Kiloparsec-scale turbulence driven by reionization may grow intergalactic magnetic fields

Documenti analoghi

• The hydrodynamic response of small-scale structure to reionization drives large IGM temperature fluctuations that persist to z = 4
  di: Cain, Christopher, et al.
  Pubblicazione: (2024)
• FlexRT -- A fast and flexible cosmological radiative transfer code for reionization studies I: Code validation
  di: Cain, Christopher, et al.
  Pubblicazione: (2024)
• Introducing SAGUARO -- Simulating IGM Evolution and Environments At High Resolution: Setup and First Results
  di: Cain, Christopher, et al.
  Pubblicazione: (2026)
• On the rise and fall of galactic ionizing output at the end of reionization
  di: Cain, Christopher, et al.
  Pubblicazione: (2023)
• Quantifying Lyman-$α$ emissions from reionization fronts
  di: Wilson, Bayu, et al.
  Pubblicazione: (2024)