Inflation, Mach's Principle & the Early Universe

In summary: Inflation was only a brief moment, lasting for 10-32 seconds according to different estimates. So even if every particle was isolated, it would only last for a tiny fraction of the time that the universe has been around.
  • #1
Bob3141592
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As I understand it, somewhere close to the beginning of the universe, the universe experienced an inflationary phase when the space 'underneath' object began to expand faster than c, the speed of light. Since it wasn't the objects themselves that were expanding, there was no violation of the principle that nothing can move faster than the speed of light, even though the separations between objects increased faster than c. Inflation only lasted for a brief moment, but in that time span the size of the universe increased by many orders of magnitude.

Therefore, when inflation ended, every object must have been isolated in it's own private realm. Since every other object in the universe was further away from it than light could travel, there was no exchange of forces or information or anything between objects. Each object was completely isolated, and would remain so for some time, until light from "nearby" objects could reach it. That's the same as saying until the light cone of the two objects intersected, right?

This strikes me to be a direct violation of Mach's principle, in which the inertia (and other intrinsic spatial properties like spin) of any particle is only in relation to the distribution of the rest of the mass in the universe. An alternate form of Mach's principle on Wikipedia says that "Mach2: An isolated body in otherwise empty space has no inertia." Then would a photon in a universe just come out of the inflation phase have momenta? Would an electron have spin? How could it? But if it doesn't how could it be an electron? (I presume there must have been electrons, even in the very high energy state early in the universe, since a blackbody always has a tail of low energy components, so everything couldn't have been higher energy particles, just most everything).

I'm confused about how this might work. Any help or thoughts would be appreciated.
 
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  • #2
You've got one part of this wrong. Inflation did NOT separate EVERYTHING so much that after inflation stopped they were outside each others light cone. Think about it this way: you travel for an hour at mach 4 and then spend the next million years traveling at 1 mph. Sound from your starting point would have no trouble reaching you after a modest amount of time. Everything in our "observable universe" was acted on by inflation but we still see it. There IS stuff (and you can get into theological arguments about how much) that is beyond our observable universe that DOES have the characteristic you describe of being outside our realm.
 
  • #3
Bob3141592 said:
As I understand it, somewhere close to the beginning of the universe, the universe experienced an inflationary phase when the space 'underneath' object began to expand faster than c, the speed of light.
We don't know whether inflation happened or not. As a theory, it has some successes and some major defects.

Bob3141592 said:
This strikes me to be a direct violation of Mach's principle, in which the inertia (and other intrinsic spatial properties like spin) of any particle is only in relation to the distribution of the rest of the mass in the universe. An alternate form of Mach's principle on Wikipedia says that "Mach2: An isolated body in otherwise empty space has no inertia."
Mach's principle is false http://www.lightandmatter.com/html_books/genrel/ch08/ch08.html#Section8.3 , so I wouldn't worry too much.

-Ben
 
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  • #4
Sure, we see it now. But we didn't always see it, just almost always. My question is about that short period, after inflation ends to just before any signal from any other part gets 'here.' For some short but real interval, every particle had to exist in complete isolation. Whatever details preceded or followed that period hardly matters. This utterly isolated state of the particles of the universe seems inevitable to me, yet it also seems contradictory.

Perhaps I don't understand how inflation works. Is it true that this 'utterly isolated' state must have existed? Given the size or age of the universe at the start of inflation, and the inflation rate and duration, you could calculate the duration of the isolation period. At least you could calculate the duration from some external frame - I can't imagine how you could measure time in a universe of only one particle.

So that's my question. Is it true that this 'utterly isolated' state must have existed? If so, then my second question is how long did it last? It has to be a nonzero positive value, and if it's longer than the Planck time, that would be interesting. I'd expect it would be much larger.
 
  • #5
Bob3141592 said:
For some short but real interval, every particle had to exist in complete isolation. [...] Is it true that this 'utterly isolated' state must have existed?

No, I don't think so (even assuming inflation did happen).

I think you're messing yourself up by assuming that the expansion of the universe can be measured in units of velocity. It can't. For example, Hubble observed that distant galaxies were receding from us at speeds proportional to their distance from us. Since the distances are all different, the speeds are all different.
 
  • #6
bcrowell said:
Mach's principle is false http://www.lightandmatter.com/html_books/genrel/ch08/ch08.html#Section8.3 , so I wouldn't worry too much.

-Ben

Please! That's a misleading overstatement of the facts.

That reference shows that a specific theory of gravitation (Brans-Dicke) which effectively incorporates Mach's Principle combined with GR is not compatible with experiment unless the strength of the Mach's Principle effect is set to something close to zero, leaving only the GR part.

The section title "Mach's Principle is false" quoted above is an extreme overstatement of that. Even in GR, local frame-dragging effects (linear and rotational) are entirely consistent with what might be expected from Mach's Principle. It can be shown that in trivial cases GR on its own is incompatible with Mach's Principle on the scale of the whole universe, but as we don't yet have a detailed understanding of the universe on that scale it seems premature to rule out some level of compatibility even at that level (even if it involves something new like "dark stress" or "dark angular momentum"!).
 
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  • #7
Bob3141592 said:
Sure, we see it now. But we didn't always see it, just almost always.

My aplogies, I completely misread your point and I now see it as a REALLY interesting question. I am hesitant to say that Ben might be wrong about something but I don't find his belief that it didn't happen compelling and don't yet see how it can be that you are wrong. I CAN imagine that the time of isolation would be truly tiny since from what I have read, if expansion did happen then although it expanded the size of the U enormously in percentage of its pre-inflation size, it was starting from very close to zero, so even after expansion, the size was still very very small (estimates seem to vary quite a bit but I remember one of them being 1 meter)
 
  • #8
Interesting topic/question
 

FAQ: Inflation, Mach's Principle & the Early Universe

1. What is inflation?

Inflation refers to a period of rapid expansion in the early universe, shortly after the Big Bang. It is believed to have occurred within the first fraction of a second after the universe's birth and is responsible for the large-scale homogeneity and isotropy of the universe.

2. What is Mach's Principle?

Mach's Principle is a philosophical concept that suggests that the properties of matter are determined by the distribution and motion of all other matter in the universe. In other words, the local properties of matter are influenced by the global properties of the universe.

3. How does Mach's Principle relate to inflation?

Inflation theory proposes that the rapid expansion of the universe during the early universe was driven by a field called the inflaton. The distribution and motion of this inflaton field, which is thought to be present throughout the entire universe, aligns with Mach's Principle as it influences the properties of matter on a global scale.

4. What evidence supports inflation theory?

There are several pieces of evidence that support inflation theory, including the uniformity of the cosmic microwave background radiation, the flatness of the universe, and the absence of magnetic monopoles. Additionally, observations of the large-scale structure of the universe and the distribution of galaxies also align with what is predicted by inflation theory.

5. Are there any alternative theories to inflation?

Yes, there are alternative theories to inflation, such as the ekpyrotic and cyclic models. These theories propose that the universe undergoes cycles of expansion and contraction, rather than a single period of rapid expansion. However, these models have not yet been fully supported by observational evidence and are still being studied and debated by scientists.

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