I Why Is a Flat Universe Infinite?

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I cannot find an answer online. Help please.
 
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albie said:
Why Is a Flat Universe Infinite?
If it is unbounded (has no edge), then flat space is infinite for the same reason a flat Euclidean 2d surface (flat unbounded paper say) must be infinite. If it is positively curved (like the surface of Earth), then it can be finite despite the lack of an edge.
 
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Because our models of the universe are everywhere homogeneous and isotropic. Something with an edge isn't homogeneous and the only way to get a flat universe with finite volume is to wrap it into something like a torus, and that isn't isotropic.
 
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Ibix said:
Because our models of the universe are everywhere homogeneous and isotropic. Something with an edge isn't homogeneous and the only way to get a flat universe with finite volume is to wrap it into something like a torus, and that isn't isotropic.
One should be able to wrap around the faces of a three-cube so that the left face is identified with the right face, the top face with the bottom face and the front face with the back face. This is the three dimensional analogue of the screen in Asteroids or Pac Man.

This could be finite, flat and isotropic

A torus embedded in three space and using the induced metric is indeed not isotropic. But there is no requirement that the space in question be embedded in a higher dimensional space or that it use the induced metric.

Or am I missing something? Never having taken a course in topology, such is a possibility...

Oops. I am missing something. If you lay out a grid of landmarks in the wrapped-around three-cube, there are directions where you can lay down more landmarks before seeing a repetition. The space has a detectable directionality. It may be homogeneous on a large scale, but it is not isotropic if you look carefully. Or, looking at it another way, there are countably many angles at which you can look down grid lines with rational slopes and see yourself. Distributed in a way that makes the grid obvious if you can measure distance. Plus uncountably many angles with irrational slopes along which the sight line never intersects any of your wrapped around positions.
 
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Ibix said:
Because our models of the universe are everywhere homogeneous and isotropic. Something with an edge isn't homogeneous and the only way to get a flat universe with finite volume is to wrap it into something like a torus, and that isn't isotropic.
But why should a universe in case it is anisoptropc and the cosmological principle doesn't hold but which is still in the frame of the EFE have an "edge"?
 
timmdeeg said:
But why should a universe in case it is anisoptropc and the cosmological principle doesn't hold but which is still in the frame of the EFE have an "edge"?
I'm not sure what you mean. I was saying a homogeneous and isotropic universe can't have an edge if it's flat. But non-homogeneity doesn't imply an edge - for example Kerr spacetime is non-homogeneous and doesn't have an edge.
 
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Ibix said:
I'm not sure what you mean. I was saying a homogeneous and isotropic universe can't have an edge if it's flat. But non-homogeneity doesn't imply an edge - for example Kerr spacetime is non-homogeneous and doesn't have an edge.
Sorry, I misunderstood you.
 
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Ibix said:
Because our models of the universe are everywhere homogeneous and isotropic. Something with an edge isn't homogeneous and the only way to get a flat universe with finite volume is to wrap it into something like a torus, and that isn't isotropic.
Sorry but doesn't make sense to me. Are you saying that an infinite universe has planets and stars going on for ever or are you saying that scientists are counting the void beyond the universe as part of our universe?

You use words like 'homogenous' and 'isotropic' but that implies a measurement. How can you measure infinity?
 
albie said:
Are you saying that an infinite universe has planets and stars going on for ever
Yes. That's what "homogeneous" means - the same everywhere.
albie said:
or are you saying that scientists are counting the void beyond the universe as part of our universe?
There is no such thing that we're aware of.
albie said:
You use words like 'homogenous' and 'isotropic' but that implies a measurement.
No, it implies a judgement that what we can see and measure of the universe means that modelling it as homogeneous is sensible. It clearly isn't homogeneous on the small scale (punch the air then punch a table and see if it feels the same), but if we look out further and further on larger scales the more same-y everything looks. Thus we make an assumption that on really large scales everything is more or less the same, feed that in to our maths, and see what it says. What it says turns out to include prediction of the cosmic microwave background and cosmological redshifts (subsequently confirmed by observation), and that there are three classes of possible universe of this type, two of which are infinite.
albie said:
How can you measure infinity?
We can't. What we can do is extrapolate based on what we can see of the universe, and that extrapolation says the universe is either infinite, or a closed 3-sphere that is very very large.
 
