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Wormholes and nonsingular spacetimes in Palatini<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>gravity

Cosimo BambiCenter for Field Theory and Particle Physics and Department of Physics, Fudan University, 220 Handan Road, 200433 Shanghai, ChinaAlejandro Cárdenas-AvendañoObservatorio Astronómico Nacional de Colombia, Universidad Nacional de Colombia, Bogotá 111321, ColombiaGonzalo J. OlmoDepartamento de Física Teórica and IFIC, Centro Mixto Universidad de Valencia—CSIC. Universidad de Valencia, Burjassot 46100, Valencia, SpainDiego Rubiera-GarciaCenter for Field Theory and Particle Physics and Department of Physics, Fudan University, 220 Handan Road, 200433 Shanghai, China
2016lv
ABI

Аннотация

We reconsider the problem of $f(R)$ theories of gravity coupled to Born-Infeld theory of electrodynamics formulated in a Palatini approach, where metric and connection are independent fields. By studying electrovacuum configurations in a static and spherically symmetric spacetime, we find solutions which reduce to their Reissner-Nordstr\"om counterparts at large distances but undergo important nonperturbative modifications close to the center. Our new analysis reveals that the pointlike singularity is replaced by a finite-size wormhole structure, which provides a geodesically complete and thus nonsingular spacetime, despite the existence of curvature divergences at the wormhole throat. Implications of these results, in particular for the cosmic censorship conjecture, are discussed.

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