Testing galaxy formation simulations with damped Lyman-alpha abundance and metallicity evolution

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    Final published version, 1.62 MB, PDF document

  • Sultan Hassan
  • Kristian Finlator
  • Romeel Dave
  • Christopher W. Churchill
  • J. Xavier Prochaska

We examine the properties of damped Lyman-alpha absorbers (DLAs) emerging from a single set of cosmological initial conditions in two state-of-the-art cosmological hydrodynamic simulations: SIMBA and TECHNICOLOR DAWN. The former includes star formation and black hole feedback treatments that yield a good match with low-redshift galaxy properties, while the latter uses multifrequency radiative transfer to model an inhomogeneous ultraviolet background (UVB) self-consistently and is calibrated to match the Thomson scattering optical depth, UVB amplitude, and Ly alpha forest mean transmission at z > 5. Both simulations are in reasonable agreement with the measured stellar mass and star formation rate functions at z >= 3, and both reproduce the observed neutral hydrogen cosmological mass density, Omega(HI)(z). However, the DLA abundance and metallicity distribution are sensitive to the galactic outflows' feedback and the UVB amplitude. Adopting a strong UVB and/or slow outflows underproduces the observed DLA abundance, but yields broad agreement with the observed DLA metallicity distribution. By contrast, faster outflows eject metals to larger distances, yielding more metal-rich DLAs whose observational selection may be more sensitive to dust bias. The DLA metallicity distribution in models adopting an H-2-regulated star formation recipe includes a tail extending to [M/H]

Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Volume492
Issue number2
Pages (from-to)2835-2846
Number of pages12
ISSN0035-8711
DOIs
Publication statusPublished - 1 Feb 2020

    Research areas

  • galaxies: evolution, galaxies: formation, intergalactic medium, quasars: absorption lines, cosmology: theory, STAR-FORMATION RATE, LESS-THAN 5, H I, COSMOLOGICAL SIMULATIONS, NEUTRAL HYDROGEN, HIGH-REDSHIFT, ABSORPTION SYSTEMS, BLACK-HOLE, GAS, ABSORBERS

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