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Ibix said:
Because our models of the universe are everywhere homogeneous and isotropic. Something with an edge isn't homogeneous and the only way to get a flat universe with finite volume is to wrap it into something like a torus, and that isn't isotropic.
Well, but, that our models of the universe are homogeneous and isotropic does not necessarily mean that the real universe is also. It could be that the real universe is a finite flat torus of a volume several orders larger than the observable universe.
 
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albie said:
You use words like 'homogenous' and 'isotropic' but that implies a measurement.
There is no such logical implication. Homogeneous and isotropic can and do apply to a (mathematical) model of our universe. These properties are used to make predictions of what can be measured. The measurements, as in all physics, in general either corroborate the model or not.
albie said:
How can you measure infinity?
The infinite extent of our universe may always be something of a conjecture. Note that not everyone agrees with this. For example, we know with certainty that the Earth is finite. It's not clear what experiment could confirm with certainty that our universe is infinite.
 
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  • #12
Jaime Rudas said:
Well, but, that our models of the universe are homogeneous and isotropic does not necessarily mean that the real universe is also. It could be that the real universe is a finite flat torus of a volume several orders larger than the observable universe.
Of course. But it seems odd that the universe is locally isotropic but globally anisotropic - why wouldn't whatever process picked out the special directions in the topology not affect mass distribution and geometry? It's not impossible, no, but it's adding complexity to the model in a way that is deliberately undetectable and with no theoretical justification beyond "it could be true".

So yes, the universe could be more complicated than our extrapolation because you can always invoke additional complexity with the only constraint being that it can't affect the model's predictions for existing measurements. But in that case why stop at a torus? We could have a universe shaped like a taurus, as long as the scale is sufficiently large.
 
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  • #13
Jaime Rudas said:
It could be that the real universe is a finite flat torus of a volume several orders larger than the observable universe.
But in the absence of any evidence for this, your proposed model here gets scraped right off by Occam's Razor.
 
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  • #14
The universe has no boundary or edge.
A 2D flat surface with no boundary or edge must be infinite.

We use "flat" to mean a 3D analogy to the 2D term. This is one of the properties carried over by analogy. Put another way, if it did not have this property, we'd probably call it something else.
 
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  • #15
Vanadium 50 said:
A 2D flat surface with no boundary or edge must be infinite.
A flat 2-torus is a counterexample to this. Such a manifold can't be embedded in Euclidean 3-space (as an ordinary curved 2-torus can), but that doesn't mean it doesn't exist.
 
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  • #16
Ibix said:
It's not impossible, no, but it's adding complexity to the model in a way that is deliberately undetectable and with no theoretical justification beyond "it could be true".
Yes, that's right, there is currently no theoretical justification for it, but there might be in the future. For example, if in the future it were discovered that the total energy can't be infinite.
 
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  • #17
Jaime Rudas said:
there is currently no theoretical justification for it
There is currently no observational justification for it. It's perfectly possible to construct theoretical models with the property you describe. We just don't see any evidence for them.

Jaime Rudas said:
if in the future it were discovered that the total energy can't be infinite
Any such "discovery" would have to be experimental.
 
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  • #18
Ibix said:
Yes. That's what "homogeneous" means - the same everywhere.

There is no such thing that we're aware of.

No, it implies a judgement that what we can see and measure of the universe means that modelling it as homogeneous is sensible. It clearly isn't homogeneous on the small scale (punch the air then punch a table and see if it feels the same), but if we look out further and further on larger scales the more same-y everything looks. Thus we make an assumption that on really large scales everything is more or less the same, feed that in to our maths, and see what it says. What it says turns out to include prediction of the cosmic microwave background and cosmological redshifts (subsequently confirmed by observation), and that there are three classes of possible universe of this type, two of which are infinite.

We can't. What we can do is extrapolate based on what we can see of the universe, and that extrapolation says the universe is either infinite, or a closed 3-sphere that is very very large.

Ibix said:
Yes. That's what "homogeneous" means - the same everywhere.

There is no such thing that we're aware of.

