ojitojuntos said:
I’m having a hard time understanding indeterminism and the notion of collapse. Does indeterminism suggest that the future of the universe is not fully “set”?
The answer is interpretation-dependent. In many worlds, for example, it is fully deterministic. Copenhagen - no. Decoherent histories (favoured by Gell-Mann and, in his final days, Feynman) sort of has a bet each way (depending on your view of 'real' and 'potentially real'):
First, I think you need to become acquainted with the modern version of Gleason's Theorem:
https://arxiv.org/abs/quant-ph/9909073
Also, it must be remembered that we know ordinary, non-relativistic QM (abbreviated here to QM) is wrong, and that our current best theory is relativistic quantum field theory (abbreviated to QFT). Surprisingly, the non-relativistic limit of QFT is not QM. This is an undergrad-level discussion, and the explanation is advanced, so those reading this are not expected to understand why, but here is the paper explaining it anyway:
https://arxiv.org/abs/1712.06605
So interpretations of QM, while interesting, are not relevant if you want to understand what QM means - basically, it is simply an approximation to QFT. We need an interpretation of QFT. The best book I know on that is unfortunately a bit pricey, but it does have the advantage of actually addressing the correct issue:
https://www.amazon.com.au/Fields-Their-Quanta-Quantum-Foundations-ebook/dp/B0DLNLLG7Y
At first, QM is mysterious, even though it is, strictly speaking, wrong (which most textbooks do not point out), and this, understandably, leaves students (thinking ones, that is, most accept it) puzzled.
As an attempt to make that puzzle more reasonable, I like to consider the following, which I call a mathematical modelling view. Think of an observation as two things interacting (at present, we think they are quantum fields) and the result of that interaction, which gives a number (assumed real), is conceptually displayed as a digital readout for simplicity. Arrange the possible numbers as vectors. The first possible number is the first entry in a vector; the second is the second entry, and so on. Arrange the vectors in a diagonal matrix, and you have a Hermitian operator (in a specific basis, but of course, we know from linear algebra that bases are really irrelevant - it is actually a linear operator in some vector space). These, we think of as observables. Now apply Gleason and, lo and behold, you have the generalised form of the Born rule. In fact, one can reasonably develop QM from these two rules alone (see Ballentine - QM: A Modern Development). Chapter 19 applies QM to the EM field (hence explaining photons), which is a good stepping stone to QFT (it evades the limiting-case issue because the photon is its own antiparticle, which, of course, is not true generally). It also contains a detailed discussion in Chapter 8 of the indeterminacy relations, which even Heisenberg got wrong (and Bohr corrected).
Bottom line here is, at the undergraduate level, I would not worry too much about these issues - they really need more advanced treatments at the graduate level. You can read Art Hobson's book as an undergraduate with a first course in QM under your belt (or simply read Lenny Susskind's book on QM - a popular book that appeared on the best seller list that includes the math - a marvel), but for now, I would leave it at that. Why is QM statistical? The interpretation-independent answer is Gleason's Theorem, and that observables are modelled as Hermitian operators. Beyond that, I would leave it until you have studied Many Worlds, Decoherent Histories and other interpretations.
Thanks
Bill