[math, computation] Raychaudhuri equation in null geodesic

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continue on last posting. In this post we want to derive Raychaudhuri equation for null geodesic.

We want to obtain this equation
RN-10.png

Construction of Null parametrization

First let us do Null parametrization by null vector k

RN-0.png

Here we introduce auxiliary null vector N^a and, since it is a null vector its square become zero but contraction with another null vector k we can set -1 by proper normalization.

In my previous posting which discuss time-like geodesic we use time-like vector u^a, here we will use null vector k instead of u. The problem here is for the previous case u_{a;b} is orthogonal to u^a, but here k_{a;b} is orthogonal to k^a but not N^a. Thus we can not decompose the B_{ab} as we did in the previous post.

Furthermore in the last posting we introduce 3-dimensional metric, but here in null case since we have two null vector, we need to introduce 2 dimensional metric h

The decomposition of metric g can be done as follows
RN-1.png

By squaring h we obtain h_{ab} h^{ab}=2. And obviously it is both orthogonal to k^a and N^a. Thus h is nothing but a 2-dimensional metric.

Decomposition of vector

First let us define quantities

RN-2.png

As i told before since B_{ab} is not orthogonal to N^a we need to introduce tilde B which both orthogonal to k and N. And do the vector decomposition on tilde B. (Obviously since tilde B is contracted with h and h is orthogonal to both k and N, tilde B is orthogonal to k and N)

RN-3.png
under this definition the square of tilde B has the following form

RN-4.png

For explicit computation about tilde theta, we have

RN-5.png

For future purpose we we need to find the relation between the square of B and the square of tilde B

RN-6.png

In the last part we impose geodesic condition. So we obtain the square of B is same with square of tilde B

Curvature

Write down the definition of Riemann curvature for null vector k^a

RN-7.png
Let's expnad L.H.S

RN-8.png

By plugging

RN-9.png

Up so far we didn't impose any condition except geodesic condition. By the same on-shell[imposing Einstein field equation and adopting perfect fluid] via the same method in my previous post, we have

RN-10.png

which is what i want to show.

[math, computation] Raychaudhuri equation in null geodesic | Ecency