No, it implies a judgement that what we can see and measure of the universe means that modelling it as homogeneous is sensible. It clearly isn't homogeneous on the small scale (punch the air then punch a table and see if it feels the same), but if we look out further and further on larger scales the more same-y everything looks. Thus we make an assumption that on really large scales everything is more or less the same, feed that in to our maths, and see what it says. What it says turns out to include prediction of the cosmic microwave background and cosmological redshifts (subsequently confirmed by observation), and that there are three classes of possible universe of this type, two of which are infinite.

We can't. What we can do is extrapolate based on what we can see of the universe, and that extrapolation says the universe is either infinite, or a closed 3-sphere that is very very large.

>>
No, it implies a judgement that what we can see and measure of the universe means that modelling it as homogeneous is sensible.
I asked if it was a measurement and then you said no but then used the word measurement in the same sentence. Just saying.

>>or a closed 3-sphere that is very very large.
So it isn't certain that the universe is infinite and flat. I will research a closed 3-sphere. Thanks for that.

Also, how do we gauge that the universe is not curved? Wouldn't a curved universe appear to be flat even to instruments? If we are searching for microwaves wouldn't we see an infinite loop if we went looking for them? if the universe was curved, I mean.
 
  • #19
albie said:
I asked if it was a measurement and then you said no but then used the word measurement in the same sentence. Just saying.
I said the infinite size was an extrapolation from measurements, not a measurement itself.
albie said:
So it isn't certain that the universe is infinite and flat. I will research a closed 3-sphere. Thanks for that.
Infinite and flat is our current best fit model, but infinite and negative curvature or finite and closed (but very large) are both possibilities.
albie said:
Also, how do we gauge that the universe is not curved?
You can measure the scale of the fluctuations in the cosmic microwave background. How they look depends slightly on the curvature of spacetime.
 
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  • #20
albie said:
I asked if it was a measurement and then you said no but then used the word measurement in the same sentence. Just saying.
Ibix said:
I said the infinite size was an extrapolation from measurements, not a measurement itself.
Note that this is actually quite a general phenomenon. We observe or measure something, which leads us to propose something we can't actually directly measure, which lets us make new predictions.

For example we notice that when we let go of things they fall. From careful numerical study we eventually realise that there are patterns to the way things fall and propose a force of gravity. From that we can predict things like the location of planets we haven't seen yet. But nobody has ever seen "the force of gravity". You can't go to a museum or a zoo or something and see the force of gravity - you can only see that when we drop things they fall. The force of gravity is a model that is based on numerical analysis of observational data and can be used to make predictions.

Similarly we have observational data on our region of the universe, and it looks reasonably homogeneous and isotropic. So we try assuming that the whole universe is homogeneous and isotropic. Given our model of gravity, this assumption implies that the universe is either negatively curved and infinite, flat and infinite, or positively curved and closed, and is expanding (or if it is closed, it may be contracting). Further measurements tell us that the universe is either flat or very nearly so and expanding.

So "the universe is spatially flat and infinite" is a true statement about one model of the universe. It's the model that best fits the observations, but it is not directly an observation or measurement itself. It would be foolish to discard the model's claims about the rest of the universe out of hand, because it rests on fairly solid foundations, but it is a model and we can only measure things about the part of the universe we can see.
 
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  • #21
To be honest, one should mention the "Hubble tension", i.e., the difference in the determination of the Hubble constant when measured via "early-time probes" (like the fluctuations of the CMBR and based on the assumption of the concordance ##\Lambda\text{CDM}## standard model of cosmology) and "late-time probes" (model independent determinations of the distance-redshift relation). Despite the problems with the latter "model-independent determinations" due to trouble with dust, etc., the discrepancy seems to consolidate recently also using other observables. Despite possible systematic quibbles one explanation could be that we live in a less dense region than on average. Here's a pretty recent review:

https://doi.org/10.1088/1361-6382/ac086d (open access)
 
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  • #22
vanhees71 said:
Despite the problems with the latter "model-independent determinations" due to trouble with dust, etc., the discrepancy seems to consolidate recently also using other observables. Despite possible systematic quibbles one explanation could be that we live in a less dense region than on average. Here's a pretty recent review:

https://doi.org/10.1088/1361-6382/ac086d (open access)
It's not clear to me what this has to do with the topic of the thread, but a more recent review on the issue of tension in ##H_0## can be seen here:

https://arxiv.org/pdf/2308.01875.pdf
 
  • #23
Ibix said:
I said the infinite size was an extrapolation from measurements, not a measurement itself.

