0000000000269419

AUTHOR

D. Bazeia

showing 5 related works from this author

Geodesically complete BTZ-type solutions of $2+1$ Born-Infeld gravity

2016

We study Born-Infeld gravity coupled to a static, nonrotating electric field in $2+1$ dimensions and find exact analytical solutions. Two families of such solutions represent geodesically complete, and hence nonsingular, spacetimes. Another family represents a point-like charge with a singularity at the center. Despite the absence of rotation, these solutions resemble the charged, rotating BTZ solution of General Relativity but with a richer structure in terms of horizons. The nonsingular character of the first two families turn out to be attached to the emergence of a wormhole structure on their innermost region. This seems to be a generic prediction of extensions of General Relativity for…

High Energy Physics - TheoryPhysicsPhysics and Astronomy (miscellaneous)010308 nuclear & particles physicsGeneral relativityDegrees of freedom (physics and chemistry)FOS: Physical sciencesCharge (physics)General Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyConnection (mathematics)General Relativity and Quantum CosmologySingularityHigh Energy Physics - Theory (hep-th)Born–Infeld model0103 physical sciencesHorizon (general relativity)Wormhole010306 general physicsMathematical physics
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Classical resolution of black hole singularities in arbitrary dimension

2015

A metric-affine approach is employed to study higher-dimensional modified gravity theories involving different powers and contractions of the Ricci tensor. It is shown that the field equations are \emph{always} second-order, as opposed to the standard metric approach, where this is only achieved for Lagrangians of the Lovelock type. We point out that this property might have relevant implications for the AdS/CFT correspondence in black hole scenarios. We illustrate these aspects by considering the case of Born-Infeld gravity in $d$ dimensions, where we work out exact solutions for electrovacuum configurations. Our results put forward that black hole singularities in arbitrary dimensions can…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy PhysicsWhite holeFOS: Physical sciencesBlack holeGravitationAdS/CFT correspondenceTheoretical physicsGeneral Relativity and Quantum CosmologyClassical mechanicsRotating black holeHigh Energy Physics - Theory (hep-th)Extremal black holeGravitational singularityRicci curvature
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Black holes in five-dimensional Palatinif(R)gravity and implications for the AdS/CFT correspondence

2014

We show that theories having second-order field equations in the context of higher-dimensional modified gravity are not restricted to the family of Lovelock Lagrangians, but can also be obtained if no a priori assumption on the relation between the metric and affine structures of space-time is made (the Palatini approach). We illustrate this fact by considering the case of Palatini $f(R)$ gravities in five dimensions. Our results provide an alternative avenue to explore new domains of the AdS/CFT correspondence without resorting to ad hoc quasitopological constructions.

PhysicsBlack holeGeneral Relativity and Quantum CosmologyNuclear and High Energy PhysicsAdS/CFT correspondenceGravity (chemistry)Metric (mathematics)A priori and a posteriorif(R) gravityContext (language use)Affine transformationMathematical physicsPhysical Review D
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Robustness of braneworld scenarios against tensorial perturbations

2015

Inspired by the peculiarities of the effective geometry of crystalline structures, we reconsider thick brane scenarios from a metric-affine perspective. We show that for a rather general family of theories of gravity, whose Lagrangian is an arbitrary function of the metric and the Ricci tensor, the background and scalar field equations can be written in first-order form, and tensorial perturbations have a non negative definite spectrum, which makes them stable under linear perturbations regardless of the form of the gravity Lagrangian. We find, in particular, that the tensorial zero modes are exactly the same as predicted by Einstein's theory regardless of the scalar field and gravitational…

PhysicsHigh Energy Physics - TheoryGravity (chemistry)Physics and Astronomy (miscellaneous)FOS: Physical sciencesPositive-definite matrixGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyGravitationsymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Metric (mathematics)symbolsBraneEinsteinScalar fieldRicci curvatureMathematical physics
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Small and hollow magnetic monopoles

2018

We deal with the presence of magnetic monopoles in a non Abelian model that generalizes the standard 't~Hooft-Polyakov model in three spatial dimensions. We investigate the energy density of the static and spherically symmetric solutions to find first order differential equations that solve the equations of motion. The system is further studied and two distinct classes of solutions are obtained, one that can also be described by analytical solutions which is called small monopole, since it is significantly smaller than the standard 't~Hooft-Polyakov monopole. The other type of structure is the hollow monopole, since the energy density is endowed with a hole at its core. The hollow monopole …

High Energy Physics - TheoryPhysics010308 nuclear & particles physicsDifferential equationHigh Energy Physics::LatticeMathematical analysisMagnetic monopoleStructure (category theory)FOS: Physical sciencesEquations of motionPattern Formation and Solitons (nlin.PS)Type (model theory)Nonlinear Sciences - Pattern Formation and Solitons01 natural sciencesCondensed Matter - Other Condensed MatterCore (optical fiber)High Energy Physics - PhenomenologyHigh Energy Physics - Phenomenology (hep-ph)High Energy Physics - Theory (hep-th)Ordinary differential equation0103 physical sciencesEnergy density010306 general physicsOther Condensed Matter (cond-mat.other)Physical Review D
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