Search results for "Theoretical physics"

showing 10 items of 751 documents

Weight Systems from Feynman Diagrams

1996

We find that the overall UV divergences of a renormalizable field theory with trivalent vertices fulfil a four-term relation. They thus come close to establish a weight system. This provides a first explanation of the recent successful association of renormalization theory with knot theory.

High Energy Physics - TheoryAlgebra and Number TheoryAssociation (object-oriented programming)FOS: Physical sciencesMathematics::Geometric TopologyKnot theoryRenormalizationTheoretical physicssymbols.namesakeHigh Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Mathematics - Quantum AlgebrasymbolsFOS: MathematicsFeynman diagramQuantum Algebra (math.QA)Field theory (psychology)Relation (history of concept)Mathematics
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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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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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Constant-roll inflation: confrontation with recent observational data

2017

The previously proposed class of phenomenological inflationary models in which the assumption of inflaton slow-roll is replaced by the more general, constant-roll condition is compared with the most recent cosmological observational data, mainly the Planck ones. Models in this two-parametric class which remain viable appear to be close to the slow-roll ones, and their inflaton potentials are close to (but still different from) that of the natural inflation model. Permitted regions for the two model parameters are presented.

High Energy Physics - TheoryClass (set theory)Cosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesGeneral Physics and AstronomyModel parametersGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsGeneral Relativity and Quantum Cosmology0103 physical sciencesPlanck010306 general physicsPhysicsInflation (cosmology)010308 nuclear & particles physicsInflatonHigh Energy Physics - Theory (hep-th)symbolsObservational studyConstant (mathematics)Astrophysics - Cosmology and Nongalactic Astrophysics
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Mixing-induced spontaneous supersymmetry breaking

2010

It is conjectured that flavor mixing furnishes a universal mechanism for the spontaneous breaking of supersymmetry. The conjecture is proved explicitly for the mixing of two Wess--Zumino $\mathcal{N}=1$ supermultiplets and arguments for its general validity are given. The mechanism relies on the fact that, despite mixing treats fermions and bosons symmetrically, both the fermionic and the bosonic zero point energies are shifted by a positive amount and this kind of shift does not respect supersymmetry.

High Energy Physics - TheoryCondensed Matter::Quantum GasesPhysicsHigh Energy Physics::LatticeSpontaneous symmetry breakingHigh Energy Physics::PhenomenologyFOS: Physical sciencesGeneral Physics and AstronomySupersymmetrySupersymmetry breakingHigh Energy Physics - PhenomenologyHigh Energy Physics::TheoryExplicit symmetry breakingTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Quantum mechanicsSymmetry breakingQuantum field theoryChiral symmetry breakingMixing (physics)Physics Letters A
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Constraints on Cosmic Strings Using Data from the Third Advanced LIGO–Virgo Observing Run

2021

We search for gravitational-wave signals produced by cosmic strings in the Advanced LIGO and Virgo full O3 data set. Search results are presented for gravitational waves produced by cosmic string loop features such as cusps, kinks and, for the first time, kink-kink collisions.cA template-based search for short-duration transient signals does not yield a detection. We also use the stochastic gravitational-wave background energy density upper limits derived from the O3 data to constrain the cosmic string tension, $G\mu$, as a function of the number of kinks, or the number of cusps, for two cosmic string loop distribution models.cAdditionally, we develop and test a third model which interpolat…

High Energy Physics - TheoryDewey Decimal Classification::500 | Naturwissenschaften::550 | Geowissenschaftengravitational radiation: stochasticAstronomyCosmic stringsWAVESGeneral Physics and Astronomy01 natural sciencesGeneral Relativity and Quantum CosmologyCosmologyGravitation Cosmology & AstrophysicsGravitationLIMITSCosmic strings & domain wallCosmology & Astrophysicsddc:550Distribution modelsTransient signalenergy: densityLIGOQCstochastic modelLIGO Scientific CollaborationShort durationsCosmic strings & domain walls; Gravitational waves; Gravitation Cosmology & AstrophysicsQBPhysicsCosmic strings & domain wallskinkSettore FIS/03Stochastic systems[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thPhysicsGravitational effectsarticleGRAVITATIONAL-RADIATION; LIMITS; EVOLUTION; WAVEStensionGravitational-wave signalsCosmologyPhysical Sciencesastro-ph.COGrand unified theories[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational waveAstrophysics - Cosmology and Nongalactic AstrophysicsGravitational effects; Gravity waves; Stochastic models; Stochastic systems; Cosmic strings; Distribution models; Grand unified theories; Gravitational-wave signals; Orders of magnitude; Short durations; Template-based; Transient signalGravitationCosmology and Nongalactic Astrophysics (astro-ph.CO)gr-qcPhysics MultidisciplinaryGRAVITATIONAL-RADIATIONO3FOS: Physical sciencesContext (language use)General Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsPhysics and Astronomy(all)Gravity wavesGravitation and AstrophysicsGravitational wavesTheoretical physicsGeneral Relativity and Quantum Cosmologystatistical analysis0103 physical sciencesTemplate-basedCosmic Strings O3 LIGO Virgoddc:530010306 general physicscosmic stringSTFCInflation (cosmology)Science & Technology010308 nuclear & particles physicsGravitational wavestring tensionVirgogravitational radiation: backgroundRCUKLIGOEVOLUTIONCosmic stringStochastic modelsOrders of magnitudeVIRGOHigh Energy Physics - Theory (hep-th)Dewey Decimal Classification::500 | Naturwissenschaften::530 | Physik[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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QCD and Strongly Coupled Gauge Theories: Challenges and Perspectives

