I had a hard time deciding which board to place this in, but this should do. I guess I'll start off with an analysis of what the proposed nuclear fuel cycle means to an expert. The choice of mining Uranium, and having the isotope abundance identical to Earth, is a bit of a naive mistake. It shows that someone did enough research to know what those values are, but not enough to know WHY. Heavier elements are produced during Supernova Nucleosynthesis and in proportions highly dependent on star size. Then, between that event and the formation of the next star system, those abundances change as heavier elements decay. Earth's 0.7% abundance of U-235 among total Uranium is not only unique to our solar system, but also the age of our solar system and the length of time between the death of the previous star and the formation of our solar system. The chances of finding another planet that has EXACTLY the same abundance of Uranium is slim to null. Much younger, and you might get relatively high U-235, enough that the ore is reactor ready with only chemical treatment. Much older, and there wouldn't be enough U-235 left at all. If the planet formed from the previous star being too small, and there wouldn't be any elements heavy enough to support fission.Alexander Pope wrote: A little learning is a dangerous thing ;
Drink deep, or taste not the Pierian spring :
There shallow draughts intoxicate the brain,
And drinking largely sobers us again.
Fired at first sight with what the Muse imparts,
In fearless youth we tempt the heights of Arts ;
While from the bounded level of our mind
Short views we take, nor see the lengths behind,
But, more advanced, behold with strange surprise
New distant scenes of endless science rise !
So pleased at first the towering Alps we try,
Mount o’er the vales, and seem to tread the sky ;
The eternal snows appear already past,
And the first clouds and mountains seem the last ;
But those attained, we tremble to survey
The growing labours of the lengthened way ;
The increasing prospect tires our wandering eyes,
Hill peep o’er hills, and Alps on Alps arise !
Suggestion: rename the ore to "Actinides". This is a vague enough term to be technically correct, no matter the age of the star system. Also, rename U-235 to "fissile material" and U-238 to "fertile material".
Next on the list is the enrichment process. I'd like to express my gratitude for making it as simple as possible, within reason. My only complaint is how the " "Kovarex enrichment process" is in the wrong machine. It should be in a small "breeder reactor". Also, if you used the naming convention from above, you wouldn't have to worry about magically turning U-238 into U-235, since it would technically be turning U-238 into Pu-239 (or Th-232 to U-233), without getting hung up the details. If you really want to, you could just have "nuclear material" the thing created in the small breeder reactor, put it into the centrifuges, and it would produce much better fissile/fertile material ratio than the ore.
Continuing with the end-enrichment result. The 5% U-235 screams a certain tech at me -- thermal light water reactor. Specifically, commercial ones. The same with abundance, this informs me that the tech was merely copied from industry standard without an understanding as to all the complex technological and political history behind it. I'll be blunt: there's no way in hell one would rationally choose to use that tech in the situation our Factorio Guy is in. I'll go more into detail in that if you really want, but I'd rather not.
Suggestion: (low priority) put only pure "fissile material" in the power reactors as a fuel source. This is pretty much what military reactors use, and the fuel cycle goes from 18 months to 10 years. This also means that you could just include the fissile and fertile material in the recipe of the reactor and not worry about ever fueling it. After a certain amount of energy produced, you could just have the reactor explode. This would be a ridiculously large number, and you should be able to check at any time how much life the reactor has (in Joules) but you wouldn't have to worry about cramming in the logistics of fuel. Just place and worry about piping, adjacent reactors, and such. Oh, and the inevitable explosion if you don't remember to dismantle it before its end-of-life.
I think it is hilarious that several proposed things were abandoned. The funniest is the reactor meltdown. I've written code for reactor simulations as a research assistant intern before, so I fully understand how much of a pain writing that code is. I feel like I don't need to give the suggestion I was planning before the FFF was released about how they should simplify the simulation instead of trying to figure out when it will explode from overheating. I do have one more suggestion: for the heat pipes. Instead of 1 big pipe, have 2 smaller pipes. In practice, heat delivery would be in the top pipe and cold return would be in the bottom pipe, to facilitate natural circulation in the event of power failure. It's a small graphical detail, but it would improve the looks and imply a circulation of some type of fluid. Molten salt or lead eutectic or something similar.
Just how much energy is in fissile material? I don't feel like doing the calculation again, so I'll just paste from the U-235 wikipedia entry:
wikipedia wrote:The fission of one atom of U-235 generates 202.5 MeV = 3.24 × 10−11 J, which translates to 19.54 TJ/mol, or 83.14 TJ/kg.
This is equal to 23.1 million kilowatt hours per kilogram of fissile material.
Edit 1: I forgot an important suggestion regarding natural abundance of fissile and fertile material! It should be random, based on map seed, and global for that map. I'd like to see it anywhere between 0.2% and 5%, which is a pretty wide range. It would also lead to people seeking out and sharing good seeds again. If the decision is made to keep the 5% enrichment max for reactors, then if you're really lucky, you can just go straight from ore to fuel rods without enrichment. I still recommend using higher enriched fuel for the reactors, any number higher than 5% will do. Thorium is about 2.5 to 3.5 times as abundant as uranium, as it is the U-235 that decays very quickly (half-life of 703 million years) compared to U-238 (half-life of 4.47 billion years) and Th-232 (half-life of 14.05 billion years).
Best regards, from someone who has entirely too much education and experience in this whole nuclear mess.