Born-Infeld inspired modifications of gravity

被引:209
|
作者
Beltran Jimenez, Jose [1 ,2 ]
Heisenberg, Lavinia [3 ]
Olmo, Gonzalo J. [4 ,5 ,6 ]
Rubiera-Garcia, Diego [7 ]
机构
[1] Univ Autonoma Madrid, CSIC, Inst Fis Teor, E-28049 Madrid, Spain
[2] Univ Toulon & Var, Aix Marseille Univ, CNRS, CPT, Marseille, France
[3] Swiss Fed Inst Technol, Inst Theoret Studies, Clausiusstr 47, CH-8092 Zurich, Switzerland
[4] Univ Valencia, CSIC, Ctr Mixto, Dept Fis Teor, E-46100 Valencia, Spain
[5] Univ Valencia, CSIC, Ctr Mixto, IFIC, E-46100 Valencia, Spain
[6] Univ Fed Paraiba, Dept Fis, BR-58051900 Joao Pessoa, Paraiba, Brazil
[7] Univ Lisbon, Fac Ciencias, Inst Astrofis & Ciencias Espaco, PT-1749016 Lisbon, Portugal
基金
欧盟地平线“2020”;
关键词
Born-Infeld gravity; Astrophysics; Black holes; Cosmology; Early universe; Compact objects; Singularities; EQUATION-OF-STATE; CHARGED BLACK-HOLE; GENERAL-RELATIVITY; COSMOLOGICAL CONSTANT; DARK ENERGY; DUALITY ROTATIONS; NONLINEAR ELECTRODYNAMICS; GRAVITATIONAL COLLAPSE; DETERMINANTAL GRAVITY; EINSTEIN EQUATIONS;
D O I
10.1016/j.physrep.2017.11.001
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
General Relativity has shown an outstanding observational success in the scales where it has been directly tested. However, modifications have been intensively explored in the regimes where it seems either incomplete or signals its own limit of validity. In particular, the breakdown of unitarity near the Planck scale strongly suggests that General Relativity needs to be modified at high energies and quantum gravity effects are expected to be important. This is related to the existence of spacetime singularities when the solutions of General Relativity are extrapolated to regimes where curvatures are large. In this sense, Born-Infeld inspired modifications of gravity have shown an extraordinary ability to regularise the gravitational dynamics, leading to non-singular cosmologies and regular black hole spacetimes in a very robust manner and without resorting to quantum gravity effects. This has boosted the interest in these theories in applications to stellar structure, compact objects, inflationary scenarios, cosmological singularities, and black hole and wormhole physics, among others. We review the motivations, various formulations, and main results achieved within these theories, including their observational viability, and provide an overview of current open problems and future research opportunities. (C) 2017 Elsevier B.V. All rights reserved.
引用
收藏
页码:1 / 129
页数:129
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