I just saw a really classic handling by Bandersnatch of newcomer questions by TigerDave. It is so clear and concise I want to save it as part of "effort to get us on same page"
Here is TigerDave's original post
TigerDaveJr said:
Regarding the creation of the universe and the current model:...
His paragraphs are interspersed in the following by Bander.
Bandersnatch said:
Hello, TigerDaveJr. Welcome to PF! ...
==quote Bandersnatch classic response to newcomer==
Is it assumed that the universe, at the time of creation was finite in size (or at least more finite than it is now) prior to the rapid expansion, or was the protoexistance finite in size in an infinite universe? So, did the universe AND its contents expand, or did a collection of mass within the universe expand, creating the physicality we know today?
The universe was either finite or infinite, and it still is one of those. We cannot say which one it is, but if it's finite, then it has got a very large curvature radius(~88 billion ly was the minimum estimate, iirc).
The key part to understand is that whenever you hear of the universe's expansion, it does mean the entirety of it. It's not about some matter expanding into a preexisting space, but space WITH matter and energy, expanding.
I have seen the expansion explained like a balloon. However, if this were true, would not most mass be on the 'outside' of the balloon? Is there content in the middle of the universe, or is there a hollow center that is getting bigger as we get further from the center? I've read that asking about the center is impossible, and that the universe has infinite shape, but if that's true can we say we're expanding? Would there not be an origin point, or is that one of the problems that a physics-uneducated person like myself would be unable to grasp (re: Plato's allegory of the cave).
The balloon analogy is not perfect, as it creates this erroneous intuition that there is something outside(or inside) the balloon, due to the way we imagine it being a three dimensional object.
The analogy requires you to think of only the surface of the balloon as the universe.
There is no centre to a 2d surface(but there is curvature), and the expansion is still easily observable by comparing the distances between any two points on that surface at two different times.
These two pages go into more detail about the balloon analogy, its aims and limitations, all in layman's terms:
http://www.mso.anu.edu.au/~charley/papers/LineweaverDavisSciAm.pdf (first page is blank)
http://www.phinds.com/balloonanalogy/
Can we not use red shift in order to determine the relative center of this expansion? I understand that we observe red shift based upon where we're standing, but should we not be able to calculate from all that where the overall center is? Where are we in regards to this?
You should see from the above links that it is impossible to define a centre of uniformly expanding space.
You can easily define the centre of the
observable universe, which is wherever you are standing.
Was expansion more like bread dough? Did the pre-expansion material tear? Was that tearing uneven, that left behind general emptiness in some spots and densely clumped matter in others that led to our original star nurseries?
You are taking the analogy too far. Of course the universe is not made of dough, so it does not tear like dough does. It is important to limit yourself to only what the analogy is trying to convey(i.e., the expansion of space) and not to go overboard with drawing conclusions from it.
Are galaxies considered expanding or collapsing? I've heard that there's supposed to be black holes in the center, so is this local mass "going down the drain" or is this mass being spun off from the center? Is it both? Do we consider galaxies to be generally "on par" with each other in the creation of more complex atomic structures, or do we expect each birth/nova/collapse/rebirth cycle of stellar material to continually generate more complex material, and that individually from galaxy to galaxy?
Galaxies are stable structures, with no significant amount of mass going down the black hole or escaping.
Sure there might be some rogue star gaining enough speed from random gravitational interactions to fling itself into the intergalactic space, and there tends to be some gas falling down the black hole - mostly because it takes so long to actually get there.
But overall, there is no expansion or collapse. The expansion of space does not affect small scale structures(like galaxies), and the black holes are not the voracious vacuum cleaners of doom that you might sometimes see in the popular media. Most stars stay in pretty much stable orbits around the galactic centre, and it's not going to change much, barring collisions with other galaxies.
All the galaxies coalesced from the same primordial gas, and the laws of physics governing them are the same, so it stands to reason that they are similar.
The difference is in the time scale. As you look farther away, you see younger galaxies, and the younger the galaxy, the less time its stars have had to go through their life cycles and produce heavier elements.
Generally the longer the universe exists, the more heavy elements it contains(in the early universe there was only hydrogen, helium and some lithium).
Second to last, is it possible, in the same way that we view time against the overall amazingness of deep time, that this initial universal expansion was just one bubble in an even larger sea of expanding pockets that we have yet to get close enough to see the evidence of? Not getting into dimensions, but is our universe just one in an entire "hyper-universe" of immense activity, that we can't directly "observe" in the same way that our tiny blip of existence fits in the concepts of deep time?
It's a kind of a vague and dangerously philosophical-sounding question, but I suppose it asks about the multiverse hypothesis?
As you say, it's not observable, therefore not falsifiable, which makes it an empty question really.
The first half an hour or so of this talk by Lee Smolin:
http://pirsa.org/13020146/
touches on the subject.
Finally and most importantly, where should I be aiming myself educationally in order to learn the answers to these questions, and to ask even more?
I'd recommend starting here:
http://www.astro.ucla.edu/~wright/cosmolog.htm
and going through either/both tutorial or/and FAQ.
Stephen Weinberg's "First three minutes" is a classic book concerning the early expansion of the universe. It's a bit dense at times, and getting somewhat old, but still worth reading.
Alan Guth's "The Inflationary Universe" talks about the birth of the idea of inflation, that is a major(if still somewhat dodgy) part of current cosmology.
Finally, understanding Relativity might be necessary. This popular treatment by Einstein himself is a good start:
http://www.gutenberg.org/files/30155/30155-pdf.pdf
You should be able to understand the ideas without any maths knowledge, but once you dig deeper into cosmology, you'll notice that it's at its heart a mathematical science, requiring you to learn higher mathematics to truly understand what's going on.
Unless you do that, you'll have to do with imperfect analogies, so if you have such an option, take calculus and algebra courses.
Finally, you might find the courses/videos on these sites relevant to your interests:
http://www.perimeterinstitute.ca/video-library (you probably want the "public lectures" section)
http://www.academicearth.org/ (try astronomy section)
https://www.coursera.org/ (actual online courses; physics section covers cosmology as well)
https://www.khanacademy.org/ (not a lot on cosmology, but good for learning maths and basic physics concepts)
==endquote Bandersnatch==