2014

We dedicate this document to the memory of Mikhail Polikarpov, who passed away in July 2013. Misha worked with us for decades as a convener of the “Confinement” section of the Quark Confinement and Hadron Spectrum Series. He guided and expanded the scientific discussion of that topic, inspiring and under taking new research avenues. From its initial conception, he supported the enterprise of this document and organized Sect. 8, writing the part on confinement himself. He attracted the XIth Conference on Quark Confinement and the Hadron Spectrum to St. Petersburg (September 8-12, 2014; see http://phys.spbu.ru/confxi.html). His warm and kind personality, his high sense of humor, his ideas in …

High Energy Physics - TheoryEFFECTIVE-FIELD-THEORYNuclear TheoryPhysics and Astronomy (miscellaneous)Physics beyond the Standard ModelReviewHEAVY-ION COLLISIONSnucl-ex7. Clean energyCosmologyHigh Energy Physics - ExperimentQUARK-GLUON PLASMADEEP-INELASTIC SCATTERINGHigh Energy Physics - Experiment (hep-ex)High Energy Physics - Phenomenology (hep-ph)[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]Gauge theoryNuclear Experiment (nucl-ex)Nuclear ExperimentQuantum chromodynamicsPhysics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thHigh Energy Physics - Lattice (hep-lat)hep-phddc:High Energy Physics - PhenomenologyYANG-MILLS THEORYastro-ph.COAstrophysics - Cosmology and Nongalactic AstrophysicsPB-PB COLLISIONSParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)nucl-th[PHYS.NUCL]Physics [physics]/Nuclear Theory [nucl-th]530 PhysicsStrong interactionComplex systemFOS: Physical scienceshep-lat[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]CHIRAL PERTURBATION-THEORY114 Physical sciencesELECTRIC-DIPOLE MOMENTNuclear Theory (nucl-th)Theoretical physicsHigh Energy Physics - Latticeddc:530Engineering (miscellaneous)Particle Physics - Phenomenologyhep-ex[PHYS.HLAT]Physics [physics]/High Energy Physics - Lattice [hep-lat]NUCLEUS-NUCLEUS COLLISIONSPerspective (graphical)FísicaRADIATIVE ENERGY-LOSSFlow (mathematics)High Energy Physics - Theory (hep-th)[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]European Physical Journal C
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Semiclassical geons at particle accelerators

2014

We point out that in certain four-dimensional extensions of general relativity constructed within the Palatini formalism stable self-gravitating objects with a discrete mass and charge spectrum may exist. The incorporation of nonlinearities in the electromagnetic field may effectively reduce their mass spectrum by many orders of magnitude. As a consequence, these objects could be within (or near) the reach of current particle accelerators. We provide an exactly solvable model to support this idea.

High Energy Physics - TheoryElectromagnetic fieldPhysicsGeneral relativityquantum black holesFOS: Physical sciencesSemiclassical physicsAstronomy and AstrophysicsParticle acceleratorGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum Cosmologylaw.inventionHigh Energy Physics - PhenomenologyFormalism (philosophy of mathematics)Theoretical physicsHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)lawMass spectrumWormholeWormholesGeon (physics)modified gravityJournal of Cosmology and Astroparticle Physics
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Ricci-Based Gravity theories and their impact on Maxwell and nonlinear electromagnetic models

2019

Abstract We extend the correspondence between metric-affine Ricci-Based Gravity the- ories and General Relativity (GR) to the case in which the matter sector is represented by linear and nonlinear electromagnetic fields. This complements previous studies focused on fluids and scalar fields. We establish the general algorithm that relates the matter fields in the GR and RBG frames and consider some applications. In particular, we find that the so-called Eddington-inspired Born-Infeld gravity theory coupled to Maxwell electromag- netism is in direct correspondence with GR coupled to Born-Infeld electromagnetism. We comment on the potential phenomenological implications of this relation.

High Energy Physics - TheoryElectromagnetic fieldPhysicsNuclear and High Energy PhysicsGravity (chemistry)010308 nuclear & particles physicsGeneral relativityScalar (physics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyNonlinear systemTheoretical physicsHigh Energy Physics - Theory (hep-th)Electromagnetism0103 physical sciencesBeyond Standard Modellcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityElectromagnetic model010306 general physicsClassical Theories of GravityGeneral algorithmJournal of High Energy Physics
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Cubic interactions of Maxwell-like higher spins

2017

We study the cubic vertices for Maxwell-like higher-spins in flat and (A)dS background spaces of any dimension. Reducibility of their free spectra implies that a single cubic vertex involving any three fields subsumes a number of couplings among different particles of various spins. The resulting vertices do not involve traces of the fields and in this sense are simpler than their Fronsdal counterparts. We propose an extension of both the free theory and of its cubic deformation to a more general class of partially reducible systems, that one can obtain from the original theory upon imposing trace constraints of various orders. The key to our results is a version of the Noether procedure al…

High Energy Physics - TheoryHigher Spin SymmetryPhysicsNuclear and High Energy PhysicsTransversalitySpins010308 nuclear & particles physicsFOS: Physical sciencesHigher Spin Gravity01 natural sciencesSpectral lineVertex (geometry)Settore FIS/02 - Fisica Teorica Modelli e Metodi Matematicisymbols.namesakeTheoretical physicsGauge Symmetry Higher Spin Gravity Higher Spin SymmetryHigh Energy Physics - Theory (hep-th)Gauge Symmetry0103 physical sciencessymbolslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityGauge Symmetry Higher Spin Gravity Higher Spin SymmetryNoether's theorem010306 general physics
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