In the Light, stars, and creationism thread, I proposed a theory to reconcile a young earth with being able to see stars that are billions of light years away. The theory assumes that the Big Bang is true, however, it also assumes that the universe is bounded. In typical cosmology, it is assumed that the universe is unbounded.
Bounded means that the universe has a boundary to it. There exists an "edge" to the universe in which beyond this boundary, our universe does not exist.
In an unbounded universe, there is no "edge". The universe "wraps" around itself. So, if you are to go in any direction in a straight line, you will eventually come back to the starting point.
This is hard to conceptualize, but can be explained like a surface of a sphere. On the surface of a sphere, if you start at any point and then go in a straight line, you will eventually come back to the starting point. Now, instead a 2-D surface on a sphere, the universe is a 3-D topology that curves in on itself.
The ramifications of either of these two assumptions make for drastically different cosmological conclusions.
So, the questions are:
1. Is the universe bounded or unbounded? Why?
2. What are the ramifications of whether it is bounded or unbounded?
Is the universe bounded or unbounded?
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- McCulloch
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Post #271
McCulloch wrote:There are two ways that a space can be unbounded and Euclidean.otseng wrote:But, let's get back to a question I asked earlier. How can the universe be unbounded and Euclidean?
- It could be infinite.
- It could be a form of a torus.
I think that most cosmologists agree with you there. Not only is the mater and the energy of the universe finite, but spacetime is as well. The Big Bang was not a singularity that exploded in a pre-existing three dimensional space. The Big Bang was the origin of the actual space that we inhabit.otseng wrote:I believe that we can rule out that our universe is infinite.
Remember the old arcade game asteroids? It's universe was a flat (euclidean) screen where if you go off one side, you immediately re-enter the other. This is topologically equivalent to a torus.otseng wrote:For a (finite) torus, how would that be Euclidean?
As I understand the current model, the universe is like that, except the 2D screen has been replaced with an expanding regular solid.
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- otseng
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Post #272
I could entirely be wrong since I just came up with this on my own. But I don't see why it would be blue-shifted.QED wrote:According to your model, then if anything, photons will be blue-shifted not red-shifted!
Are you saying that the gravitational field would be the strongest in the center?
How about this. I'll read through the article and when I have questions, I'll ask those.OK, you'll probably think I'm "fobbing you off", but I think the best way for you to understand the answers to your questions is to follow Ned Wright's Cosmology Tutorial.
I didn't realize that Auden knew so much about science!(It's his centenary this year so pardon me for inserting a minor homage)
Post #273
In an idealized model, Gravity cancels out at all points inside a hollow sphere: At the exact center of a sphere, there will obviously be an equal gravitational effect from every point on the outer shell of the sphere. Moving from the center to some other point inside the sphere, as the point approaches one edge, the forces from that side become stronger than the other. However, there is a compensating change taking place as the amount of mass behind the point gets larger, and this cancels out exactly as described by Gauss's law. At any point inside a homogeneous sphere the gravity only depends on the mass within a sub-sphere whose radius ends at that point. All mass beyond this radius can be considered as collection of spherical shells as per the limiting case of the hollow sphere, and hence contributes nothing to the field inside the radius.otseng wrote:I could entirely be wrong since I just came up with this on my own. But I don't see why it would be blue-shifted.QED wrote:According to your model, then if anything, photons will be blue-shifted not red-shifted!
Are you saying that the gravitational field would be the strongest in the center?
In your spherical universe with the Earth at the centre, a photon at any point would appear to be accelerated towards the mass of the sub-sphere centred on the Earth and ending at the photon. Such an acceleration would tend to shift it to the blue end of the spectrum.
OK, I appreciate that -- but remember -- I'm not a professional Cosmologist so I can't guarantee to be able to answer everything.otseng wrote:How about this. I'll read through the article and when I have questions, I'll ask those.QED wrote: OK, you'll probably think I'm "fobbing you off", but I think the best way for you to understand the answers to your questions is to follow Ned Wright's Cosmology Tutorial.