Infinite and flat is our current best fit model, but infinite and negative curvature or finite and closed (but very large) are both possibilities.

You can measure the scale of the fluctuations in the cosmic microwave background. How they look depends slightly on the curvature of spacetime.
>>You can measure the scale of the fluctuations in the cosmic microwave background. How they look depends slightly on the curvature of spacetime.

How much of the universe have we mapped for microwaves? to the limits of the supposed edge or just as far as our instruments allow? Could the universe be flat as far as we have measured and still have an edge?
 
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  • #24
albie said:
Could the universe be flat as far as we have measured and still have an edge?
There's no working theory that would allow such a thing. For example, what would happen to a light beam that reaches the edge?

In general, physics isn't about "what could possibly be the case". It's more about proposing a model that satisfies the observed phenomena as simply as possible.

For example, if you were a physics graduate and spent your time trying to find mathematical models where the universe has an edge, you'd be largely wasting your time.

There's also a difference between purposeful speculation (e.g. in proposed theories of quantum gravity) and idle speculation (is there a zoo of pink unicorns at the edge of the universe).
 
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  • #25
albie said:
How much of the universe have we mapped for microwaves?
I don't think you understand what the microwave background is.
albie said:
to the limits of the supposed edge
There is no edge as far as we are aware, so this is meaningless.
albie said:
just as far as our instruments allow?
The CMB comes from the last scattering surface, which is the time at which the matter in the universe cooled enough to become transparent to electromagnetic radiation. We can't see further than that because light emitted further away was either emitted before the universe became transparent, or too far away to have had time to reach us.
albie said:
Could the universe be flat as far as we have measured and still have an edge?
Our best answer to this is no. Our models could be wrong, of course, but edges are hugely problematic. Any model that includes an edge would need to answer questions like what having an edge to the universe even means. What happens to things that reach the edge? Why is everything the same everywhere except at the edge? What's beyond the edge? How can we write laws of physics that work in a finite region and forbid anything from existing outside that region? Or are somehow discontinuous at the edge?

It raises way more questions than the zero questions that it answers.
 
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  • #26
Ibix said:
I don't think you understand what the microwave background is.

There is no edge as far as we are aware, so this is meaningless.

The CMB comes from the last scattering surface, which is the time at which the matter in the universe cooled enough to become transparent to electromagnetic radiation. We can't see further than that because light emitted further away was either emitted before the universe became transparent, or too far away to have had time to reach us.

Our best answer to this is no. Our models could be wrong, of course, but edges are hugely problematic. Any model that includes an edge would need to answer questions like what having an edge to the universe even means. What happens to things that reach the edge? Why is everything the same everywhere except at the edge? What's beyond the edge? How can we write laws of physics that work in a finite region and forbid anything from existing outside that region? Or are somehow discontinuous at the edge?

It raises way more questions than the zero questions that it answers.
>>The CMB comes from the last scattering surface, which is the time at which the matter in the universe cooled enough to become transparent to electromagnetic radiation. We can't see further than that because light emitted further away was either emitted before the universe became transparent, or too far away to have had time to reach us.

So we haven't mapped far enough to determine if there is an edge or curves.

>>
Any model that includes an edge would need to answer questions like what having an edge to the universe even means. What happens to things that reach the edge?

Surely the universe is space time therefore beyond the edge would be literally nothing(no space or time) until matter and energy reach into it and create more space time.
We know this happened with the big bang so why cannot it be a good model?
 
