Cosmic inflation and singularity

In summary, cosmic inflation and the concept of singularity play significant roles in understanding the chronology of the universe. Inflationary cosmology suggests that times before the end of inflation do not follow the traditional big bang timeline and the universe before the end of inflation was a very cold near-vacuum. The traditional Planck epoch is also absent in inflationary cosmology, though similar conditions may have existed in a pre-inflationary era. Reheating marks the end of inflation and the beginning of ordinary Big Bang expansion. However, even in inflationary spacetimes, an initial singularity is expected to exist. This raises questions about the need for quantum gravity to resolve the singularity. Overall, while the exact nature of the singularity
  • #1
sshai45
86
1
"Cosmic inflation" and singularity

Hi.

I saw this on Wikipedia:
http://en.wikipedia.org/wiki/Chronology_of_the_universe#Planck_epoch

In inflationary cosmology, times before the end of inflation (roughly 10−32 second after the Big Bang) do not follow the traditional big bang timeline. The universe before the end of inflation was a very cold near-vacuum and persisted for much longer than 10−32 seconds. Times from the end of inflation are based on the big bang time of the non-inflationary big bang model, not on the actual age of the universe at that time, which cannot be determined in inflationary cosmology. Therefore, inflationary cosmology lacks a traditional Planck epoch—though similar conditions may have prevailed in a pre-inflationary era of the universe.

Later:

Inflation ended when the inflaton field decays into ordinary particles in a process called "reheating", at which point ordinary Big Bang expansion began. The time of reheating is usually quoted as a time "after the Big Bang". This refers to the time that would have passed in traditional (non-inflationary) cosmology between the Big Bang singularity and the universe dropping to the same temperature that was produced by reheating, even though, in inflationary cosmology, the traditional Big Bang did not occur.

If there was no "traditional Big Bang" with inflationary cosmology, would this remove the singularity at the beginning of the universe? If so, then what is all the hubbub about using quantum gravity and so forth to resolve this "singularity"? Hasn't "inflation" theory been a mainstream component of the standard picture of cosmology for a while now? If not, does that mean the singularity still existed, just further back in time? Note that in that previous quote it says with regard to the Planck epoch that "similar conditions may have prevailed in a pre-inflationary era of the universe" -- could this be it, or something 'close' to the supposed singularity that needs "resolving"? However, it only says "may" -- could it be that they didn't, and there was no singularity ever ever, and so it's resolved right there, just like that?
 
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  • #3
bapowell said:
It is expected that even inflationary spacetimes are not past-eternal, i.e. there is still an initial singularity to contend with. See: http://arxiv.org/abs/grqc/0110012

So then there'd ultimately be a "real Big Bang" some unknown time interval before the point marked "end of inflation"? How far back could it be, anyways?
 
  • #4
Sure, or if not a real big bang, some other sort of quantum cosmological genesis event. I don't know how far back it could be...my suspicion is "quite far".
 
  • #5



Thank you for your question. Let's start by defining what we mean by "singularity" in the context of cosmology. A singularity refers to a point in time where the laws of physics break down and our current understanding of the universe cannot explain what happened. In the traditional Big Bang model, the singularity occurs at the beginning of the universe, when it is believed that all matter and energy were condensed into a single point of infinite density and temperature.

However, with the theory of cosmic inflation, this singularity is no longer necessary. Inflation proposes that the universe underwent a rapid expansion in the first fractions of a second, stretching out the fabric of space-time and smoothing out any irregularities. This means that the universe was not condensed into a single point, and therefore there is no need for a singularity.

So to answer your question, if the universe did not undergo a traditional Big Bang, then there is no singularity at the beginning of the universe. The idea of using quantum gravity to resolve the singularity comes from the traditional Big Bang model, where the laws of physics break down at the singularity. However, with inflation, this is no longer a problem.

Inflation theory has been a mainstream component of the standard model of cosmology for a while now, and it has been supported by various observations such as the cosmic microwave background radiation. The "pre-inflationary era" mentioned in the quote refers to the period before inflation, where conditions may have been similar to those at the Planck epoch. However, this is still a topic of ongoing research and is not yet fully understood.

In conclusion, the theory of cosmic inflation does remove the need for a singularity at the beginning of the universe. It is a well-supported theory in the scientific community and has helped to explain many mysteries of the universe. You are correct in thinking that the singularity has been resolved with inflation theory, and it is no longer a major concern in cosmology.
 

What is cosmic inflation?

Cosmic inflation is a theory in cosmology that proposes that the universe underwent a rapid and exponential expansion in the first moments after the Big Bang. This expansion is thought to have occurred at a rate faster than the speed of light and lasted for a fraction of a second, causing the universe to grow from a tiny, incredibly dense point to a vast and relatively uniform state.

How does cosmic inflation explain the structure of the universe?

Cosmic inflation is thought to have smoothed out any irregularities in the early universe, resulting in the uniform and isotropic distribution of matter and energy that we observe today. This theory also explains the large-scale structure of the universe, such as the formation of galaxies and galaxy clusters.

What is a singularity?

A singularity is a point in space and time where the laws of physics break down and become infinite. In the context of cosmic inflation, a singularity refers to the initial state of the universe, where it was infinitely dense and hot.

Can cosmic inflation be proven?

Currently, there is no direct evidence for cosmic inflation, but there is a substantial amount of observational evidence that supports its predictions, such as the uniformity of the cosmic microwave background and the large-scale structure of the universe. However, further research and observations are needed to fully confirm the theory.

What are the implications of cosmic inflation and singularity for our understanding of the universe?

The theory of cosmic inflation and the concept of a singularity have significant implications for our understanding of the origin and evolution of the universe. They provide a framework for explaining the structure and composition of the universe and offer potential explanations for some of the most fundamental questions in cosmology, such as the horizon problem and the flatness problem.

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