José Luis Flores
University of Málaga
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Featured researches published by José Luis Flores.
Classical and Quantum Gravity | 2003
José Luis Flores; Miguel Sánchez
Let = 0 × 2 be a pp-wave-type spacetime endowed with the metric , z = , x + 2du dv + H(x, u) du2, where (0, , x) is any Riemannian manifold and H(x, u) is an arbitrary function. We show that the behaviour of H(x, u) at spatial infinity determines the causality of , say: (a) if −H(x, u) behaves subquadratically (i.e, essentially −H(x, u) ≤ R1(u)|x|2− for some > 0 and large distance |x| to a fixed point) and the spatial part (0, , x) is complete, then the spacetime is globally hyperbolic, (b) if −H(x, u) grows at most quadratically (i.e, −H(x, u) ≤ R1(u)|x|2 for large |x|) then it is strongly causal and (c) is always causal, but there are non-distinguishing examples (and thus, not strongly causal), even when −H(x, u) ≤ R1(u)|x|2+, for small > 0. Therefore, the classical model 0 = 2, H(x, u) = ∑i, j hij(u)xixj(≢ 0), which is known to be strongly causal but not globally hyperbolic, lies in the critical quadratic situation with complete 0. This must be taken into account for realistic applications. In fact, we argue that −H will be subquadratic (and the spacetime globally hyperbolic) if is asymptotically flat. The relation of these results with the notion of astigmatic conjugacy and the existence of conjugate points is also discussed.
Communications in Mathematical Physics | 2007
José Luis Flores
We present a new development of the causal boundary of spacetimes, originally introduced by Geroch, Kronheimer and Penrose. Given a strongly causal spacetime (or, more generally, a chronological set), we reconsider the GKP ideas to construct a family of completions with a chronology and topology extending the original ones. Many of these completions present undesirable features, like those which appeared in previous approaches by other authors. However, we show that all these deficiencies are due to the attachment of an “excessively big” boundary. In fact, a notion of “completion with minimal boundary” is then introduced in our family such that, when we restrict to these minimal completions, which always exist, all previous objections disappear. The optimal character of our construction is illustrated by a number of satisfactory properties and examples.
General Relativity and Gravitation | 2003
Anna Maria Candela; José Luis Flores; Miguel Sánchez
AbstractA general class of Lorentzian metrics,
Journal of Differential Equations | 2002
José Luis Flores; Miguel Sánchez
Journal of High Energy Physics | 2008
José Luis Flores; Miguel Sánchez
\mathcal{M}_0 \times \mathbb{R}^2
Journal of Geometry and Physics | 2000
José Luis Flores; Miguel Sánchez
Lecture Notes in Physics | 2006
José Luis Flores; Miguel Sánchez
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Classical and Quantum Gravity | 2007
José Luis Flores; Steven G. Harris
General Relativity and Gravitation | 2007
V. Alaña; José Luis Flores
\langle \cdot ,\; \cdot \rangle _z = \langle \cdot ,\; \cdot \rangle _x + 2\;\;du\;\;dv + H(x,u)\;du^2
Journal of Differential Equations | 2003
Anna Maria Candela; José Luis Flores; Miguel Sánchez