The heliopause is the theoretical boundary where
the Sun's solar wind is stopped by the interstellar
medium; where the solar wind's strength is no longer
great enough to push back the stellar winds of the
surrounding stars.2) When your experiment yields results that match your hypothesis, you consider that evidence.
3) When you have sufficient evidence, you upgrade your hypothesis to a theorem.
According to the Wikipedia article, we've got at least two probes that are producing results in line with our hypotheses. The bar for wikipedia is "sourced", not proven theorem with scientific rigor. In this case, we're in some nebulous area between 2 and 3. I think that meets the bar for an encyclopedia, which is intended to serve as a summary for these types of things.
Hit the sources and the transitive closure of references for more details.
A theorem is a mathematical result: something proved logically from (possibly physical) assumptions.
To my mind, in this context, the difference between maths and physics is that maths is exhaustive while in physics we don't usually have exhaustive evidence so we have to work with what we've got.
I'm less certain than I was before I read your post, though - so I stand to be corrected :-)
The particles slow down because they press against the electric field of interstellar particles. So the energy will smoothly go down as Voyager gets farther.
But the number of particles won't change. The number will reach zero once the particles slow down so much they turn around and go the other way but until that point the number of particles won't change.
It would be interesting to see a graph of the energy levels, but I don't know if Voyager carries such a device.