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  • #27
albie said:
So we haven't mapped far enough to determine if there is an edge or curves.
If it's actually infinite, you will always be able to make this claim. Adding an edge and all it entails just out of sight isn't wrong per se, but it's unjustified and unfalsifiable, which ought to be a warning.
albie said:
Surely the universe is space time therefore beyond the edge would be literally nothing(no space or time) until matter and energy reach into it and create more space time.
The point is that "beyond the edge of the universe" isn't necessarily a thing that makes sense, since position and time are concepts provided by spacetime. That's one reason why an edge is difficult to deal with.
albie said:
We know this happened with the big bang so why cannot it be a good model?
I don't think we do know that. An infinite universe was always infinite in size. And we know that there is a singularity in our naive models that is often described as a "beginning of the universe", but the singularity is actually our models breaking down. So we know that the model is inaccurate, and we can only say that the Big Bang singularity is the beginning of the model and we do not know how the real universe behaved. More sophisticated models avoid the singularity in one way or another, but then there isn't a start to the universe in those models either.
 
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  • #28
albie said:
Surely the universe is space time therefore beyond the edge would be literally nothing(no space or time) until matter and energy reach into it and create more space time.
We know this happened with the big bang so why cannot it be a good model?
The Big Bang model is the opposite of what you claim. The model does not involve space expanding into a "void". And, space does not have an edge in the Big Bang model even if the universe is finite.
 
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  • #29
albie said:
Surely the universe is space time therefore beyond the edge would be literally nothing(no space or time) until matter and energy reach into it and create more space time.
This is nonsense. You can't "create more spacetime". Spacetime already includes time, so it already includes all of the effects that will happen over time.

albie said:
We know this happened with the big bang
We know no such thing. Where are you getting this nonsense from?
 
  • #30
PeterDonis said:
This is nonsense. You can't "create more spacetime". Spacetime already includes time, so it already includes all of the effects that will happen over time.We know no such thing. Where are you getting this nonsense from?
Why are you being rude to me? By creating more space time I meant advancing the spacetime outwards.

The most common view of the big bang is of a singularity exploding into nothingness.
 
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  • #31
albie said:
If there was no void then there must have been an obstacle. By void I mean zero dimensions.
Cosmology has progressed enormously in the past 100 years, from Einstein's General Theory of Relativity to observations of an accelerating expansion, to measuring gravitational waves.

There are unanswered questions, most notably whether there is dark matter influencing galaxy rotation curves and what causes the accelerating expansion.

Modern cosmogy does not rely on meeting with your approval. Cosmologists will continue to research and develop the theories we have. That research is not going to stop and be replaced with "ask albie what he thinks".
 
  • #32
albie said:
Why are you being rude to me? By creating more space time I meant advancing the spacetime outwards.

The most common view of the big bang is of a singularity exploding into nothingness.
The most common view is that a sufficiently coarse-grained picture of the universe can be described as a Friedeman-Lemaitre-Robertson-Walker spacetime, which has necessarily (Penrose/Hawking) singularities, where the theory breaks down, and nothing can be said about what was really going on close to these singularities.

For the rest of this exact solution of the Einstein field equations, which also implies that the "cosmological substrate" is described as some ideal fluid (which is no surprise given the coarse-graining over large spatial areas we are considering), whose "content" is defined by the corresponding equations of state, there's no "nothingness" into which something explodes. The FLRW solution simply describes the spacetime of the entire universe. The choice of the various components of the matter (+em. radiation) can be inferred from observations. The most important ones are the measurement of the angular distribution of the fluctuations of the temperature of the cosmic microwave background radiation and the distance-redshift relation (Hubble-Lemaitre relation) from measurements on supernovae, which an be taken with some conficence as "standard candles". The best-fit result is then what's described as the "history of our universe":

https://en.wikipedia.org/wiki/Physical_cosmology
 
  • #33
Ibix said:
It's not impossible, no, but it's adding complexity to the model in a way that is deliberately undetectable and with no theoretical justification beyond "it could be true".
It is not impossible, but the resulting models violate Occham’s razor and have less predictive power than current models.
 
  • #34
albie said:
Why are you being rude to me?
Pointing out that you are wrong is not rude. It's what you should expect here when you make wrong statements. Particularly when you continue to make wrong statements after it should be abundantly clear to you that your understanding of the subject is flawed and multiple people with much better understanding are trying to help you improve it, but you're not listening to them.

albie said:
By creating more space time I meant advancing the spacetime outwards.
Which is still wrong.

albie said:
The most common view of the big bang is of a singularity exploding into nothingness.
Wrong. The Big Bang was not a explosion "into" anything.
 
