A homogenized ICL definition applied to Horizon-AGN, TNG100, Gizmo-Simba and Hydrangea yields consistent z=0 fractions of 0.1-0.2 with no significant redshift evolution and dominant contributions from satellites of 10^10.5-10^11.5 solar masses.
Monthly Notices of the Royal Astronomical Society , volume =
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Lagrangian tracers show mixing with low-entropy seeds drives most condensation in cluster cores; magnetic fields cause earlier divergence, higher vorticity, lower Mach numbers, and slower cold-cloud motion via tension.
Including dark matter or modified gravity enhances the effective charge-to-baryonic-mass ratio Q/M_bar by a factor of 10-30 at virial radii, producing structurally linked seed fields of ~10^{-23} G in high-redshift proto-galaxies that could probe the dark sector via distinct radial and mass-dependen
citing papers explorer
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A Consistent Comparison of Intracluster Light Assembly in Simulations I. Redshift Evolution and Progenitor Galaxies
A homogenized ICL definition applied to Horizon-AGN, TNG100, Gizmo-Simba and Hydrangea yields consistent z=0 fractions of 0.1-0.2 with no significant redshift evolution and dominant contributions from satellites of 10^10.5-10^11.5 solar masses.
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XMAGNET -- Stir before serving: a Lagrangian perspective on mixing-driven condensation in the intracluster medium
Lagrangian tracers show mixing with low-entropy seeds drives most condensation in cluster cores; magnetic fields cause earlier divergence, higher vorticity, lower Mach numbers, and slower cold-cloud motion via tension.
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Gravitational-Electric Polarization as a Probe of Dark Matter and Modified Gravity
Including dark matter or modified gravity enhances the effective charge-to-baryonic-mass ratio Q/M_bar by a factor of 10-30 at virial radii, producing structurally linked seed fields of ~10^{-23} G in high-redshift proto-galaxies that could probe the dark sector via distinct radial and mass-dependen