Far from a faux pax, drunken physical questions are perhaps the best and most fruitful.
GBR said:
1. e = m*c² -- how does lightspeed come into this equation, and why is it squared?
c squared is just a proportionality constant here---it converts between our conventional units of mass, to our conventional units of energy. There are lots of other ways of explaining the presence of [tex]c^2[/tex], but I think this is perfectly sufficient for your question.
GBR said:
2. Shape of the universe: How can something have a shape if it does not occupy a tangible space? For example, if we live in a saddle shaped universe, how can we say it it is saddle shaped without any observers who are able to see it as so?
Shape doesn't just tell you how something looks from the outside; it also tells you how things behave in that environment. Try drawing a triangle on the surface of a sphere, hopefully you can convince yourself that the sum of the angles is actually larger than 180 degrees. There are other configurations where the angle would be less. In either case, this has an effect even to an observer existing within that geometry. Another example would be walking along a mobius strip---coming back to where you started.
GBR said:
3. Expansion: Can gravity have an influence between parallel universes, and can it explain expansion and dark matter (ie. our universe is getting stretched by other universes in our neighborhood)?
No. Parallel universes cannot (for the most part) interact with our universe---thats what makes them
different universes. Note also that dark
energy is the one that has to do with accelerated expansion.
GBR said:
4. Gravity waves: What if we don't find 'em?
That's really really unlikely... If you ask most astrophysicists they'll tell you we've already observed gravitational radiation (see:
http://en.wikipedia.org/wiki/PSR_B1913+16), but only indirectly. BUT, if we were to NEVER directly detect GW... i suppose it would completely change our notion of how gravity works---most notably, we'd have to throw lots of general relativity to the wind.