Null geodesics of the FRW metric

In summary, when working with light-propagation in the FRW metric, most texts use the equation ds^2 = 0 to obtain the equation d\chi/dt = -1/a for a light-ray moving from the emitter to the observer. However, this does not automatically guarantee that the obtained relation specifies a geodesic. It is necessary to check that the above equation actually specifies a geodesic. For a radial null path, there is one solution due to the spherical symmetry of the metric. While it is an interesting consistency check, it is not necessary for reaching a valid conclusion in this case.
  • #1
center o bass
560
2
When working with light-propagation in the FRW metric
$$ds^2 = - dt^2 + a^2 ( d\chi^2 + S_k(\chi) d\Omega^2)$$
most texts just set $$ds^2 = 0$$ and obtain the equation
$$\frac{d\chi}{dt} = - \frac{1}{a}$$
for a light-ray moving from the emitter to the observer.

Question1: Do we not strictly speaking also have to check that the above equation actually specifies a geodesic?

Setting ##ds^2 = 0## does not automatically guarantee that the obtained relation specifies a geodesic, right?

Question2: Is there a quick way to verify that the above curve indeed is a null-geodesic?
 
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  • #2
center o bass said:
Do we not strictly speaking also have to check that the above equation actually specifies a geodesic?

Yes.

center o bass said:
Is there a quick way to verify that the above curve indeed is a null-geodesic?

I don't know of any quicker way than finding an affine parametrization of the curve and plugging into the geodesic equation, but someone else might.
 
  • #3
Well, the given metric displays spherical symmetry. Then, for a radial null path, there is one solution. Then, if it is not a geodesic, what could choose a direction?

I would thus say, it is an interesting consistency check (which I have done for Kruskal coordinates) to verify satisfaction of the geodesic equation. However, for purposes of doing the least work for a valid conclusion, it is superfluous (in this particular case).
 

Related to Null geodesics of the FRW metric

1. What is the FRW metric?

The FRW metric is a mathematical description of the expanding universe in the framework of Einstein's general theory of relativity. It is named after the scientists who first derived it: Friedmann, Robertson, and Walker.

2. What are null geodesics?

Null geodesics are the paths that light (or any other massless particle) travels in a curved spacetime. They are described by the equations of motion in general relativity and are important in understanding the behavior of light in the universe.

3. How are null geodesics related to the FRW metric?

The FRW metric describes the curvature of the universe, and null geodesics are the paths that light takes in this curved spacetime. Therefore, the FRW metric is used to calculate the trajectory of light and understand how it is affected by the expanding universe.

4. What is the significance of null geodesics in cosmology?

Null geodesics play a crucial role in cosmology because they allow us to observe and study the distant parts of the universe. The speed of light is finite, so we can only see objects that are within a certain distance from us. Null geodesics help us understand how light from these distant objects is affected by the expanding universe.

5. How do null geodesics affect the shape and size of the universe?

Null geodesics determine the shape and size of the universe by influencing the paths that light travels. As the universe expands, the curvature of spacetime changes, which in turn affects the paths of null geodesics. By studying the behavior of light, we can determine the curvature and expansion of the universe.

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