Tracing the sources of reionization in cosmological radiation hydrodynamics simulations
Résumé
We use the photon flux and absorption tracer algorithm presented in Katz et al. to characterize the contribution of haloes of different mass and stars of different age and metallicity to the reionization of the Universe. We employ a suite of cosmological multifrequency radiation hydrodynamics AMR simulations that are carefully calibrated to reproduce a realistic reionization history and galaxy properties at z ≥ 6. In our simulations, haloes with mass 109M⊙h−1
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https://hal.science/hal-03046360
Soumis le : lundi 26 juin 2023-11:09:48
Dernière modification le : mardi 12 novembre 2024-15:20:05
Archivage à long terme le : mercredi 27 septembre 2023-19:14:58
Dates et versions
Identifiants
- HAL Id : hal-03046360 , version 1
- ARXIV : 1806.07474
- DOI : 10.1093/mnras/sty3154
- INSPIRE : 1678685
Citer
Harley Katz, Taysun Kimm, Martin Haehnelt, Debora Sijacki, Joakim A Rosdahl, et al.. Tracing the sources of reionization in cosmological radiation hydrodynamics simulations. Monthly Notices of the Royal Astronomical Society, 2019, 483 (1), pp.1029-1041. ⟨10.1093/mnras/sty3154⟩. ⟨hal-03046360⟩
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