An analysis of Born-Infeld determinantal gravity in Weitzenbock spacetime
arXiv:1608.02622 · doi:10.1016/j.physletb.2016.10.016
Abstract
The Born-Infeld theory of the gravitational field formulated in Weitzenbock spacetime is studied in detail. The action, constructed quadratically upon the torsion two-form, reduces to Einstein gravity in the low field limit where the Born-Infeld constant goes to infinity, and it is described by second order field equations for the vielbein field in spacetime dimensions. The equations of motion are derived, and a number of properties coming from them are discussed. In particular, we show that under fairly general circumstances, the equations of motion are those of Einstein's General Relativity plus an energy-momentum tensor of purely geometrical character. This tensor is obtained solely from the parallelization defining the spacetime structure, which is encoded in a set of D smooth, everywhere non-null, globally defined 1-forms. Spherical symmetry is studied as an example, and we comment on the emergence of the Schwarzschild geometry within this framework. Potential (regular) extensions of it are envisioned.
8 pages, no figures. Additional comments at the end of Sec. II. Two more references are included. Accepted in PLB
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Cited by in corpus (8)
- McVittie solution in f(T) gravity
- BTZ gems inside regular Born-Infeld black holes
- Matching tetrads in f(T) gravity
- Chronology protection in gravity: the case of Gott's pair of moving cosmic strings
- Role of the remnant symmetries in gravitational theories based on absolute parallelism: a 2D standpoint
- Thick branes in Born-Infeld determinantal gravity in Weitzenböck spacetime
- Teleparallel Jackiw-Teitelboim gravity
- Local symmetries in -like models: lessons from 2D