3 documentos corresponden a la consulta.
Palabras contadas: infeld: 4, born: 8
Ferraro, R. - Fiorini, F.
Phys Lett Sect B Nucl Elem Part High-Energy Phys 2010;692(3):206-211
2010
Descripción: In the context of Born-Infeld determinantal gravity formulated in an n-dimensional spacetime with absolute parallelism, we found an exact 3-dimensional vacuum circular symmetric solution without cosmological constant consisting in a rotating spacetime with non-singular behavior. The space behaves at infinity as the conical geometry typical of 3-dimensional General Relativity without cosmological constant. However, the solution has no conical singularity because the space ends at a minimal circle that no freely falling particle can ever reach in a finite proper time. The space is curved, but no divergences happen since the curvature invariants vanish at both asymptotic limits. Remarkably, this very mechanism also forbids the existence of closed timelike curves in such a spacetime. © 2010 Elsevier B.V.
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Ferraro, R. - Fiorini, F.
J. Phys. Conf. Ser. 2011;314(1)
2011
Temas: Relativity - Closed timelike curves - Conical singularities - Cosmic strings - Einstein gravity - Cosmology
Descripción: It is shown that Born-Infeld gravity -a high energy deformation of Einstein gravity-removes the singularities of a cosmic string. The respective vacuum solution results to be free of conical singularity and closed timelike curves. The space ends at a minimal circle where the curvature invariants vanish; but this circle cannot be reached in a finite proper time. © Published under licence by IOP Publishing Ltd.
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Eiroa, E.F. - Simeone, C.
AIP Conf. Proc. 2011;1458:383-386
2011
Descripción: The characterization and the mechanical stability of charged thin shells with spherical symmetry are analyzed in the context of Einstein-Born-Infeld theory. The study of stability is performed by considering linearized perturbations preserving the symmetry of the static configurations. It is found that as the charge increases, the shells can be stable for a wider range of the parameters. © 2012 American Institute of Physics.
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