How does this affect our ability to see the early universe?

In summary, the conversation discusses the concept of the big bang theory and the limitations of seeing the early universe due to expansion. It also touches on the idea of breaching the speed of light and the conditions of the infant universe. The participants also explore the concept of space and its relationship to mass.
  • #1
AJ_2010
25
0
When I think of what happened in the big bang theory and in today's world when we look through telescopes and look at distant objects it raises the question of how far back in time can we actually see with more and more powerful telescopes?

One thing that I find confusing is that at the time of the big bang I assume many things were expanding at or close to the speed of light and then slowed down as they changed to particles with more mass. In which case, everything on the boundary of expansion would have its 'history' moving at the same speed as everything else. How is it possible to see light that has already passed us and is heading outwards from the centre of expansion?

Sure we can see distant stars and we see them as they were 100 or so light years away...but the light that was present when the universe was close would surely have passed the Earth with nothing to reflect it back... is this right?
If this is true then the light or information that we can view that shows the very early universe is way passed the Earth with nothing in the beyond that is able to reflect it back.
 
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  • #2
Expansion is the short answer. Immediately following the big bang, the universe expanded faster than light, then slowed down.
 
  • #3
So in effect are we still awaiting the light from the big bang to catch up to us here on earth?

The particles that formed Earth must have been traveling faster than light for a LONG time before they slowed down, in order that 13.75billion years have passed and the light from the big bang has still not passed us. ? Is this a correct statement?
 
  • #4
Anybody have a reply for this?I used to be good at physics at 'A' level but its been a while since I took a questioning interest on the huge subject that it is.
I'm hoping to get back into building my knowledge on physics but first I need to clear up some good old fundamental questions that are running around in my head.
 
  • #5
See #3 and #5 in this thread. Make sure you click the links in #5.
 
  • #6
Thanks Fredrik.
 
  • #7
well the idea is that after the big bang there was a period of "inflation" where space was actually expanding faster than light there fore thee universe before this time is opaque. Then expansion settled down about 100,000 years after the big bang and we can see this as the cmb or cosmic microwave background. And we can see that with telescopes today, but we cannot see any further back. Thats why gravity waves have become a hot topic as gravity waves travel with space,

As for distant stars that would be "in front " of us, that's a bad way to think of it. There is no real center of the universe there fore they are not in front or behind us they are simply traveling with respect to us. We can see them because stars emit radiation atall wavelengths in every direction.
 
  • #8
If an object travels the speed of light it becomes infainitly heavy, so it would effectivly implode hence not exsist so no light.

Einstein’s theories
No physical object can travel at or faster than the speed of light. The speed of light is generally considered to be a physical speed barrier.
As objects approach the speed of light, their "rate of time" approaches zero, and distances (travelled by the object) approach zero, and their mass increases.
 
  • #9
If the speed of light limit has been breached before then we can breach it again. It is only a matter of time.

If only we can create conditions that were similar to the infant Universe...

Conversely if there is no upper limit for a particle then it can exist in multiple locations at the same time which puts a sort of dampner on our hopes.

The only reason I want us to breach the speed of light is because I want to see us visit other stars and galaxies in a short space of time.
 
  • #10
Plebeian said:
If the speed of light limit has been breached before then we can breach it again. It is only a matter of time.

If only we can create conditions that were similar to the infant Universe...


When we say that in the early universe, space was expanding faster than the speed of light, we mean just that, space -- not mass. The concept of "inflation" does not suggest that any object with mass ever moved at C (velocity of light). And even though some have suggested that in the early universe, the speed of light may have differered from its current value, no one has ever suggested that any object containing mass can reach C (whatever C's velocity is or was). The postulates of the special theory of relativity would still hold, regardless of the value of C.
 
  • #11
JamiePocock said:
If an object travels the speed of light it becomes infainitly heavy, so it would effectivly implode hence not exsist so no light.
This is false.

Objects moving relativistically will gain mass as observed from an external frame of reference. They do not not gain in hteir own frame of reference, and thus will not "implode".
 
  • #12
Plebeian said:
If the speed of light limit has been breached before then we can breach it again. It is only a matter of time.

If only we can create conditions that were similar to the infant Universe...
Well, one of the conditions during this phase is that the universe was smaller than an atom.

Which means...
Plebeian said:
The only reason I want us to breach the speed of light is because I want to see us visit other stars and galaxies in a short space of time.
...no stars or galaxies.

And, well, come to think of it, no atoms either...
 
  • #13
LBrandt -- So what exactly is 'space' if there is no mass to occupy it, or to define its boundary?

And next question; is this saying that a universe can be defined as a small vacuum?
 
  • #14
In special relativity (flat spacetime), there is a standard definition of (spatial) distance that can be applied both locally and globally. In other words, this definition of distance applies to nearby objects, and to objects that are far away. Speed is change in distance divided by elapsed time, so this standard definition of distance can be used to calculated speeds of objects that are near and far. Speeds of objects, near and far, calculated in this way always have the speed of light as their speed limit.

The situation in general relativity (curved spacetime) is far different. Because of spacetime curvature, the definition of (spatial) distance used in the flat spacetime of special relativity can only be applied locally, just as the Earth looks flat only locally. This leads to speeds of nearby objects that limited by the the speed of light, but it say nothing about the behaviour of objects that are far away.

Even though the special relativity definition of distance cannot be applied globally in curved spacetime, there is a standard cosmological definition of distance that is used in the Hubble relationships. Strangely, this cosmological definition of distance can be applied to the flat spacetime of special relativity (Milne universe), and when this is done, it produces a definition of distance (for special relativity) that is different than the standard definition of distance in special relativity!

