Why is it so hard to create atoms from other atoms?
So helium is a limited resource. Okay gotcha. So why not take two hydrogen atoms. Take their protons and neutrons. And just fucking start squeezing them together until you get helium?
And I don't mean in the same way you get H2. Those are still separate from each other.
Because you need the concentrated gravity of the sun to do this. Otherwise the electromagnetic force between the positively charged protons will keep them from sticking together.
Good news: This actually "creates" energy because helium is slightly lighter than two hydrogens. Look at the sun, that's how it sends us all the nice sunshine.
Bad news: You need more energy to actually push them together.
But we're trying to get there. That's what all the fusion reactors are supposed to do. We'll probably get it to work in about 50 years.
Is the LHC trying to do this? I know it smashes atoms together at high speeds, is this us trying to "squeeze" the atoms together like the sun does?
Or is the LHC is completely unrelated to OP's question?
Not really, but another massive international project, ITER, is trying to do this. Its timeline is measured in decades if not the better part of a century.
Fun fact: pretty much all the helium we have access to comes from alpha decay of heavier atoms, such as natural uranium. An alpha radiation particle is just a "naked" and fast moving helium nucleus. (Missing the electrons.) When this happens deep in the earth, it quickly runs into something, stops moving, and picks up some electrons to make it helium, which can accumulate in certain rocks.
We get the energy from fission. To put two hydrogens together to turn it into one helium is the very definition of fusion.
Separate but related: among the many mind-blowing astronomical discoveries of the past decade or two, kilonovas are in the short list for most spectacular.
Imagine two tiny neutron stars plowing into each other, all those densely packed neutrons suddenly and with great force being clumped together into super heavy elements, creating a spiral spray of silver, gold, platinum, uranium nuclei, but just the neutrons.
With time, some of these neutrons decay into protons, or absorb whatever hydrogen atoms they encounter along their path - a proton and an electron - along with whatever random free electrons may also be around, floating freely in space.
Eventually you'll get the full atoms. Some of that bounty got caught in the gravity well of the gas and dust nebula that collapsed into our solar system.
And that's how the universe created the silver, gold, titanium, uranium, etc, that is in our planet today.
In addition to everything else mentioned, in your scenario, you would also need to pull 2 neutrons from somewhere. A helium nucleus has 2 protons and 2 neutrons, but each H nucleus (generally) is just 1 proton. The 2 neutrons are critical in holding nuclei together.
That's why nuclear fusion uses deuterium and tricium, isotopes of hydrogen with respectively one and two neutrons. These are much rarer than regular hydrogen, but can be found in some water molecules known as "heavy water". They can be separated from the other molecules with a centrifuge since they're heavier.
Two deuterium atoms would produce Helium 4, but that's not the most efficient fusion, and thus not the one that they plan to use in fusion reactors. Instead, they fuse a deuterium and a tricium, resulting in an Helium 5 atom. Unlike regular helium(4), helium 5 is radioactive, but it's got a relatively short half-life and will soon expell it's extra neutron, creating the helium we know and love.
Because it takes a real lot of energy. Like a real lot of it. We’re currently trying to do that in a controlled form in ITER which is still getting built
Others have already mentioned that this is fusion. But the fact that any nucleus with more than two protons exists at all is interesting. E=mc^2 is a well known equation, but not many people understand it's practical application. If you shove 2 protons and 2 neutrons together to form Helium, the resulting nucleus weighs less than it's constituent pieces. Where'd the lost mass go? It turned into binding energy. The energy necessary to force two positively charged protons to hang out together without flying apart. And this is part of the energy input necessary to fusion things. Conversely, when we break Uranium apart we get a lot of energy. For the same reasons. Which is how current fission reactors work.
If you really find this stuff interesting do some googling related to fission, fusion, mass defect, and binding energy.
Not the really the "same reason". Unless that reason is the in both cases, the binding energy per nucleon is increasing. So, for interested people, also look at the binding energy per nucleon curve. Fe is boring...but stable.
The forces within an atom are very strong and complex. We can create fission chain reactions in some very radioactive elements, and we can fuse some small elements, but the amounts of such reactions we can produce is pretty restricted. Beside, a particule that exits an atom will leave at a high speed, and it's impossible to reliably know where it goes because of the rules of quantum physics, so it's not like you can just take a proton and leave it in a box to reuse later. What we can use is the energy produced by the fission, and that's what nuclear plants do.
Its just hard for us. Not hard at all for a sun, which makes up a far greater proportion of observable matter than what exists at 'our' temperature/ gravity. Even then, gasses make up an even larger proportion of observable matter.
So a counter way of asking the same question might be "Why is it so hard to not undergo nuclear fusion?" or "Why is it so hard to not be gas?". Even further, the observable stuff is practically nothing compared to the relatively unobservable stuff. So maybe the question could be "Why is it so hard to not be dark matter/ energy?"
Just something to consider in the framing of your question Fat Tony, is that you are asking it from your perspective, and there are assumptions baked into the view you have of the universe because of your position. If you were a neutrino, or a star, or some gas in the milky way, you might consider things very differently