This might sound silly. But we always talk about nuclear

Raphael Mccullough

Raphael Mccullough

Answered question

2022-05-08

This might sound silly. But we always talk about nuclear fusion in stars and I have always wondered why this process happens at all.
Is it inevitable for fusion to happen at the temperature and pressure present in a star?

Answer & Explanation

Lankenp19hh

Lankenp19hh

Beginner2022-05-09Added 11 answers

Think of 2 hydrogen atoms or, protons more accurately since at those temperature the atoms don't have electrons, it's more of a soup. So, 2 protons, both positively charged so they repel each other, crash into each other pretty rarely, cause it's still a lot of empty space, but they do make contact every so often. The energy required to get 2 protons or any other atomic nuclei to touch is very high. This is called the Coulomb barrier
That's basically all fusion is, it's when 2 atomic nuclei, which naturally repel each other, get pushed close enough to touch and fuse into 1 nuclei.
Once they touch, in the case of protons, then it's a matter of what quantum combination is most likely to follow. Protons actually don't like each other so much more often than not, they'll just say "lets not do this" to each other and they effectively bounce off each other, basically staying hydrogen.
About one time in a million . . . or so, the protons will stay and fuse but for this to happen, one of them has to become a neutron, because 2 protons aren't a stable nucleus. So in this rare occurrence when they do fuse, one proton kicks out a positron, a neutrino and a gamma ray, essentially getting the energy to do this from the fusion and you're left with a proton-neutron bound together (Deuterium) from a proton-proton collision. This happens rarely but because the sun is so large and there's trillions and trillions of proton-proton collisions every second, you get trillions and trillions of Deuterium nuclei formed every second and Deuterium, unlike protons, is very eager to merge with a proton or another Deuterium so, from there, the process continues.
This is also why hydrogen bombs are made with Deuterium, not hydrogen - hydrogen is much much harder to create fusion with.
Because of this, the sun effectively burns very very slowly, but all that's needed is sufficient temperature and pressure to break the coulomb barrier.

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