Light from the big Bang/Inflation

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In summary: Starts with a description of the horizon problem and how it relates to the expansion of the universe and the singularity. Then goes on to explain some misconceptions about cosmological horizons and the superluminal expansion of the universe. In summary, the horizon problem is a problem in understanding how the universe expands and the singularity is a theoretical point at which the laws of physics break down. The misconceptions about cosmological horizons and the superluminal expansion of the universe are due to a lack of understanding of the concepts involved.
  • #1
Lazernugget
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Okay, so here's my questions:

1. Why can't we see the light from the big bang? If it happened 14 billion years ago, shouldn't we be able to see the light from the big bang by now? Or is the Earth and everything else moving away from the spot of the big bang faster than or at the speed of light? (Space itself can move at rates that are technically faster that light, right?)

2. If the universe where spherical, then the universe could be bigger than 13-14 bil. LY in diameter, right?

3. What do we think the singularity was "Made out of"? Dark matter/Energy, strings, energy, etc.

Thanks,

-Lazer
 
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  • #2
We can see nothing beyond the surface of last scattering. Period.
 
  • #3
Light is emitted form the centre of the sun, yet we can't see the centre of the sun. This is becuase the plasma is opaque, so one can only see the surface. Similarly the CMB was emitted 380,000 years after the big bang. This is known as the era of recombination. The CMb at the time of recombination is an opaque plasma like the surface of the sun , hence we cannot get any lights from the big bang.
However the structure of the CMB can give us clues as to what happened before the era of recombination. But it is not a direct observation of the light.
 
  • #4
Lazernugget said:
1 . Why can't we see the light from the big bang?
We can! It's called the cosmic microwave background. This is the radiation that decoupled from matter as soon as the universe cooled to the point where neutral hydrogen could form. It has since been streaming across the cosmos...

2. If the universe where spherical, then the universe could be bigger than 13-14 bil. LY in diameter, right?
It's important to point out that the observable universe is ~ 28 Mpc -- the actual universe is likely much larger -- perhaps infinite. The observable universe is, however, very nearly flat. If the universe is in fact spherical, then it has a comparatively large radius with our observable universe occupying only a small, locally very nearly flat, portion of this sphere.

3. What do we think the singularity was "Made out of"? Dark matter/Energy, strings, energy, etc.
Most think the singularity simply disappears when a more complete theory of gravity is implemented.
 
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  • #6
Naty1 said:
Great explanations here:
http://adsabs.harvard.edu/abs/2004PASA...21...97D

Expanding Confusion: Common Misconceptions of Cosmological Horizons and the Superluminal Expansion of the Universe

Davis, Tamara M.; Lineweaver, Charles H.

Good article that gives physical feel to what is going on.
 

1. What is "light from the Big Bang/Inflation"?

The term "light from the Big Bang/Inflation" refers to the cosmic microwave background (CMB) radiation, which is the oldest light in the universe. It is the faint glow of heat left over from the Big Bang, which is believed to have occurred approximately 13.8 billion years ago.

2. How is the light from the Big Bang/Inflation detected?

The light from the Big Bang/Inflation is detected using specialized telescopes, such as the Planck satellite and the Wilkinson Microwave Anisotropy Probe (WMAP). These telescopes are designed to measure the faint microwave radiation that permeates the entire universe.

3. What does the light from the Big Bang/Inflation tell us about the early universe?

The light from the Big Bang/Inflation provides valuable insights into the early universe, such as its temperature, density, and composition. It also helps us understand the formation of structures in the universe, such as galaxies and galaxy clusters.

4. How does the concept of inflation relate to the light from the Big Bang?

Inflation is a theory that suggests the universe went through a rapid expansion phase in the first fraction of a second after the Big Bang. This theory is supported by the observations of the uniformity and isotropy of the CMB, which is believed to have been caused by the rapid expansion of the universe during inflation.

5. Can we see the light from the Big Bang/Inflation with the naked eye?

No, the light from the Big Bang/Inflation cannot be seen with the naked eye. It is detectable only through specialized telescopes that can measure microwaves. However, the effects of the Big Bang and inflation can be seen in the large-scale structures of the universe and the distribution of galaxies.

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