Paper 3, Section II, D

General Relativity
Part II, 2017

Let M\mathcal{M} be a two-dimensional manifold with metric g\boldsymbol{g} of signature +-+.

(i) Let pMp \in \mathcal{M}. Use normal coordinates at the point pp to show that one can choose two null vectors V,W\mathbf{V}, \mathbf{W} that form a basis of the vector space Tp(M)\mathcal{T}_{p}(\mathcal{M}).

(ii) Consider the interval IRI \subset \mathbb{R}. Let γ:IM\gamma: I \rightarrow \mathcal{M} be a null curve through pp and U0\mathbf{U} \neq 0 be the tangent vector to γ\gamma at pp. Show that the vector U\mathbf{U} is either parallel to V\mathbf{V} or parallel to W\mathbf{W}.

(iii) Show that every null curve in M\mathcal{M} is a null geodesic.

[Hint: You may wish to consider the acceleration aα=UββUαa^{\alpha}=U^{\beta} \nabla_{\beta} U^{\alpha}.]

(iv) By providing an example, show that not every null curve in four-dimensional Minkowski spacetime is a null geodesic.