Search results for "THEORIE"

showing 10 items of 354 documents

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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The moduli spaces of S-fold CFTs

2019

An S-fold has played an important role in constructing supersymmetric field theories with interesting features. It can be viewed as a type of AdS_4 solutions of Type IIB string theory where the fields in overlapping patches are glued by elements of SL(2,Z). This paper examines three dimensional quiver theories that arise from brane configurations with an inclusion of the S-fold. An important feature of such a quiver is that it contains a link, which is the T(U(N)) theory, between two U(N) groups, along with bifundamental and fundamental hypermultiplets. We systematically study the moduli spaces of those quiver theories, including the cases in which the non-zero Chern-Simons levels are turne…

High Energy Physics - TheoryNuclear and High Energy PhysicsPure mathematicsSettore FIS/02 - Fisica Teorica Modelli E Metodi MatematiciBrane Dynamics in Gauge TheoriesStructure (category theory)FOS: Physical sciencesString theory01 natural sciencesSupersymmetric Gauge TheoryHigh Energy Physics::Theory0103 physical scienceslcsh:Nuclear and particle physics. Atomic energy. Radioactivity010306 general physicsPhysics010308 nuclear & particles physicsQuiverSupersymmetryModuli spaceBrane Dynamics in Gauge Theories Duality in Gauge Field Theories Supersymmetric Gauge Theory Supersymmetry and DualityHigh Energy Physics - Theory (hep-th)Supersymmetric gauge theorySupersymmetry and Dualitylcsh:QC770-798Anti-de Sitter spaceBraneDuality in Gauge Field TheoriesJournal of High Energy Physics
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Wilson Loop Form Factors: A New Duality

2017

We find a new duality for form factors of lightlike Wilson loops in planar $\mathcal N=4$ super-Yang-Mills theory. The duality maps a form factor involving an $n$-sided lightlike polygonal super-Wilson loop together with $m$ external on-shell states, to the same type of object but with the edges of the Wilson loop and the external states swapping roles. This relation can essentially be seen graphically in Lorentz harmonic chiral (LHC) superspace where it is equivalent to planar graph duality. However there are some crucial subtleties with the cancellation of spurious poles due to the gauge fixing. They are resolved by finding the correct formulation of the Wilson loop and by careful analyti…

High Energy Physics - TheoryNuclear and High Energy PhysicsWilson loopgauge fixingHigh Energy Physics::LatticeFOS: Physical sciencesDuality (optimization)Type (model theory)Superspace01 natural sciencesSuperspacesspace: EuclideanGeneral Relativity and Quantum CosmologyWilson loopQuantum mechanics0103 physical sciencesMinkowski spacelcsh:Nuclear and particle physics. Atomic energy. RadioactivityMinkowskiScattering Amplitudes010306 general physicssuperspaceMathematical physicsGauge fixingPhysicsform factor010308 nuclear & particles physicsEuclidean space[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]hep-thAnalytic continuationWilsonLoop (topology)chiralCERN LHC CollHigh Energy Physics - Theory (hep-th)’t Hooft and Polyakov loopslcsh:QC770-798dualitysupersymmetryParticle Physics - TheoryDuality in Gauge Field TheoriesLorentz
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Brane cosmology with an anisotropic bulk

2004

In the context of brane cosmology, a scenario where our universe is a 3+1-dimensional surface (the ``brane'') embedded in a five-dimensional spacetime (the ``bulk''), we study geometries for which the brane is anisotropic - more specifically Bianchi I - though still homogeneous. We first obtain explicit vacuum bulk solutions with anisotropic three-dimensional spatial slices. The bulk is assumed to be empty but endowed with a negative cosmological constant. We then embed Z_2-symmetric branes in the anisotropic spacetimes and discuss the constraints on the brane energy-momentum tensor due to the five-dimensional anisotropic geometry. We show that if the bulk is static, an anisotropic brane ca…

High Energy Physics - TheoryNuclear and High Energy Physicsmedia_common.quotation_subjectFOS: Physical sciencesContext (language use)Perfect fluidGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantAstrophysics01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum Cosmology0103 physical sciencesBrane cosmologyTensor010306 general physicsmedia_commonPhysicsSpacetimeExtra Large Dimensions010308 nuclear & particles physics[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Astrophysics (astro-ph)Cosmology of Theories beyond the SMUniverseHigh Energy Physics - Theory (hep-th)Brane
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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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What is a singular black hole beyond general relativity?

2017

Exploring the characterization of singular black hole spacetimes, we study the relation between energy density, curvature invariants, and geodesic completeness using a quadratic $f(R)$ gravity theory coupled to an anisotropic fluid. Working in a metric-affine approach, our models and solutions represent minimal extensions of General Relativity (GR) in the sense that they rapidly recover the usual Reissner-Nordstr\"{o}m solution from near the inner horizon outwards. The anisotropic fluid helps modify only the innermost geometry. Depending on the values and signs of two parameters on the gravitational and matter sectors, a breakdown of the correlations between the finiteness/divergence of the…

High Energy Physics - TheoryPhysicsMODIFIED THEORIES OF GRAVITY010308 nuclear & particles physicsGeneral relativityCiencias FísicasFOS: Physical sciences//purl.org/becyt/ford/1.3 [https]General Relativity and Quantum Cosmology (gr-qc)COSMIC CENSORSHIPOtras Ciencias Físicas01 natural sciencesCLASSICAL BLACK HOLESGeneral Relativity and Quantum Cosmology//purl.org/becyt/ford/1 [https]General Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)EINSTEIN-MAXWELL SPACETIMEQuantum mechanics0103 physical sciences010306 general physicsHumanitiesCIENCIAS NATURALES Y EXACTASPhysical Review D
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Born-Infeld gravity and its functional extensions

2014

We investigate the dynamics of a family of functional extensions of the (Eddington-inspired) Born-Infeld gravity theory, constructed with the inverse of the metric and the Ricci tensor. We provide a generic formal solution for the connection and an Einstein-like representation for the metric field equations of this family of theories. For particular cases we consider applications to the early-time cosmology and find that non-singular universes with a cosmic bounce are very generic and robust solutions.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsFOS: Physical sciencesClassical field theoryRicci flowGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyClassical unified field theoriesTheoretical physicsEinstein tensorsymbols.namesakeHigh Energy Physics - Theory (hep-th)Born–Infeld modelsymbolsRicci decompositionf(R) gravityRicci curvaturePhysical Review D
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