Ibix said:
A meter is roughly as far as our monkey arms reach. A second is roughly how long it takes our monkey hearts to beat.
Neither of those is true.
The definition of the second goes back to around 1000 AD. It was based on the theory that the period of the Earth's rotation was constant. That period was divided into 24 hours, each divided into 60 minutes of 60 seconds each. So the original definition of the second was 1/86400 of the period of the Earth's rotation, and this lasted right up until the mid-20th century after it had been demonstrated that the Earth's rotation was slowing down.
The intended definition of the metre - first proposed in the 17th century - was the length of a pendulum with a half-period equal to one second. However it was discovered that this definition was dependent on fluctuations in the Earth's gravity, and so in the late 18th century a definition relating to the Earth's circumference was adopted - one ten-millionth of the distance from the North Pole to the Equator, along the meridian passing through Paris. There have been several redefinitions since then, as I mentioned in an earlier post.
The invariant speed at which light travels is simply the unit conversion factor between time and length - so in SI units it's roughly the ratio of the length of one monkey heartbeat to one monkey arm length.
The first quantitative estimate of the speed of light was made by Ole Rømer in 1670, by observation of the periods of one of Jupiter's moons. Since then it's been refined by centuries of experimentation. Michelson's 1926 experiment determining the speed of light between Mount Wilson and Lookout Mountain was probably the original basis for the value we use today, but it took until 1983 until the current standard was adopted.
What would it mean to change the speed of light?
It's difficult to know. The values of so many other physical constants are related to the speed of light that any change would have huge consequences on the rest of our theories of physics.
It turns out that what you actually want to do is vary the fine structure constant.
I don't actually
want to do anything. I am simply saying that if the value of the speed of light - or indeed the fine-structure constant, or anything else - were different outside the observable universe, we'd have no way of gathering any evidence.
The fine-structure constant, being a dimensionless constant, is independent of any system of units, and so I suppose it's in a sense more fundamental than the others; but we're no more able to gather evidence of the value of the fine-structure constant outside the observable universe than of any other value.
You are missing the point here too. We construct a model of a homogeneous universe (which turns out to imply finite but unbounded, flat, or open - but flat matches observation best) because it's simpler than any other model and pretty much consistent with what we see.
Indeed - Occam's razor, as has been mentioned before. That's a philosophical principle though, and not a scientific one.
The hypothesis being tested is not "is the universe infinite, flat, and homogeneous" but "is the universe experimentally distinguishable from our model of an infinite, flat, homogeneous one". If it's not distinguishable then our model is good (whatever the truth is about the unobservable stuff). If it is distinguishable then we need to revisit something. So far it works, with a bit of tweaking. Sure we could develop models that do other stuff outside the observable universe, but why bother? We can't test it.
No we can't. And that's why any theory of what exists outside the observable universe is unscientific.
It may well be that the universe is not experimentally distinguishable from our model of an infinite, flat, homogeneous one, but also that the universe is
not infinite, flat, and homogeneous. And there's no way of experimentally falsifying that hypothesis.
Ultimately, there are limits on what we can know about the universe, and any theory outside those limits is not a scientific theory.