Search results for "Modified gravity"

showing 9 items of 19 documents

Planck scale physics and topology change through an exactly solvable model

2014

We consider the collapse of a charged radiation fluid in a Planck-suppressed quadratic extension of General Relativity (GR) formulated à la Palatini. We obtain exact analytical solutions that extend the charged Vaidya-type solution of GR, which allows to explore in detail new physics at the Planck scale. Starting from Minkowski space, we find that the collapsing fluid generates wormholes supported by the electric field. We discuss the relevance of our findings in relation to the quantum foam structure of space–time and the meaning of curvature divergences in this theory.

High Energy Physics - TheoryPhysicsNuclear and High Energy PhysicsModified gravityPlanck scaleTopology changeLibrary scienceFOS: Physical sciencesPlanck-scale physicsGeneral Relativity and Quantum Cosmology (gr-qc)Palatini formalismGeneral Relativity and Quantum Cosmologysymbols.namesakeTheoretical physicsGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Dynamical Vaidya solutionsResearch councilFísica AplicadasymbolsPartial support
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On gravitational waves in Born-Infeld inspired non-singular cosmologies

2017

We study the evolution of gravitational waves for non-singular cosmological solutions within the framework of Born-Infeld inspired gravity theories, with special emphasis on the Eddington-inspired Born-Infeld theory. We review the existence of two types of non-singular cosmologies, namely bouncing and asymptotically Minkowski solutions, from a perspective that makes their features more apparent. We study in detail the propagation of gravitational waves near these non-singular solutions and carefully discuss the origin and severity of the instabilities and strong coupling problems that appear. We also investigate the role of the adiabatic sound speed of the matter sector in the regularisatio…

High Energy Physics - Theorycosmological modelCosmology and Nongalactic Astrophysics (astro-ph.CO)[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]FOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmology[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th][ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]GravitationTheoretical physicsGeneral Relativity and Quantum CosmologyBorn–Infeld modelgravitational radiation: propagation0103 physical sciencesMinkowski spacestrong couplingphysics of the early universeMinkowski010306 general physicsAdiabatic processmodified gravityPhysics010308 nuclear & particles physicsGravitational waveNon singular[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Astronomy and Astrophysicsalternatives to inflationstabilityvelocity: acousticBorn-Infeld modelregularizationHigh Energy Physics - Theory (hep-th)gravitationRegularization (physics)adiabaticStrong coupling[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]primordial gravitational waves (theory)[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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Cosmological data analysis of f(R) gravity models

2009

A class of well-behaved modified gravity models with long enough matter domination epoch and a late-time accelerated expansion is confronted with SNIa, CMB, SDSS, BAO and H(z) galaxy ages data, as well as current measurements of the linear growth of structure. We show that the combination of geometrical probes and growth data exploited here allows to rule out f(R) gravity models, in particular, the logarithmic of curvature model. We also apply solar system tests to the models in agreement with the cosmological data. We find that the exponential of the inverse of the curvature model satisfies all the observational tests considered and we derive the allowed range of parameters. Current data s…

PhysicsGravity (chemistry)Cosmology and Nongalactic Astrophysics (astro-ph.CO)Cosmological parameters from LSSLogarithmCosmic microwave backgroundFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCurvatureGalaxyLinear perturbation theoryExponential functionsymbols.namesakeTheoretical physicssymbolsAstronomiaf(R) gravityModified GravityEinsteinAstrophysics - Cosmology and Nongalactic Astrophysics
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Nonsingular Black Holes in $f(R)$ Theories

2015

We study the structure of a family of static, spherically symmetric space-times generated by an anisotropic fluid and governed by a particular type of $f(R)$ theory. We find that for a range of parameters with physical interest, such solutions represent black holes with the central singularity replaced by a finite size wormhole. We show that time-like geodesics and null geodesics with nonzero angular momentum never reach the wormhole throat due to an infinite potential barrier. For null radial geodesics, it takes an infinite affine time to reach the wormhole. This means that the resulting space-time is geodesically complete and, therefore, nonsingular despite the generic existence of curvat…

PhysicsHigh Energy Physics - TheoryAngular momentumGeodesicNull (mathematics)General Physics and AstronomyFOS: Physical sciencesnonsingular black holesGeneral Relativity and Quantum Cosmology (gr-qc)Type (model theory)CurvaturewormholesGeneral Relativity and Quantum Cosmologylaw.inventionGeneral Relativity and Quantum CosmologySingularityInvertible matrixHigh Energy Physics - Theory (hep-th)lawWormholemodified gravityMathematical physics
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Rotating black holes in Eddington-inspired Born-Infeld gravity: an exact solution

