Jason Wright said:
I understand that right-handed neutrinos do not interact by the weak force, so we would not detect them. My question is why we read that they might not / probably do not even exist.
Where did you read this? It is difficult to answer your questions if we do not know what you have read.
The bottom line is, we don't know if they exist or not. We currently have no experimental evidence of their existence.
Jason Wright said:
With electrons, their mass couples their left- and right-handed chiral states, so they oscillate between the two. If they are Dirac particles, shouldn't neutrinos do the same?
We currently do not know the origin of neutrino masses. They
could be Dirac particles and get their mass from the Higgs vev and the corresponding Yukawa couplings just like the charged fermions, but we also have no evidence that this is the case either. We simply do not know and there are may different models for neutrino masses out there.
I would say that the main reason why high-energy physicists dislike Dirac neutrinos with just the addition of right-handed neutrinos and neutrino Yukawas to the Standard Model is that those Yukawas would have to be extremely small. Many already consider it a problem that the electron Yukawa is so much smaller than the top Yukawa and the neutrino Yukawas would be orders and orders of magnitude smaller still.
In addition, as soon as you introduce right-handed neutrinos (or, equivalently, Standard Model-singlet fermions) into your theory, something happens that does not happen for charged fermions. Not only is the Yukawa coupling between left- and right-handed neutrinos allowed, but since the right-handed neutrino is a Standard Model singlet a Majorana mass term for it would not be forbidden by gauge invariance and it becomes a free parameter with mass dimension in the Lagrangian for which you have no real handle on what scale it should be in. If you let the Yukawas have a size of order one and set a very high scale for the Majorana mass of the right-handed neutrinos (ca 10
15 GeV), then you will naturally get very small Majorana masses for the left-handed neutrinos as a result. This is the very popular seesaw mechanism (more precisely, a type-I seesaw), which is one of the more widely considered models for describing the lightness of active neutrinos.
However, there are also other ways of introducing neutrino masses that do not require the introduction of right-handed neutrinos, for example the type-II seesaw mechanism.
Jason Wright said:
Is it observationally permitted that the Universe is filled with right-handed neutrinos (either primordial or having oscillated from the left-handed chirality), or do are there constraints from, for instance, cosmic neutrino detectors or cosmology that rule this out?
There are some models where right-handed neutrinos are dark matter candidates (or rather, the neutrinos that are dominantly right-handed, there would be a small mixing angle to the light neutrinos). You typically cannot oscillate from light neutrinos to heavy right-handed neutrinos in most situations (because kinematics would be well determined enough to tell whether you have a heavy neutrino or a light one). It is difficult to say more without a more specific model in mind.