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Palabras contadas: fiorini: 6, f: 184
Ferraro, R. - Fiorini, F.
J. Phys. Conf. Ser. 2011;314(1)
2011

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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Tipo de documento: info:ar-repo/semantics/documento de conferencia

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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Tipo de documento: info:ar-repo/semantics/artículo

Ferraro, R. - Fiorini, F.
Phys Lett Sect B Nucl Elem Part High-Energy Phys 2011;702(1):75-80
2011

Descripción: Some conceptual issues concerning f(T) theories - a family of modified gravity theories based on absolute parallelism - are analyzed. Due to the lack of local Lorentz invariance, the autoparallel frames satisfying the field equations are evasive to an a priori physical understanding. We exemplify this point by working out the vierbein (tetrad) fields for closed and open Friedmann-Robertson-Walker cosmologies. © 2011 Elsevier B.V.
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Tipo de documento: info:ar-repo/semantics/artículo