Search results for "THEORIE"

showing 10 items of 354 documents

Matter Dependence of the Four-Loop Cusp Anomalous Dimension

2019

We compute analytically the matter-dependent contributions to the quartic Casimir term of the four-loop light-like cusp anomalous dimension in QCD, with $n_f$ fermion and $n_s$ scalar flavours. The result is extracted from the double pole of a scalar form factor. We adopt a new strategy for the choice of master integrals with simple analytic and infrared properties, which significantly simplifies our calculation. To this end we first identify a set of integrals whose integrands have a dlog form, and are hence expected to have uniform transcendental weight. We then perform a systematic analysis of the soft and collinear regions of loop integration and build linear combinations of integrals w…

High Energy Physics - Theory530 PhysicsHigh Energy Physics::LatticeScalar (mathematics)FOS: Physical sciencesGeneral Physics and Astronomy10192 Physics Institute01 natural sciencessymbols.namesakeHigh Energy Physics - Phenomenology (hep-ph)Feynman diagrams Form factors Perturbation theory Perturbative QCD Quantum field theory Scattering amplitudes Supersymmetric field theoriesQuartic function0103 physical sciencesFeynman diagramQuantum field theory010306 general physicsLinear combinationMathematical physicsQuantum chromodynamicsPhysics010308 nuclear & particles physicsPropagatorPerturbative QCD3100 General Physics and AstronomyHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)symbolsPhysical Review Letters
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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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Flavour mixing transport theory and resonant leptogenesis

2021

We derive non-equilibrium quantum transport equations for flavour-mixing fermions. We develop the formalism mostly in the context of resonant leptogenesis with two mixing Majorana fermions and one lepton flavour, but our master equations are valid more generally in homogeneous and isotropic systems. We give a hierarchy of quantum kinetic equations, valid at different approximations, that can accommodate helicity and arbitrary mass differences. In the mass-degenerate limit the equations take the familiar form of density matrix equations. We also derive the semiclassical Boltzmann limit of our equations, including the CP-violating source, whose regulator corresponds to the flavour coherence d…

High Energy Physics - TheoryDensity matrixNuclear and High Energy PhysicsCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesSemiclassical physicsQC770-798hiukkasfysiikkakosmologia01 natural sciences114 Physical sciencesHigh Energy Physics - Phenomenology (hep-ph)Nuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesMaster equationThermal Field Theory010306 general physicscosmology of theories beyond the SMMixing (physics)Mathematical physicsPhysicsThermal quantum field theory010308 nuclear & particles physicsHigh Energy Physics::PhenomenologyFermionCosmology of Theories beyond the SMthermal field theory3. Good healthHigh Energy Physics - PhenomenologyMAJORANACP violationHigh Energy Physics - Theory (hep-th)LeptogenesisAstrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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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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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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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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Brane-world and loop cosmology from a gravity–matter coupling perspective

2015

We show that the effective brane-world and the loop quantum cosmology background expansion histories can be reproduced from a modified gravity perspective in terms of an $f(R)$ gravity action plus a $g(R)$ term non-minimally coupled with the matter Lagrangian. The reconstruction algorithm that we provide depends on a free function of the matter density that must be specified in each case and allows to obtain analytical solutions always. In the simplest cases, the function $f(R)$ is quadratic in the Ricci scalar, $R$, whereas $g(R)$ is linear. Our approach is compared with recent results in the literature. We show that working in the Palatini formalism there is no need to impose any constrai…

High Energy Physics - TheoryModified gravityNuclear and High Energy Physicsf(R) theoriesFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Palatini formalismGeneral Relativity and Quantum CosmologyCosmologyGeneral Relativity and Quantum Cosmologysymbols.namesakeQuadratic equationGravity–matter couplingLoop quantum cosmologyMathematical physicsPhysicsReconstruction algorithmlcsh:QC1-999High Energy Physics - Theory (hep-th)Quadratic cosmologysymbolsf(R) gravityBranelcsh:PhysicsLagrangianScalar curvaturePhysics Letters B
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Efficient resummation of high post-Newtonian contributions to the binding energy

2021

A factorisation property of Feynman diagrams in the context the Effective Field Theory approach to the compact binary problem has been recently employed to efficiently determine the static sector of the potential at fifth post-Newtonian (5PN) order. We extend this procedure to the case of non-static diagrams and we use it to fix, by means of elementary algebraic manipulations, the value of more than one thousand diagrams at 5PN order, that is a substantial fraction of the diagrams needed to fully determine the dynamics at 5PN. This procedure addresses the redundancy problem that plagues the computation of the binding energy with respect to more "efficient" observables like the scattering an…

High Energy Physics - TheoryNuclear and High Energy PhysicsBlack HolesComputationFOS: Physical sciencesBinary numberContext (language use)General Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesake0103 physical sciencesEffective field theoryFeynman diagramlcsh:Nuclear and particle physics. Atomic energy. RadioactivityStatistical physicsAlgebraic numberResummation010306 general physicsPhysics010308 nuclear & particles physicsEffective Field TheoriesObservableHigh Energy Physics - Theory (hep-th)symbolslcsh:QC770-798Classical Theories of GravityJournal of High Energy Physics
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Hairy black-holes in shift-symmetric theories

2020

Scalar hair of black holes in theories with a shift symmetry are constrained by the no-hair theorem of Hui and Nicolis, assuming spherical symmetry, time-independence of the scalar field and asymptotic flatness. The most studied counterexample is a linear coupling of the scalar with the Gauss-Bonnet invariant. However, in this case the norm of the shift-symmetry current $J^2$ diverges at the horizon casting doubts on whether the solution is physically sound. We show that this is not an issue since $J^2$ is not a scalar quantity, since $J^\mu$ is not a diff-invariant current in the presence of Gauss-Bonnet. The same theory can be written in Horndeski form with a non-analytic function $G_5 \s…

High Energy Physics - TheoryNuclear and High Energy PhysicsBlack HolesCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyGeneral Relativity and Quantum Cosmology0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsPhysical quantityMathematical physicsPhysics010308 nuclear & particles physicsScalar (physics)Black HoleInvariant (physics)Linear couplingSettore FIS/02 - Fisica Teorica Modelli e Metodi MatematiciHigh Energy Physics - Theory (hep-th)astro-ph.COlcsh:QC770-798Circular symmetryScalar fieldClassical Theories of GravityAstrophysics - Cosmology and Nongalactic AstrophysicsCounterexample
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Matter dependence of the four-loop QCD cusp anomalous dimension: from small angles to all angles

2019

We compute the fermionic contributions to the cusp anomalous dimension in QCD at four loops as an expansion for small cusp angle. As a byproduct we also obtain the respective terms of the four-loop HQET wave function anomalous dimension. Our new results at small angles provide stringent tests of a recent conjecture for the exact angle dependence of the matter terms in the four-loop cusp anomalous dimension. We find that the conjecture does not hold for two of the seven fermionic color structures, but passes all tests for the remaining terms. This provides strong support for the validity of the corresponding conjectured expressions with full angle dependence. Taking the limit of large Minkow…

High Energy Physics - TheoryNuclear and High Energy PhysicsConformal anomalyFOS: Physical sciencesConformal map01 natural sciencesTheoretical physicsHigh Energy Physics - Phenomenology (hep-ph)Dimension (vector space)Perturbative QCD0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityScattering Amplitudes010306 general physicsWave functionQuantum chromodynamicsCusp (singularity)Physics010308 nuclear & particles physicsPerturbative QCDEffective Field TheoriesWilson ’t Hooft and Polyakov loopsScattering amplitudeHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)lcsh:QC770-798Journal of High Energy Physics
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