I am not so sure about the win here. Redshifts are used but the range is not stated like z=1 to 10 or whatever. All galaxy models using redshifts come with the comoving radial distances too, something not shown in the simulations. Do the galaxies evolve along their comoving radial distances too, just like the simulations for comparing look back time distances? There is no way to observe this evolution if it takes place. The space.com article did mention inflation and its importance.
"As the infant universe underwent a period of rapid expansion called inflation, small perturbations spread through the plasma as a sound wave, producing under- and over-densities of both matter and radiation, but not affecting dark matter."
Comments like this seem to have problems now because inflation creates primordial black holes.
Primordial black holes may have 'frozen' the early universe,
https://phys.org/news/2023-04-primordial-black-holes-frozen-early.html
Ref - Primordial Black Holes Place the Universe in Stasis,
https://arxiv.org/abs/2212.01369, 29-March-2023.
My notes. From the 25-page PDF report cited by phys.org article, "I. INTRODUCTION In a broad class of inflationary scenarios, a population of black holes (BHs) is generated shortly after inflation as a consequence of the gravitational collapse of primordial density fluctuations. Such primordial black holes (PBHs) have received a significant amount of recent attention, in part because they can potentially provide a solution to the dark-matter problem. Indeed, while black holes evaporate over time as a consequence of Hawking radiation [1, 2], PBHs with masses M ~> 10^15 g would nevertheless have lifetimes longer than the age of the universe. Indeed, a population of PBHs with masses within the range 10^17 g <~ M <~ 10^23 g can potentially account for the entirety of the present-day dark-matter abundance, even when the spectrum of PBHs is approximately monochromatic (for reviews, see, e.g., Refs. [3-6]). PBHs with lower masses can also have implications for cosmology. Indeed, PBHs with masses in the range 10^9 g <~ M <~ 10^14 g evaporate at a significant rate during or after Big-Bang nucleosynthesis (BBN), generating energetic particles which can modify the primordial abundances of light nuclei. As a result, the abundance of PBHs with masses in this range is tightly constrained [4, 7, 8]." [My note. Inflation with PBHs apparently creates more constraints for the BB model, production of H, He, and perhaps a little Li too as well as DM creation. Is this another fine-tuning problem in cosmology using exotic physics, not seen operating in the universe today to explain how we evolved naturally?
Question. Does this new simulation for how galaxies evolved over billions of years state clearly how dark matter evolved too? PBH evolution may be an additional headache here