2020

We find an exact, rotating charged black hole solution within Eddington-inspired Born-Infeld gravity. To this end we employ a recently developed correspondence or {\it mapping} between modified gravity models built as scalars out of contractions of the metric with the Ricci tensor, and formulated in metric-affine spaces (Ricci-Based Gravity theories) and General Relativity. This way, starting from the Kerr-Newman solution, we show that this mapping bring us the axisymmetric solutions of Eddington-inspired Born-Infeld gravity coupled to a certain model of non-linear electrodynamics. We discuss the most relevant physical features of the solutions obtained this way, both in the spherically sym…

PhysicsHigh Energy Physics - TheoryGravity (chemistry)Modified gravityFísica-Modelos matemáticos010308 nuclear & particles physicsGeneral relativityRotational symmetryFOS: Physical sciencesAstronomy and AstrophysicsGR black holesGeneral Relativity and Quantum Cosmology (gr-qc)Charged black hole01 natural sciencesGravitational-wave astronomyGeneral Relativity and Quantum CosmologyTheoretical physicsGeneral Relativity and Quantum CosmologyExact solutions in general relativityHigh Energy Physics - Theory (hep-th)0103 physical sciencesMetric (mathematics)Física matemáticaWormholesRicci curvature
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The virial theorem and the dark matter problem in hybrid metric-Palatini gravity

2012

Hybrid metric-Palatini gravity is a recently proposed theory, consisting of the superposition of the metric Einstein-Hilbert Lagrangian with an f(R) term constructed a la Palatini. The theory predicts the existence of a long-range scalar field, which passes the Solar System observational constraints, even if the scalar field is very light, and modifies the cosmological and galactic dynamics. Thus, the theory opens new possibilities to approach, in the same theoretical framework, the problems of both dark energy and dark matter. In this work, we consider the generalized virial theorem in the scalar-tensor representation of the hybrid metric-Palatini gravity. More specifically, taking into ac…

Physicsdark matter theory010308 nuclear & particles physicsDark matterVelocity dispersionFOS: Physical sciencesAstronomy and AstrophysicsVirial massAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesPotential energyGeneral Relativity and Quantum CosmologyVirial theoremTheoretical physicsGeneral Relativity and Quantum CosmologyPhysics - General PhysicsGeneral Physics (physics.gen-ph)Gravitational field0103 physical sciencesDark energygalaxy clusters010303 astronomy & astrophysicsScalar fieldmodified gravity
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Noncanonical approaches to inflation

2019

El paradigma inflacionario provee al Modelo Cosmológico Estándar de un mecanismo que fácilmente resuelve los problemas del horizonte y la planicie y, al mismo tiempo, produce las semillas primordiales que se dieron lugar a las estructuras que hoy vemos en el cielo. Independientemente de la naturaleza precisa del mecanismo, la inflación cosmológica consiste en una etapa de aceleración durante el universo primitivo que sucedió momentos después del big bang. En esta Tesis, cubrimos aproximaciones fenomenológicas y teóricas sobre el estudio de la inflación: desde parametrizaciones independientes de modelos a modificaciones de las leyes de gravedad. Está dividida en cuatro partes. La primera, co…

UNESCO::CIENCIAS DE LA TIERRA Y DEL ESPACIO::Ciencias del espacio:CIENCIAS DE LA TIERRA Y DEL ESPACIO::Ciencias del espacio [UNESCO]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Gravitacióninflationcosmologymodified gravity:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Gravitación [UNESCO]early universe
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Cosmologie des théories de gravite modifiées

2017

The study of physical cosmology has reached an exciting era. For the first time in human history, a quantitative model for the formation and the evolution of the Universe exists, which explains a wide range of phenomena and has been tested with incredible accuracy during the last century. Moreover, weare approaching a time when a bounty of high quality cosmological data will be available,allowing us to use cosmology as a tool to test fundamental physics.In particular, as the large-scale structures of the Universe are governed by gravity, cosmology can help us to asses the correctness of Albert Einstein’s general relativity. This idea fueledmost of the work described in this manuscript,in wh…

[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Modified gravity[PHYS.ASTR.CO] Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Gravite modifiéeLarge scale structureCosmologieCosmologyStructure grand echelle
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Black Holes, Geons, and Singularities in Metric-Affine Gravity

2016

Uno de los problemas abiertos en la descripción de la gravedad es la existencia de singularidades. Las geometrías singulares se caracterizan por geodésicas incompletas, lo que físicamente se corresponde con observadores que desaparecen del espacio-tiempo, o que aparecen de la nada. Múltiples extensiones de la Relatividad General tratan de resolver este problema de algún modo. Por ello, en esta tesis estudio modificaciones al Lagrangiano de Relatividad General, tales como gravedad cuadrática y gravedad de Born-Infeld, en el formalismo Métrico-Afín. En este formalismo, la conexión (de la cual se derivan los tensores de curvatura) se considera independiente de la métrica, y permitimos que sea …

geonquadratic gravityUNESCO::FÍSICAblack holessingularityborn-infeldquantum gravity:FÍSICA [UNESCO]palatiniwormholegeneral relativitywave scatteringmodified gravitygeodesics
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