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Remy Moll
2025-09-14 02:38:29 +02:00
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abstract.typ
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#import "helpers.typ": *
= Abstract
We present an updated version of the #beorn framework, a semi-numerical simulation suite that generates maps of the cosmic dawn and the epoch of reionization. The refinements include a self-consistent treatment of the evolution of individual galaxies, a parametrization of stochasticity of the mass accretion rate, and a general optimization that allows for speedier simulation runs.
We present an improved version of the #beorn framework, a semi-numerical simulation suite that generates maps of the cosmic dawn and the epoch of reionization. The refinements include a self-consistent treatment of the evolution of individual galaxies, a parametrization of stochasticity of the mass accretion rate, and a general optimization that allows for speedier simulation runs.
We validate the improved version of the suite against ??. We employ the Thesan-Dark simulation to inder halo mass history and demonstrate the effect of this more detailed treatment.