English

Causality and Conjugate Points in General Plane Waves

General Relativity and Quantum Cosmology 2007-05-23 v2 High Energy Physics - Theory

Abstract

Let M=M0×R2M = M_0 \times \R^2 be a pp--wave type spacetime endowed with the metric <,>z=<,>x+2dudv+H(x,u)du2<\cdot,\cdot>_z = <\cdot,\cdot>_x + 2 du dv + H(x,u) du^2, where (M0,<,>x)(M_0, <\cdot,\cdot>_x) is any Riemannian manifold and H(x,u)H(x,u) an arbitrary function. We show that the behaviour of H(x,u)H(x,u) at spatial infinity determines the causality of MM, say: (a) if H(x,u)-H(x,u) behaves subquadratically (i.e, essentially H(x,u)R1(u)x2ϵ-H(x,u) \leq R_1(u) |x|^{2-\epsilon} for some ϵ>0\epsilon >0 and large distance x|x| to a fixed point) and the spatial part (M0,<,>x)(M_0, <\cdot,\cdot>_x) is complete, then the spacetime MM is globally hyperbolic, (b) if H(x,u)-H(x,u) grows at most quadratically (i.e, H(x,u)R1(u)x2-H(x,u) \leq R_1(u) |x|^{2} for large x|x|) then it is strongly causal and (c) MM is always causal, but there are non-distinguishing examples (and thus, non-strongly causal), even when H(x,u)R1(u)x2+ϵ-H(x,u) \leq R_1(u) |x|^{2+\epsilon} , for small ϵ>0\epsilon >0. Therefore, the classical model M0=R2M_0 = \R^2, H(x,u)=i,jhij(u)xixj(≢0)H(x,u) = \sum_{i,j} h_{ij}(u) x_i x_j (\not\equiv 0), which is known to be strongly causal but not globally hyperbolic, lies in the critical quadratic situation with complete M0M_0. This must be taken into account for realistic applications. In fact, we argue that H-H will be subquadratic (and the spacetime globally hyperbolic) if MM is asymptotically flat. The relation of these results with the notion of astigmatic conjugacy and the existence of conjugate points is also discussed.

Keywords

Cite

@article{arxiv.gr-qc/0211086,
  title  = {Causality and Conjugate Points in General Plane Waves},
  author = {J. L. Flores and M. Sánchez},
  journal= {arXiv preprint arXiv:gr-qc/0211086},
  year   = {2007}
}

Comments

Version improved with further discussions and a new section; 21 pages, Latex