Ray of light travelling through universe (applying cosmological principle)

In summary, the cosmological principle states that the universe is homogeneous and isotropic on large scales, meaning it looks the same in every direction and from every point of view. This applies to the path of a ray of light traveling through the universe, as long as it travels a large distance. The path may appear straight, but it can be affected by gravitational fields, causing it to bend or curve. In some cases, the path may even be deflected significantly due to gravitational lensing or reflections.
  • #1
keks
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cosmological principle states that, on large spatial scales, universe is homogeneous and isotropic. in other words, universe looks the same in every direction and that is true for every point of view. there are some challanges to this principle, but for this discussion, I will assume it is correct.
so, let's start.
on the following picture we can see: a source of light (laser), a ray of light and a receptor. this is hypothetical setting, so, i will assume that a source and receptor are massless, so there are no gravitational fields here.
pic1:
https://www.physicsforums.com/attachments/13682
we see, ray of light, following a straight line and hiting earth.

next example is a bit more complicated because ray of light travels through universe. but according to cosmological principle universe is homogeneous and isotropic on large scales, and our ray of light traveles great distance so we can apply the principle.
pic2:
https://www.physicsforums.com/attachments/13683
ok, what do we see on pic2?
on top we see universe and gravity presented with the same shade of gray. but why did I do that? I did this because I simply applied cosmological principle on this ray.

on bottom part of pic2 we can see it in 'reality'. I used this beautiful picture of omega centauri to represent the whole universe. here yellow line isn't really 'straight'. I used a straight line only to approximate the path of light. what really happens is that this line bends as light travels through gravitational fields of different strength (gravitational lensing). but, since universe is homogeneous and isotropic I can assume this local bending will be 'straightened' with another bending, but in different direction, providig that this ray of light travelles large distances. so, at the end, its path can be approximated with a 'straight' line.
and this we can see on pic3.
pic3:
https://www.physicsforums.com/attachments/13684



and fially - my question is:
can we approximate path of a ray of light through universe with a straight line, providing that the ray traveles large distance?
 
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  • #2
Hi Keks,

Your attachment links don't work, so I didn't view them.

Viewed from a comoving frame, a light ray will travel on a perfectly "straight" line (geodesic) if the spacetime is flat: i.e., it doesn't pass through a gravitational field and the background spatial geometry is perfectly flat.

On the other hand, if the light ray passes through a gravitational field, then its spacetime geodesic will not be perfectly straight. One can't really say that it is "approximately" a straight line; the total amount of deflection from the original course depends on the intensity of the gravitational field(s) (curved spacetime) it passes through, how close it passes to the gravitational source(s), etc. For example, if the light ray is gravitationally lensed because it passes very close to a highly massive structure (such as a rich galaxy cluster), then the amount of deflection will be noticeably significant.

Or if a light ray strikes an object and reflects off of it, then obviously the deflection could be any amount, even 180 degrees.

Jon
 

1. How does light travel through the universe?

According to the cosmological principle, light travels through the universe in a straight line at a constant speed of 299,792,458 meters per second in a vacuum. This is known as the speed of light and is the fastest speed possible in the universe.

2. Does light experience any changes or distortions as it travels through the universe?

Yes, light can experience changes or distortions as it travels through the universe. This can occur due to the presence of gravitational fields, such as those caused by massive objects like galaxies or black holes. These distortions can cause light to bend or warp, known as gravitational lensing.

3. How does the cosmological principle explain the redshift of light from distant galaxies?

The cosmological principle explains the redshift of light from distant galaxies by the expansion of the universe. As space itself expands, the wavelengths of light are stretched, causing them to appear redder. This is known as cosmological redshift and provides evidence for the expansion of the universe.

4. Can the cosmological principle be applied to all types of light?

Yes, the cosmological principle can be applied to all types of light, including visible light, radio waves, and X-rays. This is because all forms of light travel through the universe at the same speed and are subject to the same laws of physics.

5. How does the cosmological principle impact our understanding of the universe?

The cosmological principle is a fundamental concept in cosmology and helps us understand the large-scale structure and behavior of the universe. It allows us to make predictions about the expansion of the universe, the distribution of matter and energy, and the overall structure of the universe on a grand scale.

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