A different definition of distance gives a different concept of speed, since speed is distance over time. This alternative definition of speed, even within the context of special relativity, produces speeds of material objects that are greater than the standard speed of light! In other words, this definition of speed produces, in both cosmology and in special relativity, speeds that are greater than the standard speed of light.

If v is standard speed in special relativity, and V is cosmological "speed" applied to special relativity, then some corresponding values (as fractions of the numerical value of the standard speed of light) are:

Code:
  v                   V
0.200                0.203
0.400                0.424
0.600                0.693
0.800                1.10
0.990                2.65

Even though there can be different definitions of spatial distance, there is no ambiguity with respect to the prediction of experimental measurements. One just has to keep in mind what definition is being used.
 
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  • #15
George Jones said:
In special relativity (flat spacetime), there is a standard definition of (spatial) distance that can be applied both locally and globally. In other words, this definition of distance applies to nearby objects, and to objects that are far away. Speed is change in distance divided by elapsed time, so this standard definition of distance can be used to calculated speeds of objects that are near and far. Speeds of objects, near and far, calculated in this way always have the speed of light as their speed limit.

The situation in general relativity (curved spacetime) is far different. Because of spacetime curvature, the definition of (spatial) distance used in the flat spacetime of special relativity can only be applied locally, just as the Earth looks flat only locally. This leads to speeds of nearby objects that limited by the the speed of light, but it say nothing about the behaviour of objects that are far away.

Is this tantamount to saying that the superluminal expansion of the universe cannot be adequately explained without general relativity? i.e. that it is the curvature of space that allows objects to recede superluminally?
 
  • #16
LBrandt said:
When we say that in the early universe, space was expanding faster than the speed of light, we mean just that, space -- not mass. The concept of "inflation" does not suggest that any object with mass ever moved at C (velocity of light). And even though some have suggested that in the early universe, the speed of light may have differered from its current value, no one has ever suggested that any object containing mass can reach C (whatever C's velocity is or was). The postulates of the special theory of relativity would still hold, regardless of the value of C.

Okay. Thank you for clearing that up for me.

So for reaching large distances in a short space of time we can use the same principle right?

If we can create an inflation drive that can expand/contract the space around an object then reaching far away distances could be made easier. I think our understanding of space is rudimentary at best so maybe if we can figure out ways to manipulate it then this seemingly large distances might just become short.

There is the other paradox that I mentioned in my post - i.e if objects can say move really fast(say using inflation drives/ warp drives or whatever) then they can be at two places at the same time.
 
  • #17
Plebeian said:
If we can create an inflation drive that can expand/contract the space around an object then reaching far away distances could be made easier.
http://en.wikipedia.org/wiki/Alcubierre_drive :biggrin:
Plebeian said:
There is the other paradox that I mentioned in my post - i.e if objects can say move really fast(say using inflation drives/ warp drives or whatever) then they can be at two places at the same time.

How does this follow? Being in two places almost at once is not the same as actually being in two places a once.
 
  • #18
DaveC426913 said:
http://en.wikipedia.org/wiki/Alcubierre_drive :biggrin:How does this follow? Being in two places almost at once is not the same as actually being in two places a once.

Regarding the Alcubierre drive.. His explanation seems plausible. I just thought that we need to contract space to move toward an object and expand space to move away from an object. Like objects stuck on a flat rubber sheet.

We need to do exactly what space did to expand when the universe was born. I always believe that if something has occurred in nature then we can replicate it too.

About the second point, you are right. :)
 
  • #19
Blimey...a lot of this is over my head but I still find it fascinating.
 
  • #20
Plebeian said:
We need to do exactly what space did to expand when the universe was born.
This might take you far away from home, but it won't take you closer to anything else.
 
  • #21
Fredrik said:
This might take you far away from home, but it won't take you closer to anything else.

Oh yeah.

What if we expand space relative to everyother object except one?

Or like the Alcubierre drive, expand the space behind the object and contract the space in front of it.
 

1. What is the speed of light?

The speed of light is a fundamental constant in physics, denoted by the letter c. In a vacuum, it has a value of approximately 299,792,458 meters per second, or about 186,282 miles per second. This means that light can travel a distance of about 9.46 trillion kilometers in one year.

2. Why is the speed of light important in the study of the big bang?

The speed of light is important in the study of the big bang because in the early stages of the universe, when it was incredibly hot and dense, light was the only thing that could move at this speed. This means that the light from these early stages of the universe is still reaching us today, allowing us to study and understand the origins of our universe.

3. How does the speed of light relate to the expansion of the universe?

The speed of light is directly related to the expansion of the universe. As the universe expands, the light traveling through it also expands, which means that the wavelength of the light gets stretched out. This is known as redshift and is one of the pieces of evidence for the expansion of the universe.

4. Can anything travel faster than the speed of light?

According to our current understanding of physics, nothing can travel faster than the speed of light. The theory of relativity states that as an object approaches the speed of light, its mass increases infinitely, making it impossible to reach or exceed this speed. This also means that information and particles cannot travel faster than the speed of light.

5. What does the speed of light tell us about the age of the universe?

The speed of light plays a crucial role in determining the age of the universe. By measuring the distance between distant galaxies and the time it takes for light to reach us from those galaxies, scientists can calculate the age of the universe. This is known as the cosmic distance ladder and is one of the ways we can estimate the age of our universe, which is currently believed to be about 13.8 billion years old.

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