Litcius/Paper detail

Nonlinear <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>σ</mml:mi></mml:math>-models in the Eddington-inspired Born-Infeld gravity

J. R. Nascimento, Gonzalo J. Olmo, P. J. Porfírio, A. Yu. Petrov, A. R. Soares

2020Physical review. D/Physical review. D.36 citationsDOIOpen Access PDF

Abstract

In this paper we consider two different nonlinear $\ensuremath{\sigma}$-models minimally coupled to Eddington-inspired Born-Infeld gravity. We show that the resultant geometries represent minimal modifications with respect to those found in GR, though with important physical consequences. In particular, wormhole structures always arise, though this does not guarantee by itself the geodesic completeness of those space-times. In one of the models, quadratic in the canonical kinetic term, we identify a subset of solutions which are regular everywhere and are geodesically complete. We discuss characteristic features of these solutions and their dependence on the relationship between mass and global charge.

Topics & Concepts

GeodesicWormholeNonlinear systemQuadratic equationPhysicsCompleteness (order theory)Theoretical physicsKinetic termBorn–Infeld modelSpace (punctuation)Classical mechanicsPure mathematicsMathematical physicsStatistical physicsMathematical analysisMathematicsComputer scienceAction (physics)GeometryQuantum mechanicsOperating systemScalar fieldCosmology and Gravitation TheoriesBlack Holes and Theoretical PhysicsNoncommutative and Quantum Gravity Theories