Subject: 10 Problems with Dark Matter - With Pavel Kroupa
Pavel Kroupa (born 24 September 1963 in
Jindřichův Hradec,
Czechoslovakia) is a Czech-Australian
astrophysicist and professor at the
University of Bonn.
Luckely, some scientists have observed the flaws of "dark matter" and other invented dogmas.
BTW: There is nothing new to me in his critical analysis and perceptions, but he also needs more alternate informations if solving some more problems.
So, from what I can see, this is not a problem for dark matter. Early collisions notwithstanding, dark matter halo is still the explanation for the Milky Way rotation curve.
At the end of the day, though, rotation curves aren't even the best evidence for dark matter. Baryon acoustic oscillations are. If I were able to, I'd upload some slides I made about using BAO as independent constraints on dark energy alongside Type 1a supernovae at high redshifts: different topic, but ultimately relevant when we get to the BAO portions.
We know the density parameter of baryonic matter very well, and it's just not enough to produce the peaks (and acoustic echoes) in the BAO. That'd be a problem because the energy densities are parametrized by the critical density at which the universe appears flat. In other words, if dark matter didn't exist, dark energy would have dominated MUCH earlier and the universe would have flown apart. We'd be measuring a completely different BAO.
The evidence is so strong for dark matter existing that it's really pretty much on the skeptic at this point to explain why we get the BAO curves that we do when we plot the multipole moment. I can't stress enough how precisely Planck has done this.