Artist: Fast radiative transfer for large-scale simulations of the epoch of reionization
| dc.contributor.author | Molaro, Margherita | |
| dc.date.accessioned | 2023-01-11T09:58:48Z | |
| dc.date.available | 2023-01-11T09:58:48Z | |
| dc.date.issued | 2019 | |
| dc.description.abstract | We introduce the ‘Asymmetric Radiative Transfer In Shells Technique’ (ARTIST), a new method for photon propagation on large scales that explicitly conserves photons, propagates photons at the speed of light, approximately accounts for photon directionality, and closely reproduces results of more detailed radiative transfer (RT) methods. Crucially, it is computationally fast enough to evolve the large cosmological volumes required to predict the 21cm power spectrum on scales that will be probed by future experiments targeting the epoch of reionization (EoR). Most seminumerical models aimed at predicting the EoR 21cm signal on these scales use an excursion set formalism (ESF) to model the gas ionization, which achieves computational viability by making a number of approximations | en_US |
| dc.identifier.citation | Molaro, M. et al. (2019). Artist: Fast radiative transfer for large-scale simulations of the epoch of reionization, Monthly Notices of the Royal Astronomical Society, 489(4), 5594–5611. https://doi.org/10.1093/mnras/stz2171 | en_US |
| dc.identifier.issn | 2331-8422 | |
| dc.identifier.uri | http://hdl.handle.net/10566/8277 | |
| dc.language.iso | en_US | en_US |
| dc.publisher | Oxford University Press | en_US |
| dc.subject | radiative transfer | en_US |
| dc.subject | dark ages | en_US |
| dc.subject | reionization | en_US |
| dc.subject | first stars | en_US |
| dc.title | Artist: Fast radiative transfer for large-scale simulations of the epoch of reionization | en_US |
| dc.type | Article | en_US |