Abstract
The Abundance Matching Box for the Epoch of Reionization (AMBER) is a
semi-numerical code for modeling the cosmic dawn. The new algorithm is not
based on the excursion set formalism, but takes the novel approach of
calculating the reionization-redshift field $z_re(x)$
assuming that hydrogen gas encountering higher radiation intensity are
photoionized earlier. Redshift values are assigned while matching the abundance
of ionized mass according to a given mass-weighted ionization fraction
$x_i(z)$. The code has the unique advantage of allowing users to
directly specify the reionization history through the redshift midpoint
$z_mid$, duration $\Delta_z$, and asymmetry $A_z$
input parameters. The reionization process is further controlled through the
minimum halo mass $M_min$ for galaxy formation and the radiation mean
free path $l_mfp$ for radiative transfer. We implement improved
methods for constructing density, velocity, halo, and radiation fields, which
are essential components for modeling reionization observables. We compare
AMBER with two other semi-numerical methods and find that our code more
accurately reproduces the results from radiation-hydrodynamic simulations. The
parallelized code is over four orders of magnitude faster than radiative
transfer simulations and will efficiently enable large-volume models, full-sky
mock observations, and parameter-space studies. AMBER will be made publicly
available to facilitate and transform studies of the EoR.
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