I'm trying to understand how to compute the null future-directed vector fields if I have a given (Bondi) metric

$g=-e^{2\nu}du^{2}-2e^{\nu+\lambda}dudr+r^{2}d\Omega$

with $d\Omega$-standard metric on the unit sphere. I was reading this paper http://www.jstor.org/stable/2118619 and there came the statement (no proof) that the null future directed vector fields, called $n$ and $l$, are given by

$n=2e^{-\nu}\frac{\partial}{\partial u}-e^{-\lambda}\frac{\partial}{\partial r}$

$l=e^{-\lambda}\frac{\partial}{\partial r}$

with $g(n,l)=-2$.

I do not understand where these expressions for the null vector fields came from, i.e. what kind of formulas did one use? I know that null vector fields are composed of null vectors, and a null vector $v$ is such that $g(v,v)=0$, but this doesn't really bring me a way to calculate $n$ and $l$.

Attempt at the solution: Let $v=v_{1}\frac{\partial}{\partial u}+v_{2}\frac{\partial}{\partial r}$ be a null vector field. Then should hold:

$g_{00}(v_{1})^{2}+2g_{01}v_{1}v_{2}=0$

this gives us two possible solutions, let call them $l$ and $r$, so as to be consistent with the paper. The first solution gives $v_{1}=0$ so one can write

$l=\mathrm{something}\cdot\frac{\partial}{\partial r}$

and the second solution gives $v_{1}=-2e^{\lambda-\nu}v_{2}$, so that we can write

$n=(-2e^{\lambda-\nu}\cdot\mathrm{somethingElse})\cdot\frac{\partial}{\partial u}+\mathrm{somethingElse}\cdot\frac{\partial}{\partial r}$.

So I seem to get the general form of these null fields, but still have two open questions:

where do I see that they are "future-directed"?

how was the choice of "something" and "somethingElse" made? (in the paper, rather specific functions occur there without any explanation)

`n`

and`l`

are an example. I have, for example, seen other authors take`g(n,l)=-1`

rather than`-2`

. – Ben Whale Nov 12 '13 at 21:39