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  • #35
albie said:
If there was no void then there must have been an obstacle.
Wrong.

albie said:
By void I mean zero dimensions.
Wrong.

You need to stop making statements based on your flawed understanding and actually take the time to read, digest, and consider the multiple valid responses you have been given in this thread. Otherwise the discussion will just keep going in circles, which is pointless and a waste of everyone's time.
 
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  • #36
albie said:
You say having an edge is unjustified and unfalsifiable. What does that mean?
Unjustified means that there is no evidence supporting it. Unfalsifiable means that there can never be evidence against it. These are both problematic scientifically speaking. Because of these two issues there is simply no way that a model with an edge would be considered currently
 
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  • #37
PeterDonis said:
A flat 2-torus is a counterexample to this. Such a manifold can't be embedded in Euclidean 3-space (as an ordinary curved 2-torus can), but that doesn't mean it doesn't exist.
Technical point: A flat torus cannot be smoothly embedded in Euclidean 3-space. It can be ##C^1## embedded.

A simple physical model of such an embedding is to take a paper cylinder, squash it flat, and now connect its ends. No tears or stretches involved, just 'crinkling' that suggest the required non-smoothness of the formal mathematical treatment.
 
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  • #38
albie said:
The most common view of the big bang is of a singularity exploding into nothingness.

Why are you repeating this nonsensical claim, when people alreade have told you it's wrong? Now THAT is rude, because it seems you are not listening and not here to learn.
 
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  • #39
PeroK said:
Cosmology has progressed enormously in the past 100 years, from Einstein's General Theory of Relativity to observations of an accelerating expansion, to measuring gravitational waves.

There are unanswered questions, most notably whether there is dark matter influencing galaxy rotation curves and what causes the accelerating expansion.

Modern cosmogy does not rely on meeting with your approval. Cosmologists will continue to research and develop the theories we have. That research is not going to stop and be replaced with "ask albie what he thinks".
>>
Modern cosmogy does not rely on meeting with your approval.
Of course it does. It has to adhere to logic and all your models of the universe do not.
 
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  • #40
weirdoguy said:
Why are you repeating this nonsensical claim, when people alreade have told you it's wrong? Now THAT is rude, because it seems you are not listening and not here to learn.
You all are not giving me logical responses and explanations. Is it any wonder I am confused?
 
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  • #41
PeterDonis said:
Pointing out that you are wrong is not rude. It's what you should expect here when you make wrong statements. Particularly when you continue to make wrong statements after it should be abundantly clear to you that your understanding of the subject is flawed and multiple people with much better understanding are trying to help you improve it, but you're not listening to them.Which is still wrong.Wrong. The Big Bang was not a explosion "into" anything.
All you do is say "this wrong". This would go a lot quicker if you actually told me why I was wrong.
 
  • #42
PeterDonis said:
Pointing out that you are wrong is not rude. It's what you should expect here when you make wrong statements. Particularly when you continue to make wrong statements after it should be abundantly clear to you that your understanding of the subject is flawed and multiple people with much better understanding are trying to help you improve it, but you're not listening to them.Which is still wrong.Wrong. The Big Bang was not a explosion "into" anything.
Oh so the big bang wasn't an explosion of energy now? You need to go on wiki and put them right. Including all the websites I've looked at all saying just that.
 
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  • #43
albie said:
It has to adhere to logic and all your models of the universe do not.
Your problem here is that when you say "logic" you don't mean that at all. All cosmological models are mathematical models and hence are logical models, since maths is a branch of logic. What you actually mean is that the results of the model don't match your common sense. Which is true, and shouldn't really be a surprise. The universe on the large scale is nothing like your everyday experience.
albie said:
This would go a lot quicker if you actually told me why I was wrong.
He did. Several posts back up the chain Peter said:
PeterDonis said:
You can't "create more spacetime". Spacetime already includes time, so it already includes all of the effects that will happen over time.
If you didn't understand that, try asking for more explanations.
albie said:
Oh so the big bang wasn't an explosion of energy now?
No it wasn't. I don't think that even makes sense.
albie said:
You need to go on wiki and put them right. Including all the websites I've looked at all saying just that.
Where exactly on Wikipedia does it say that the Big Bang was an explosion of energy? We can't do anything about every poor source, but we can at least try on Wikipedia.

