Tell it depend on what part you mean exactly, some were observed some are theoratically, meaning it fit with our model of physic and this is what should happen given what we know, but right now we have no way of confirming it.
First we know that the neutron star is made of Iron. Why we know that? Well a supernovea occur because iron accumulate in the core, so if the core is mostly made of something else it couldn’t go supernovea yet. Then we know the mass and dimensions of a neutron star, by looking at it with instrument and how it interact with other stuff. A bit like we measure the mass and dimensions of planets or stars. So now that we know that, we can model the gradiant of pressure along the depth of the star. That pretty much like we can calculate the pressure of water as we go deeper, we can calcualte what will be the pressure at each depth in the star.
Next step is two fold, theorically we can calculate with our current model what should happen to matter at those different pressure and secondly we can test some of it with particule accelerator. By accelerating small particle to extreme speed, we can see what happen to them if they collide, create huge pressure and can see if that fit our model or if there is something we don’t understand.
So if you look at the video, we know that the outer layer is iron, because at this point the pressure is low enough to keep iron intact. But as the pressure get higher, we know that at a certain pressure electrons and protons fuse to get neutrons. So we can calculate at which depth the pressure is enought to do that. I’m not sure if we recreated that in a particle accelerator for sure, but it’s possible since both of those are charged particles. What I know for sure is that this nuclear pasta is purely theoric. It’s the point where the nuclear force and coulomb repulsion are equal so we know that this happen, but what exactly it would be is speculation based on what we know of physics.
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