SpaceTiger said:
I'm not quite sure what you mean.
I'm not either. :-) Cosmology is fascinating. I once
read a book called Frozen Star (or something like that), and
have picked up bits and pieces here and there. However,
I have only a very pedestrian, very naive apprehension of
the field. For example, I don't know what it means to say
(that is, how it's calculated) that some galaxies are moving
away from us at superluminal speeds.
Anyway, thanks (and to others too) for replying.
What's a good intro to the nuts and bolts of cosmological
model-making? Not too advanced, but I'm ok with algebra,
linear algebra, calculus, the usual intermediate stuff.
So, something along the lines of a more conceptual
intro -- but not just a popularization of it.
I haven't gotten around to reading all the journals
of the advisors and mentors here yet. This hasn't been
my main area of interest, but I can see how one could
get hooked on cosmology.
SpaceTiger said:
The recession speed of galaxies increases with distance from the earth, eventually going well beyond the speed of light. There is a distance at which galaxies are receding at approximately the speed of light, but this distance is not important. If we were viewing the universe from another galaxy, the "sphere" inside which galaxies were receding at less than the speed of light would be different.
As for the expansion rate (parameterized by the Hubble constant), that's usually assumed to be independent of position, by the cosmological principle. The recession velocity of galaxies relative to us is not a measure of the expansion rate because it depends on distance. To first order:
v_r=H_0d
where H0 is hubble's constant and d is the distance from us.
That the recession velocity increases with distance was
part of my consideration. I assumed that the isotropic expansion
rate also increases with distance from us, and that the speed of
light in vacuum also increases with distance from us. Then,
assuming a finite, bounded universe, the expansion rate (and the
speed of light) would reach a maximum at the boundary. And,
then I wondered if the (finite) expansion rate could be related
to the finite propagational rates of all the phenomena that
we're familiar with, including light -- in some limiting sense.
Which all had to do with *first* wondering about whether it
would be possible for an object inside our universe to
accelerate beyond the boundary, and also about what
the physical basis for inertia might be.
As you can see, this is a bit ... scattered. I think I really
need that intro. :-)