The Big Bang origin is a singularity, not an explosion.
 
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  • #44
albie said:
>>

Of course it does. It has to adhere to logic and all your models of the universe do not.
They do adhere to logic because they can be expressed mathematically. What they do not adhere to is your preconceived notions and assumptions.

albie said:
You all are not giving me logical responses and explanations. Is it any wonder I am confused?
You not accepting an explanation is not the same as us not giving an explanation.

The current models are based on the assumption that the universe at sufficiently large scales is homogenous, isotropic, and simply connected. The logic is as follows:

1) we observe that what we can see of the universe is homogenous, isotropic, and simply connected

2) we assume that we are not at a special location in the universe. (This is often called the Copernican assumption, since Copernicus introduced the idea that the earth is not the center of the universe)

3) that implies that the universe would be observed to be homogenous, isotropic, and simply connected everywhere

4) that further implies that there is no edge because the universe would not be observed to be homogenous and isotropic near an edge

5) that allows three possible shapes: a positively curved finite space, a zero-curvature (flat) infinite space, or a negatively curved infinite space.

6) observations currently are consistent with 0 curvature, implying a flat infinite space.

7) Projecting this model backwards in time leads to a universe that was hotter and denser in the past. It predicts cosmological redshift and the cosmic background radiation, both of which have been observed.

8) Projecting the model further back we eventually reach a state of infinite density, called a singularity. For mathematical reasons the singularity itself is not part of the model.

9) Just after the singularity, the universe is infinite, flat, and very extremely dense. However, we expect that our classical model breaks down at extreme densities. We are not sure exactly where it breaks down, but wherever it does will be substantially later than the singularity. Therefore, the universe (to the best of our current knowledge) was infinite as far back as our model is valid.

If you don’t understand something here then ask specific follow-up questions. Blanket assertions that it is illogical etc. are both incorrect and not productive.
 
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  • #45
albie said:
All you do is say "this wrong". This would go a lot quicker if you actually told me why I was wrong.
You have already been told, multiple times, why these statements are wrong. Yet you keep making them.

Also, your statement here goes both ways. See below.

albie said:
You all are not giving me logical responses and explanations.
"Logic" alone is not enough. Logic always starts with premises. What we are saying doesn't seem "logical" to you because you have the wrong premises somewhere. But we can't help you with that because you are not explicitly stating your premises. You are not giving us the explicit reasoning that is telling you that what we are saying is "not logical". You just keep rejecting what we're saying without explaining why.
 
  • #46
albie said:
so the big bang wasn't an explosion of energy now?
That's not what I said. I said the big bang wasn't "a singularity exploding into nothingness" (your words). Which is correct.

albie said:
You need to go on wiki and put them right. Including all the websites I've looked at all saying just that.
First, Wikipedia and pop science articles aren't good sources for learning actual science. You need to look at textbooks and peer-reviewed papers.

Second, even though the word "explosion" is indeed used often in pop science sources to describe the big bang, I'm not aware of any that say "explosion into nothingness". The "into nothingness" part is the real problem. "Explosion" is not exactly wrong, just likely to be misleading. But "into nothingness" is straight up wrong.
 
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  • #47
albie said:
"advancing outward" "expanding"

expanding on "What" ?

better.

Articulating the reasoning/inquire, implies using the concepts correctly, greater precision, less mess, obviously, logic also counts.
 
  • #48
The flat universe is NOT infinite. It can’t be. If it would never end, it could have never begun (because space = spacetime). Infinity only exists in mathematics, not in the real world.
 
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  • #49
Space =/= spacetime.
 
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  • #50
mark! said:
The flat universe is NOT infinite.
If it's flat, it must be infinite.
mark! said:
It can’t be. If it would never end, it could have never begun (because space = spacetime).
That's patently false.
mark! said:
Infinity only exists in mathematics, not in the real world.
You don't know that. Physics is an empirical science. Until the universe is shown to be finite, there remains the possibility that it is infinite.
 
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