You have some misconceptions. 1) For all that we have been able to measure it, the electron is a point particle. It does not have a radius. The concept of ra

You have some misconceptions. 1) For all that we have been able to measure it, the electron is a point particle. It does not have a radius. The concept of radius does not apply. Every time we try to measure it, we just end up setting a smaller upper bound for the radius than last time. This is true of all of the leptons ("lightweight particles"). The same sorts of probes of electrons suggest that there is no "stuff" in them. That's all you get, this point with some numbers associated with it (charge, mass, angular momentum, lepton number, etc). 2) Black holes -- and I am going to constrain myself to a "no-hair" situation for those of you in the know -- have only three variables that describe them: mass, charge, and angular momentum. Anything else describes its position and how it is moving at the time. They're really quite dull. (Exploration of where the information that fell into the black hole went is ... contentious, abandoned, frustrating, etc). Radius is a function of mass (and angular momentum, you can distort the event horizon if it had enough spin). 3) They don't "explode." The theorized-but-not-yet-observed Hawking radiation is about chucking out the occasional particle and "borrowing" it from the black hole. This is done under conservation of the above mass, charge, and angular momentum. The smaller they get, the more chance they throw something out, so it is really a runaway process that only looks like an explosion at the end. 4) Due to this conservation, if you somehow made a single electron into a black hole, that black hole could only ever spit out one thing in its lifetime: an electron. 5) The proton is quite different. It is not the opposite of an electron. It is known as what is called a baryon ("heavyweight particle") and it has a size. It is also composed of smaller things, unlike the electron, three quarks and some gluons (which serve to hold the whole thing together). 6) Atomic scales are fine. We can understand things about relativity at the atomic scale. For example, we use the surprisingly extended half-lives of certain incoming particles to verify time dilation. Or just look up how relativity affects the orbital radii of very heavy atoms, in particular gold. Subatomic scales are more interesting.