Search results for "Affine"

showing 10 items of 183 documents

Observational effects of varying speed of light in quadratic gravity cosmological models

2017

We study different manifestations of the speed of light in theories of gravity where metric and connection are regarded as independent fields. We find that for a generic gravity theory in a frame with locally vanishing affine connection, the usual degeneracy between different manifestations of the speed of light is broken. In particular, the space-time causal structure constant ([Formula: see text]) may become variable in that local frame. For theories of the form [Formula: see text], this variation in [Formula: see text] has an impact on the definition of the luminosity distance (and distance modulus), which can be used to confront the predictions of particular models against Supernovae t…

PhysicsGravity (chemistry)Physics and Astronomy (miscellaneous)010308 nuclear & particles physicsFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Cosmological constantAffine connectionType (model theory)01 natural sciencesGeneral Relativity and Quantum Cosmology0103 physical sciencesSpeed of lightConnection (algebraic framework)010306 general physicsConstant (mathematics)Luminosity distanceMathematical physics
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Correspondence between modified gravity and general relativity with scalar fields

2018

We describe a novel procedure to map the field equations of nonlinear Ricci-based metric-affine theories of gravity, coupled to scalar matter described by a given Lagrangian, into the field equations of General Relativity coupled to a different scalar field Lagrangian. Our analysis considers examples with a single and $N$ real scalar fields, described either by canonical Lagrangians or by generalized functions of the kinetic and potential terms. In particular, we consider several explicit examples involving $f(R)$ theories and the Eddington-inspired Born-Infeld gravity model, coupled to different scalar field Lagrangians. We show how the nonlinearities of the gravitational sector of these t…

PhysicsHigh Energy Physics - TheoryGeneralized function010308 nuclear & particles physicsGeneral relativityScalar (mathematics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)CosmologicalKinetic energy01 natural sciencesGeneral Relativity and Quantum CosmologyRicci-based metric-affineAstrophysicalGravitationNonlinear systemGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Gravity model of tradeTheories of gravity0103 physical sciences010306 general physicsScalar fieldMathematical physicsPhysical Review D
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Generalized Ashtekar variables for Palatini f(R) models

2021

We consider special classes of Palatini f(R) theories, featured by additional Loop Quantum Gravity inspired terms, with the aim of identifying a set of modified Ashtekar canonical variables, which still preserve the SU(2) gauge structure of the standard theory. In particular, we allow for affine connection to be endowed with torsion, which turns out to depend on the additional scalar degree affecting Palatini f(R) gravity, and in this respect we successfully construct a novel Gauss constraint. We analyze the role of the additional scalar field, outlining as it acquires a dynamical character by virtue of a non vanishing Immirzi parameter, and we describe some possible effects on the area ope…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy Physics010308 nuclear & particles physicsImmirzi parameterGaussScalar (mathematics)FOS: Physical sciencesLoop quantum gravityGeneral Relativity and Quantum Cosmology (gr-qc)Affine connection01 natural sciencesGeneral Relativity and Quantum CosmologyAshtekar variablessymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)0103 physical sciencessymbolslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityEinstein010306 general physicsScalar fieldMathematical physics
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Observable traces of non-metricity: new constraints on metric-affine gravity

2018

Relaxing the Riemannian condition to incorporate geometric quantities such as torsion and non-metricity may allow to explore new physics associated with defects in a hypothetical space-time microstructure. Here we show that non-metricity produces observable effects in quantum fields in the form of 4-fermion contact interactions, thereby allowing us to constrain the scale of non-metricity to be greater than 1 TeV by using results on Bhabha scattering. Our analysis is carried out in the framework of a wide class of theories of gravity in the metric-affine approach. The bound obtained represents an improvement of several orders of magnitude to previous experimental constraints.

PhysicsHigh Energy Physics - TheoryNuclear and High Energy Physics010308 nuclear & particles physicsScatteringPhysics beyond the Standard ModelFOS: Physical sciencesTorsion (mechanics)ObservableGeneral Relativity and Quantum Cosmology (gr-qc)16. Peace & justice01 natural scienceslcsh:QC1-999General Relativity and Quantum CosmologyGravitationTheoretical physicsClassical mechanicsHigh Energy Physics - Theory (hep-th)0103 physical sciencesNuclear and High Energy Physics; theories of gravity; geometric quantitiesAffine transformation010306 general physicsQuantumlcsh:Physics
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Ghosts in metric-affine higher order curvature gravity

2019

We disprove the widespread belief that higher order curvature theories of gravity in the metric-affine formalism are generally ghost-free. This is clarified by considering a sub-class of theories constructed only with the Ricci tensor and showing that the non-projectively invariant sector propagates ghost-like degrees of freedom. We also explain how these pathologies can be avoided either by imposing a projective symmetry or additional constraints in the gravity sector. Our results put forward that higher order curvature gravity theories generally remain pathological in the metric-affine (and hybrid) formalisms and highlight the key importance of the projective symmetry and/or additional co…

