Inner structure of dark matter halos at high $z$ in cosmological models with non-power-law primordial spectra

Ähnliche Einträge

• Excess of high-$z$ galaxies as a test for bumpy power spectrum of density perturbations
  von: Tkachev, M. V., et al.
  Veröffentlicht: (2023)
• High-$z$ SMBHs in Cosmological Models with Enhanced Power Spectra
  von: Tkachev, M. V., et al.
  Veröffentlicht: (2025)
• Absorption in the 21 cm Hydrogen Line at $z>10$ as a Sensitive Tool for the Construction of a Cosmological Model on Small Scales
  von: Eroshenko, Yu. N., et al.
  Veröffentlicht: (2025)
• Properties of Central Regions of the Dark Matter Halos in the Model with a Bump in the Power Spectrum of Density Perturbations
  von: Eroshenko, Yu. N., et al.
  Veröffentlicht: (2024)
• On the increase in the concentration of primordial black holes in the halos of dwarf galaxies
  von: Pilipenko, S. V., et al.
  Veröffentlicht: (2025)