Well, as the title asks, are the physical constants of the universe (such as plank's constant or the gravitational constant) rational or irrational numbers?
One can pick units for which some constants are rational numbers. But even if one were to do this, some of them still
must be irrational. For example, with the right set of units one could make hbar a rational number. But then h would necessarily be irrational. Conversely, if one makes h rational, then hbar must be irrational. Same thing for k and epsilon (two different forms of the constant for Coulomb's law): they're related by irrational numbers, so they cannot both be rational (but they can both be irrational).
I sure can't see a ready fraction in any of them, but then again these numbers are determined experimentally, so how can you tell for sure.
You can't. But as mentioned above, since units are arbitrary and generally we don't pick them based upon fundamental constants, the probability is rather overwhelmingly in favor of any fundamental constant with units being irrational.
How about the universe itself? Is there a countable number of states for it?As a layman I understand that units of dimensions in the universe are quantified in various Plank units, so that would seem to say that these must be countable, but is this the case?
No, that is not the case.
It's a common misconception that the Planck scales represent some sort of fundamental quantization of the universe. That is not the case. Or to be more precise, we have no evidence that this is the case. The significance of these scales is something rather different, namely the intersection of quantum mechanics and general relativity.
Let's think about length and mass/energy. In general relativity, a given mass will have an associated length scale, the Schwarzchild radius, which describes how small you need to get that mass in order to turn it into a black hole. If you're much further away from that mass than this length scale, then even if it IS a black hole, the gravitational field at that distance will still behave like Newtonian gravity. Which means you can essentially ignore general relativity. Conversely, if you're at distances from your mass of similar magnitude to this length scale, then even if it hasn't actually collapsed into a black hole, general relativistic effects will still be strong. So for a given mass, this distance characterizes the crossover from where you can ignore GR to where you must include GR. Now, the larger you make your mass, the longer this length scale will be.
We can do something very similar with quantum mechanics. Pick an energy, and you can associate a length scale, for example, the wavelength of a photon with that energy or the de Broglie wavelength of a particle. If we're at distances much larger than this wavelength, we can often ignore quantum effects, but below this length we definitely need to consider quantum mechanics. So that idea of a crossover is the same as with GR, but unlike GR, this length gets
smaller as we increase out mass.
Now, let's start out by considering a very small mass/energy, much smaller than an electron. The quantum length scale is large, and the GR length scale is tiny. Now we start increasing the mass we're considering. The quantum length scale decreases, and the GR length scale increases. At some point, if we increase our mass enough, the two length scales will cross. This happens at the Planck mass, and the length is the Planck length. That's really the only thing either of those things definitely indicate.
But that's not
quite the end of the story. If it were, they might be nothing more than a curiosity. The question is, what
happens at these scales? And the answer is that we just don't know. The problem is that quantum mechanics and general relativity don't agree with each other. That's usually not a problem: almost everything in the universe interacts under conditions where we're in the quantum OR general relativity regime (or neither). So we can almost always ignore either quantum mechanics or general relativity, if not both. That means that we can get away without resolving that conflict. But if we got down to the Planck scales (which require fantastically large energy densities), then we wouldn't be able to ignore either GR or quantum mechanics, and we can't make predictions without knowing how to resolve that conflict. Now, some people
speculate that some additional quantization of space itself happens at these scales, and that this additional quantization may resolve the conflict, but that's just speculation. We really don't know. And since we can't get anywhere near that density for practical reasons, we can't do direct experimentation to study such conditions either. But as it stands now, the Planck scales should be thought of as a limit to our understanding, not as a limit to space itself.