Early Cosmic Inflation: Questions & Answers

In summary, the conversation discusses the early stages of Cosmic Inflation, where all matter was in a plasma form and continued to expand for 380,000 years before cooling to form the first atoms. The questions raised are whether the matter remained in a plasma state for the entire duration and if the expansion was constant during that time. The conversation also mentions the concept of dark energy causing the acceleration of expansion and the event known as "surface of last scattering." It is noted that the expansion slowed down during this period. The conversation ends with a discussion on what the universe was composed of before the Big Bang.
  • #1
Kylie87
3
0
Hello,

In the early stages of Cosmic Inflation, immediately after the Big Bang, all matter was basically energy in a plasma form. It continued to expand for 380,000 years before cooling enough to form the first atoms. I have two questions:

1. Did this matter continue to exist in a plasma state for that entire 380,000 years?
2. Did that plasma continue to expand at a constant rate for that entire 380,000 years?

Thanks,
Kylie
 
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  • #2
Your title question is about inflation and then your actual question is about expansion. They are different.

Inflation is a proposed, but not fully known to be actual, "expansion" at a rate that defies human understanding and is hypothesized to have occurred during a very tiny fraction of a second after the singularity. It solves several known issues with how the universe has formed.

Following inflation, the universe has been expanding (THIS is "expansion") ever since.

About 5 billion years ago a non-understood force (or SOMETHING) that is called "dark energy" for want of a better name, started to overcome the gravitational slowdown of the expansion and caused the expansion to accelerate, which it is still doing.

For exactly what happened at 380,000 years, Google "surface of last scattering". It was not a change in the rate of the expansion but at change in the opacity of the plasma ("let there be light").
 
  • #3
1. Did this matter continue to exist in a plasma state for that entire 380,000 years?
Neglecting the first seconds, it did.
2. Did that plasma continue to expand at a constant rate for that entire 380,000 years?
No, expansion slowed down during that period (and the following billions of years - accelerated expansion is a relatively "new" effect).
 
  • #4
Thanks for the answers. Mfb, if it was not a plasma for the first seconds, what was it?
 
  • #5
Not a plasma of nuclei, electrons and photons.
Before that, it was a plasma of nuclei, electrons and positrons and photons, and before that, it was a quark-gluon plasma.
Timeline
 
  • #6
Thanks heaps for that. It's just amazing to think that the universe was so basic in the early days; just energy really. Still, the biggest question of all still remains, which is why the big bang happened in the first place, and what was before it?
 

Related to Early Cosmic Inflation: Questions & Answers

1. What is early cosmic inflation?

Early cosmic inflation is a period of rapid expansion that occurred in the first fraction of a second after the Big Bang. During this time, the universe expanded exponentially, increasing in size by a factor of at least 10^26.

2. What caused early cosmic inflation?

The exact cause of early cosmic inflation is still unknown, but it is believed to have been triggered by a theoretical field called the inflaton field. This field is thought to have been responsible for the rapid expansion of the universe.

3. What evidence supports the theory of early cosmic inflation?

There are several pieces of evidence that support the theory of early cosmic inflation, including the uniformity of the cosmic microwave background radiation, the large-scale structure of the universe, and the abundance of light elements. These observations are consistent with the predictions of cosmic inflation.

4. How does early cosmic inflation relate to the Big Bang theory?

Early cosmic inflation is thought to have occurred immediately after the Big Bang, and is considered to be a crucial component of the Big Bang theory. It helps to explain some of the observed features of the universe, such as its large-scale homogeneity and isotropy.

5. What are some current challenges in understanding early cosmic inflation?

One of the biggest challenges in understanding early cosmic inflation is the lack of a complete and consistent theory that can explain all of its features. Additionally, there are questions about the duration of inflation and the properties of the inflaton field that are still being investigated by scientists.

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