PhysicsHigh Energy Physics - TheoryPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsFOS: Physical scienceslcsh:AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (physics)Curvature01 natural sciencesRotation formalisms in three dimensionsGeneral Relativity and Quantum CosmologyFormalism (philosophy of mathematics)Theoretical physicsHigh Energy Physics - Theory (hep-th)0103 physical scienceslcsh:QB460-466lcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityAffine transformationProjective test010306 general physicsEngineering (miscellaneous)Ricci curvatureEuropean Physical Journal C: Particles and Fields
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Scattering amplitudes in affine gravity

2020

Affine gravity is a connection-based formulation of gravity that does not involve a metric. After a review of basic properties of affine gravity, we compute the tree-level scattering amplitude of scalar particles interacting gravitationally via the connection in a curved spacetime. We find that, while classically equivalent to general relativity, affine gravity differs from metric quantum gravity.

PhysicsHigh Energy Physics - TheorySpacetime010308 nuclear & particles physicsGeneral relativityScalar (physics)FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyScattering amplitudeHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)0103 physical sciencesQuantum gravityAffine transformation010306 general physicsMathematical physicsPhysical Review
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Anisotropic deformations in a class of projectively-invariant metric-affine theories of gravity

2020

Among the general class of metric-affine theories of gravity, there is a special class conformed by those endowed with a projective symmetry. Perhaps the simplest manner to realise this symmetry is by constructing the action in terms of the symmetric part of the Ricci tensor. In these theories, the connection can be solved algebraically in terms of a metric that relates to the spacetime metric by means of the so-called deformation matrix that is given in terms of the matter fields. In most phenomenological applications, this deformation matrix is assumed to inherit the symmetries of the matter sector so that in the presence of an isotropic energy-momentum tensor, it respects isotropy. In th…

PhysicsPhysics and Astronomy (miscellaneous)Spacetime010308 nuclear & particles physicsIsotropyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Invariant (physics)16. Peace & justiceSpecial class01 natural sciencesGeneral Relativity and Quantum CosmologyTheoretical physics0103 physical sciencesHomogeneous spaceAffine transformationAnisotropy010303 astronomy & astrophysicsRicci curvatureClassical and Quantum Gravity
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On Chiral Quantum Superspaces

2011

We give a quantum deformation of the chiral Minkowski superspace in 4 dimensions embedded as the big cell into the chiral conformal superspace. Both deformations are realized as quantum homogeneous superspaces: we deform the ring of regular functions together with a coaction of the corresponding quantum supergroup.

PhysicsRing (mathematics)High Energy Physics::LatticeConformal mapSupersymmetryQUANTUM GROUPSSuperspaceGeneral Relativity and Quantum CosmologyHigh Energy Physics::TheoryTheoretical physicsNonlinear Sciences::Exactly Solvable and Integrable SystemsMathematics::Quantum AlgebraQuantum mechanicsMinkowski spaceAffine varietySUPERSYMMETRYSupergroupQuantum
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Affine camera calibration from homographies of parallel planes

2010

This paper deals with the problem of retrieving the affine structure of a scene from two or more images of parallel planes. We propose a new approach that is solely based on plane homographies, calculated from point correspondences, and that does not require the recovery of the 3D structure of the scene. Neither vanishing points nor lines need to be extracted from the images. The case of a moving camera with constant intrinsic parameters and the one of cameras with possibly different parameters are both addressed. Extensive experiments with both synthetic and real images have validated our approach.

Pixelbusiness.industryComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISIONIterative reconstructionReal imagePlane (Unicode)Computer Science::Computer Vision and Pattern RecognitionPoint (geometry)Computer visionAffine transformationArtificial intelligenceVanishing pointbusinessCamera resectioningMathematics2010 IEEE International Conference on Image Processing
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Uniform estimates for the X-ray transform restricted to polynomial curves

2012

We establish near-optimal mixed-norm estimates for the X-ray transform restricted to polynomial curves with a weight that is a power of the affine arclength. The bounds that we establish depend only on the spatial dimension and the degree of the polynomial. Some of our results are new even in the well-curved case.

Polynomial curvesPolynomialX-ray transformMixed normDegree (graph theory)Mathematical analysisMixed normPower (physics)Affine arclengthDimension (vector space)Mathematics - Classical Analysis and ODEsClassical Analysis and ODEs (math.CA)FOS: MathematicsRestricted X-rayAffine transformation42B25Generalized Radon transformAnalysisMathematicsJournal of Functional Analysis
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