More questions about the totally off-topic of Stellar Evolution. What do you think?

I've discovered that the 4th power of mass formula for Stella Luminosity is slightly wrong. This formula would only be true if all atoms were the same exact thing as one another. IN a real Star, the atoms in the core grow denser as they fuse into heavier elements, which means the real stellar Luminosity curve is much more complex than just using 4th power of mass. For example, Carbon is much more dense than Helium, so for stars which burn 51% or more Carbon, those stars burn many, many times brighter than a star which burns only a few percent Carbon. Meanwhile, stars which burn 51% Helium burn much brighter than stars which burn 1% or less Helium. Understand? The denser the core, the faster the rate of burning, even if the mass remains unchanged.

One consequence of this is I think I can show most stars *SHOULD* explode by the time they accumulate 1.44 solar masses of Carbon, Nitrogen, and Oxygen in their cores, which implies "First Generation" stars which are perhaps 10 Masses or greater actually "waste" most of their stellar Hydrogen, while stars more like the Sun burn up almost all of their hydrogen in their lifetimes.

How to derive the 4th power of mass for an ideal fluid-like star? Well, I know how to do that, but it doesn't work in the real world. So how to derive what really works?

Very simple: Stars should be re-classified by the heaviest element they can fuse as at least 51% of their fuel supply. Then star types and supernova types would make more sense.

More questions about the totally off-topic of Stellar Evolution. What do you think?
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