Zaphodx57x said:
I was reading today about superfluids and the like. They were talking about how at a certain low temperature bosons will all go into their ground state. I'm trying to get a physical feel for what this means. If a mole of helium 4 atoms(boson) are cooled so that condensation occurs. What exactly happens? I can imagine, if there is no degeneracy pressure, then the mole of atoms can become extremely dense. But how dense can they get? Is the nucleus nucleus coulomb repulsion the only thing stopping them from becoming unified?
I'm not exactly sure, don't take this as gospel, but I'd imagine that when they came closely packed, occupying similar space, that the constituent particles of He4 (neutrons and protons) are actually Fermions, so they would have to satisfy Pauli Exclusion Principle...
For example, a Cooper Pair in a Superconductor is a Boson, with constituents of 2 electrons, but the two spins are in opposite directions. So if another electron came within range, it would destroy the Cooper Pair (Boson) by means of breaking the binding energy. So I think a similar process may be availible for liquid Helium.
Superconductors and Superfluids are similar concepts involving Bose-Einstein condensation. Superconductors involve zero resistance, Superfluids involve zero viscosity.
May I make it clear I have only studied superconductors before, not superfluids, so my superfluid assumptions are based on analogy from superconductors.
I have often asked these questions myself before, but couldn't be bothered to seek an answer, and these were the conclusions I reached.
Hopefully a better informed person will be able to shed some real light.
Also, I believe that neutrons in neutron stars are superfluid - Bose-Einstein condensation again - I think they form neutron pairs, similar to Cooper Pairs. But they are obviously really dense.