PeterDonis said:
This is a paper on heavy ion fusion, which is not the kind of fusion that takes place in the Sun.
Also, although the paper does give a schematic formula for the potential barrier, which could be used to analyze fusion in the Sun, it does not give actual formulas for the key terms, the nuclear and coulomb potential. In other words, it does not provide any way of answering the question, why is it the case that quantum tunneling is necessary for fusion in the Sun?
If you'd like to spin this off into another thread, it might be better. I'll do my best to at the end give the steps for OP to estimate it if they're interested (without getting into junk such as the gamow factor), otherwise, not sure if it's the relevant to them.
The details come down to the core density and temperature. In order for the protons to overcome the coulomb barrier, and be in the strong force range, the sun's core needs to be hotter to sustain fusion. Classically, there is none that do that. The only way we can see it occurring is with quantum tunneling, hence the sun needs it. I will post, another I level link, which you can complain isn't "peer-reviewed" (which shouldn't be relevant here, this is standard physics known since the 30s...).
Alas, here are some slides that make the same claim:
https://sites.astro.caltech.edu/~george/ay20/Ay20-Lec7x.pdf (page 45/46).
Without going into more details*, the fact is that the sun's core needs to be ~##10^{11} K##. Since your background is in nuclear, open up good ole Krane, start of chapter 14 he gives a similar estimate for thermonuclear fusion for a container of neon gas.
In order to sustain nuclear fusion classically (because that's how much kinetic energy the nuclei need), we need something in that region. It's not that hot, it's ~##10^7 K##, what do we conclude? There is a macroscopic object in our solar system that NEEDS quantum tunneling to sustain it's existence, and even then, it rarely occurs. That's why I thought it'd be a fun exercise for them to see that even in the sun core, only a small amount of THAT tunnels at a given time. This would open their eyes to the concept that it's absurdly rare! If we consider objects, such as chairs, what hope do they have to ever tunnel as a whole?
*If OP would like to learn how to estimate this for the sun, treat the core like an idealized gas, assume that the average kinetic energy is proportional to the temperature in idealized gasses, then use the "equipartition energy equation" (##KE = \frac{3}{2}kT## where KE is kinetic energy of the needed fusion, k is the boltzmann constant, and T is the temperature needed, which you would solve for algebraically) find the required kinetic energy needed for nuclear fusion to occur for protons, and solve for T. Make sure to convert units if you're not in the habit of doing so yet!