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Nonsingular Black Holes in ƒ (R) Theories

Departamento de Física Teórica and IFIC, Centro Mixto Universidad de Valencia - CSIC. Universidadde Valencia, Burjassot-46100, Valencia, Spain
Departamento de Física, Universidade Federal da Paraíba, 58051-900 João Pessoa, Paraíba, Brazil
Center for Field Theory and Particle Physics and Department of Physics, Fudan University, 220 Handan Road, 200433 Shanghai, China
Author to whom correspondence should be addressed.
Academic Editor: Lorenzo Iorio
Universe 2015, 1(2), 173-185;
Received: 21 May 2015 / Revised: 28 July 2015 / Accepted: 29 July 2015 / Published: 4 August 2015
(This article belongs to the Collection Open Questions in Black Hole Physics)
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 curvature divergences at the wormhole throat. View Full-Text
Keywords: nonsingular black holes; modified gravity; wormholes nonsingular black holes; modified gravity; wormholes
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MDPI and ACS Style

Olmo, G.J.; Rubiera-Garcia, D. Nonsingular Black Holes in ƒ (R) Theories. Universe 2015, 1, 173-185.

AMA Style

Olmo GJ, Rubiera-Garcia D. Nonsingular Black Holes in ƒ (R) Theories. Universe. 2015; 1(2):173-185.

Chicago/Turabian Style

Olmo, Gonzalo J., and Diego Rubiera-Garcia. 2015. "Nonsingular Black Holes in ƒ (R) Theories" Universe 1, no. 2: 173-185.

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