Physicists captured individual atoms and observed them merge into a molecule
otago.ac.nz
otago.ac.nz
> Each atom has some amount of energy associated with it. If you just bring two atoms together, the total energy is simply the sum of their individual energies. This state is typically referred to as an excited state. However, the stable bonded form of the two atoms actually has a lower energy. So to go from two separate atoms to two bonded atoms, the atoms have to first collide and form the excited state and then lose some amount of energy to go to the stable state. If they don’t lose that energy, then they can and will break apart again. One way to lose that energy is via collision with the third atom.
> In normal systems where you have tons of atoms flying around, collisions happen very frequently, so you can typically assume that the stabilization will happen immediately following the reaction. This is why the idea that stabilization is an important step in a chemical reaction is typically not covered in intro chemistry. However, it’s not uncommon to have conditions where that assumption does not hold. This then gets into the concept of pressure dependent reaction kinetics, which studies the effect of having slow stabilization.
[0] https://www.reddit.com/r/science/comments/f7mqwl/physicists_...
https://en.m.wikipedia.org/wiki/Activation_energy
They don't necessarily bring atoms or molecules together, per se, but some do.
Just learned on Wikipedia (en/Platinum) that the 2007 Nobel price in Chemistry was awarded for explaining how that works. doi:10.1002/anie.200800480
In fact, at room temperature they don't work at all, which is exactly the problem with catalysts, they don't work when you start your car.
They need to heat with the hot combustion gases to start working, and that takes a while.
This is one of the reasons that laboratory's measurements of particles and gases like nitrogen oxides do not apply to real emissions in cities, because most people in cities will use the cars, for example, diesels in Europe, for very short periods of time, then let the car cool down and use it again to go back less than 10 kilometers away.
Here's a good example of how enzymes catalyze reactions: https://pdb101.rcsb.org/learn/videos/how-enzymes-work
The last 1/3 of this old video from Shell describes how catalytic cracking, a crucial part of oil refining, works. It covers practical reactor considerations, including getting the products out so more are formed and 'poisoning' where a catalyst's efficiency is reduced by contamination and how that's dealt with in a continuous process. https://www.youtube.com/watch?v=hC1PKRmiEvs
[1] According to my grade-school chemistry. :/
What you are probably thinking of, is the fact that if you put NaOH, or HCl in water, you get Na+, OH-, etc., and these are more stable than their neutral counterparts. But this is because they are stabilised by (polar) water molecules. Outside of water (or some other stabilising solvent), Na+, OH-, H+ and Cl- are all very reactive species.
> It appears you need the energy from 3 in order for the 2 to make a bond.
> It's the other way around. Two atoms alone will release a bunch of energy when they form a molecule; exactly enough energy to rip the molecule back apart. That energy has to go somewhere, and where it goes is the third atom.
In other atomic physics experiments it's a problem - three-body collisions are able to dump energy into one of the three atoms and that atom has enough energy to escape the trap. These are "three-body losses".
Whereas with two-body collisions, neither atom can be going any faster afterwards than the fastest one was before the collision. So they remain trapped.
Since the three-body collision rate is proportional to the cube of the density of atoms, and the two-body collision rate only to the square of density (for obvious reasons), this phenomenon limits the density of atomic clouds we can do experiments with. If we increase the density to the point where three-body collisions are significant, we rapidly lose atoms.
https://physics.aps.org/synopsis-for/10.1103/PhysRevLett.124...