摘要: The first measurements of the 21 cm brightness temperature power spectrum
from the epoch of reionization will very likely be achieved in the near future
by radio interferometric array experiments such as the Hydrogen Epoch of
Reionization Array (HERA) and the Square Kilometre Array (SKA). Standard MCMC
analyses use an explicit likelihood approximation to infer the reionization
parameters from the 21 cm power spectrum. In this paper, we present a new
Bayesian inference of the reionization parameters where the likelihood is
implicitly defined through forward simulations using density estimation
likelihood-free inference (DELFI). Realistic effects including thermal noise
and foreground avoidance are also applied to the mock observations from the
HERA and SKA. We demonstrate that this method recovers accurate posterior
distributions for the reionization parameters, and outperforms the standard
MCMC analysis in terms of the location and size of credible parameter regions.
With the minutes-level processing time once the network is trained, this
technique is a promising approach for the scientific interpretation of future
21 cm power spectrum observation data. Our code 21cmDELFI-PS is publicly
available at this link.