His father was a physicist.otseng wrote:I didn't realize that Auden knew so much about science!QED wrote:It's his centenary this year so pardon me for inserting a minor homage)

Post #274
I remember reading somewhere about theories of how the early universe worked, right after the Big Bang. They said "time" didn't start immediately after. They even used the expression "before time began". That one cracked me up. The universe expanding into spacelessness also confounds me a great deal. Not that it takes much...McCulloch wrote:The Big Bang was not a singularity that exploded in a pre-existing three dimensional space. The Big Bang was the origin of the actual space that we inhabit.
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Post #275
I would not agree that they would be "topologically equivalent". But, no matter, here's some questions:McCulloch wrote:Remember the old arcade game asteroids? It's universe was a flat (euclidean) screen where if you go off one side, you immediately re-enter the other. This is topologically equivalent to a torus.otseng wrote:For a (finite) torus, how would that be Euclidean?
As I understand the current model, the universe is like that, except the 2D screen has been replaced with an expanding regular solid.
If I approach a "side" and come out on the other "side", how would the two points be causally connected?
Also, could such a side even exist if we could not perceive of crossing a side and reentering another side? If other words, how would it be detectable that a side even exists?
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Post #276
Why a hollow sphere? I would think an idealized model would be a sphere uniformly filled with points. Or even a solid sphere.QED wrote:In an idealized model, Gravity cancels out at all points inside a hollow sphere:
It made a jump here to a metric expansion of the universe. How did it get from the Hubble recession to metric expansion?Ned Wright's Cosmology Tutorial wrote:The Hubble law generates a homologous expansion which does not change the shapes of objects, while other possible velocity-distance relations lead to distortions during expansion.
As far as I know, the Copernican principle is only an assumption.Since we actually see the same redshift-distance law in all directions, either the redshift-distance law is linear or else we are at the center which is anti-Copernican.

I am stuck at understanding the red light cone in this space-time diagram. What exactly does the red line mean?
Post #277
You must have missed the transition from hollow to "solid" (homogeneous) in my explanation above:otseng wrote:Why a hollow sphere? I would think an idealized model would be a sphere uniformly filled with points. Or even a solid sphere.QED wrote:In an idealized model, Gravity cancels out at all points inside a hollow sphere:
The reason for starting out the explanation with a hollow sphere is to make clear the cancellation effect that accords with Gauss's law by considering a limiting case.QED wrote: At any point inside a homogeneous sphere the gravity only depends on the mass within a sub-sphere whose radius ends at that point. All mass beyond this radius can be considered as collection of spherical shells as per the limiting case of the hollow sphere, and hence contributes nothing to the field inside the radius.
Because the extremes of red-shift seen in distant galaxies can only be due to cosmological expansion.otseng wrote:It made a jump here to a metric expansion of the universe. How did it get from the Hubble recession to metric expansion?Ned Wright's Cosmology Tutorial wrote:The Hubble law generates a homologous expansion which does not change the shapes of objects, while other possible velocity-distance relations lead to distortions during expansion.
It's only an assumption that you and I are typical human beings, that neither of us live at the place on the planet where life first evolved (or God placed Adam and Eve if you will). And I've already pointed out how the view from the centre of an explosion would give the game away. What physical process could you possibly have in mind whereby all the material in the cosmos was first assembled where our galaxy is now and then ends up being distributed uniformly around our galaxy -- which is the only one not to have moved?otseng wrote:As far as I know, the Copernican principle is only an assumption.Since we actually see the same redshift-distance law in all directions, either the redshift-distance law is linear or else we are at the center which is anti-Copernican.
Do you understand Space-Time Diagrams? The "cosmic speed limiter" prevents lines of distance/time exceeding 45 degrees on the diagram as that angle has been chosen to represent light-speed. So for any point we might place ourselves at, such as the one at top center, then looking out and back in time, information beyond the (red) line at 45 deg, to the normal cannot reach us.otseng wrote:
I am stuck at understanding the red light cone in this space-time diagram. What exactly does the red line mean?
Post #279
Member spotlight - QED will answer your question Openmind. What little I know of Cosmology is gleaned from an interest in amateur Astronomy and a pile of paperbacks. I am deeply envious of those who are smart enough to do it for a profession.