• If all that matter had been what cosmologists call “dust,” matter with no pressure or internal friction, and if it had been entirely homogeneous, it would continue to fly apart at the same rate everywhere. But matter was not completely homogeneous. There were small initial fluctuations. And where matter was a little denser, it had a little more self-gravity. Which means that over time, it was flying apart a little more slowly at such locations.
  • In some places, the overdensity of matter was large enough to stop the flying apart completely. Pressure and internal friction also helped, making it possible for matter’s kinetic energy to dissipate as heat, further slowing matter down. If the flying apart was stopped entirely, gravity took over and caused matter to clump. These clumps eventually became clusters of galaxies, and within those clusters, individual galaxies, star clusters in those galaxies, and solar systems in those star clusters. So, the point is that matter inside a galaxy has stopped flying apart. Its self-gravity prevailed over the initial “kick” that this matter received from the Big Bang.
  • And just to be clear, when I talk about this initial “kick,” I don’t mean matter flying into pre-existing space. All of space has been filled with matter since the beginning. It’s just that, on average, matter is a lot less dense today than it was just after the Big Bang. If the universe were finite, it must be more significant today than it was back then. But to our knowledge, the universe has always been spatially infinite. And any mathematician can tell you that there are (very counterintuitively) precisely as many points on the real line between 0 and 1 as between o and 10 or 0 and 1,000,000. Dark energy contributes essentially repulsive gravity. That is, under its own gravity, dark energy expands instead of contracting. So, in any region of space dominated by dark energy, dark energy speeds up the expansion.
  • Dark energy must first dominate. And the energy density of dark energy is very low. So it is only in space between galaxy clusters, and only in the past few billion years, that dark energy came to dominate over other forms of matter. In regions where the expansion stopped billions of years ago, such as inside a cluster of galaxies or in a galaxy, the density of ordinary (and dark) matter never dropped below the threshold where dark energy becomes dominant. So, the repulsive gravitational response of dark energy never got a chance to prevail over the attractive self-gravity of other forms of matter.