Burning Chain

The nuclear fusion burning chains end with the production of iron. We can understand as follows. The nucleus of an atom contains neutron (uncharged) and protons (positive charges). The particles (known as baryons) are bound together by the strong force. However, the electrical force between the like-charged protons wants to disrupt the nucleus. The way the nucleus gets around this is to insert neutral neutrons between the protons (to separate them). We can actually make several isotopes of helium, 2 protons (di-proton), 2 protons + 1 neutron (He3), and the most common form 2 protons + 2 neutrons (He4).



Based on the details of the structure of nuclei, nuclei range from strongly bound to weakly bound (a to c) to unbound. As for atoms, if two nuclei fuse to make a new nucleus, they release an amount of energy (convert mass to energy) determined by the depth of the well. What does mean for nuclear reactions?

Iron is the most tightly bound nucleus and so, beyond iron, nuclear fusion reactions act to steal energy from the system. In the case of a star, this would mean that nuclear fusion would act as an energy loss mechanism rather than an energy production mevchanism:

    In each successive stage of nuclear burning, the reactions involve the ash of the previous step (that is, it involves more massive nuclei with higher charges than for the previous step). Consequently, each step takes place at higher temperature which is why the later stages of burning requires a more massive star. Also note that the amount of fuel for each successive stage is smaller. The combination of the preceding leads to the successively shorter and shorter amounts of time required for each stage.