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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. NascimentoDepartamento de Física, Universidade Federal da Paraíba, Caixa Postal 5008, 58051-970 João Pessoa, Paraíba, BrazilGonzalo J. OlmoDepartament de Física Teòrica and IFIC, Centro Mixto Universitat de València—CSIC, Universitat de València, Burjassot-46100, València, SpainP. J. PorfírioDepartament of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania 19104, USAA. Yu. PetrovDepartamento de Física, Universidade Federal da Paraíba, Caixa Postal 5008, 58051-970 João Pessoa, Paraíba, BrazilA. R. SoaresDepartamento de Física, Universidade Federal da Paraíba, Caixa Postal 5008, 58051-970 João Pessoa, Paraíba, Brazil
2020en
ABI

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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.

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