Supersymmetry BreakingSupersymmetry Breaking[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]010308 nuclear & particles physicsbubbleComputer Science::Information RetrievalAdS-CFT Correspondence; Gauge-gravity correspondence; Superstring Vacua; Supersymmetry Breakingduality: holographystabilitydecay: nonperturbativeHigh Energy Physics - Theory (hep-th)renormalization group: flowD-brane: 5spin: 2Journal of High Energy Physics
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Revising the Predictions of Inflation for the Cosmic Microwave Background Anisotropies

2009

4 pages, 1 figure.-- PACS nrs.: 98.70.Vc; 11.10.Gh; 98.80.Cq.-- ArXiv pre-print available at: http://arxiv.org/abs/0901.0439

High Energy Physics - TheoryParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)Scalar (mathematics)Cosmic microwave backgroundFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)[PACS] Cosmic background radiations01 natural sciencesGeneral Relativity and Quantum CosmologySpectral lineRenormalizationHigh Energy Physics - Phenomenology (hep-ph)[PACS] Particle-theory and field-theory models of the early UniverseQuantum mechanics0103 physical sciencesQuantum field theory010306 general physicsPhysicsInflation (cosmology)010308 nuclear & particles physicsSpectral densityCMB cold spot3. Good healthHigh Energy Physics - Phenomenology[PACS] Renormalization in quantum field theoryHigh Energy Physics - Theory (hep-th)Astrophysics - Cosmology and Nongalactic AstrophysicsPhysical Review Letters
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Pinch Technique: Theory and Applications

2009

We review the theoretical foundations and the most important physical applications of the Pinch Technique (PT). This general method allows the construction of off-shell Green’s functions in non-Abelian gauge theories that are independent of the gauge-fixing parameter and satisfy ghost-free Ward identities. We first present the diagrammatic formulation of the technique in QCD, deriving, at one loop, the gauge independent gluon self-energy, quark–gluon vertex, and three-gluon vertex, together with their Abelian Ward identities. The generalization of the PT to theories with spontaneous symmetry breaking is carried out in detail, and the profound connection with the optical theorem and the disp…

High Energy Physics - TheoryParticle physicsSpontaneous symmetry breakingGluonsHigh Energy Physics::LatticeFOS: Physical sciencesGeneral Physics and AstronomyDynamical mass generationGauge-invarianceSchwinger–Dyson equationsRenormalizationTheoretical physicsQuantization (physics)symbols.namesakeHigh Energy Physics::TheoryHigh Energy Physics - Phenomenology (hep-ph)Non-Abelian gauge theoriesFeynman diagramGauge theoryGauge bosonsQuantum chromodynamicsPhysicsBackground field methodGreens functionsElectroweak interactionHigh Energy Physics::PhenomenologyFísicaHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)symbols
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