Search results for "Theories"

showing 10 items of 302 documents

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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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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Implications of nonplanar dual conformal symmetry

2018

Recently, Bern et al observed that a certain class of next-to-planar Feynman integrals possess a bonus symmetry that is closely related to dual conformal symmetry. It corresponds to a projection of the latter along a certain lightlike direction. Previous studies were performed at the level of the loop integrand, and a Ward identity for the integral was formulated. We investigate the implications of the symmetry at the level of the integrated quantities. In particular, we focus on the phenomenologically important case of five-particle scattering. The symmetry simplifies the four-variable problem to a three-variable one. In the context of the recently proposed space of pentagon functions, the…

High Energy Physics - TheoryNuclear and High Energy PhysicsFunction spaceFeynman graphFOS: Physical sciencesanomalyContext (language use)Ward identitySpace (mathematics)Conformal and W Symmetry01 natural sciencesProjection (linear algebra)Identity (mathematics)High Energy Physics - Phenomenology (hep-ph)Conformal symmetry0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. RadioactivityAnomalies in Field and String Theories010306 general physicsScattering AmplitudesParticle Physics - PhenomenologyMathematical physicsPhysicsloop integral010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thscattering amplitudehep-phSymmetry (physics)Loop (topology)High Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)symmetry: conformalsupersymmetry: 4[PHYS.HPHE]Physics [physics]/High Energy Physics - Phenomenology [hep-ph]lcsh:QC770-798dualityParticle Physics - Theoryinfrared problem
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A non-perturbative study of massive gauge theories

2013

We consider a non-perturbative formulation of an SU(2) massive gauge theory on a space-time lattice, which is also a discretised gauged non-linear chiral model. The lattice model is shown to have an exactly conserved global SU(2) symmetry. If a scaling region for the lattice model exists and the lightest degrees of freedom are spin one vector particles with the same quantum numbers as the conserved current, we argue that the most general effective theory describing their low-energy dynamics must be a massive gauge theory. We present results of a exploratory numerical simulation of the model and find indications for the presence of a scaling region where both a triplet vector and a scalar re…

High Energy Physics - TheoryNuclear and High Energy PhysicsHiggs PhysicsHigh Energy Physics::Latticehep-latFOS: Physical sciences01 natural sciencesTheoretical physicsHigh Energy Physics - LatticeHigh Energy Physics - Phenomenology (hep-ph)Lattice (order)0103 physical sciencesEffective field theoryGauge theory010306 general physicsConserved currentScalingLattice Gauge Field TheoriesPhysics010308 nuclear & particles physicshep-thHigh Energy Physics - Lattice (hep-lat)Físicahep-phQuantum numberHigh Energy Physics - PhenomenologyChiral modelHigh Energy Physics - Theory (hep-th)Gauge SymmetryNon-perturbativeSigma Models
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Testing freeze-in with axial and vector Z′ bosons

2021

The freeze-in production of Feebly Interacting Massive Particle (FIMP) dark matter in the early universe is an appealing alternative to the well-known - and constrained - Weakly Interacting Massive Particle (WIMP) paradigm. Although challenging, the phenomenology of FIMP dark matter has been receiving growing attention and is possible in a few scenarios. In this work, we contribute to this endeavor by considering a $Z^\prime$ portal to fermionic dark matter, with the $Z^\prime$ having both vector and axial couplings and a mass ranging from MeV up to PeV. We evaluate the bounds on both freeze-in and freeze-out from direct detection, atomic parity violation, leptonic anomalous magnetic moment…

High Energy Physics - TheoryNuclear and High Energy PhysicsParticle physicsCosmology and Nongalactic Astrophysics (astro-ph.CO)media_common.quotation_subjectDark matterMassive particleFOS: Physical sciencesContext (language use)QC770-7987. Clean energy01 natural sciencesPartícules (Física nuclear)law.inventionHigh Energy Physics - Phenomenology (hep-ph)WIMPlawNuclear and particle physics. Atomic energy. Radioactivity0103 physical sciencesBeam dump010306 general physicsmedia_commonBosonHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsCosmologia010308 nuclear & particles physicsCosmology of Theories beyond the SMUniverse3. Good healthHigh Energy Physics - PhenomenologyHigh Energy Physics - Theory (hep-th)Beyond Standard ModelAstrophysics - High Energy Astrophysical PhenomenaPhenomenology (particle physics)Astrophysics - Cosmology and Nongalactic AstrophysicsJournal of High Energy Physics
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