Show simple item record

dc.contributor.authorMolaro, Margherita
dc.date.accessioned2023-01-11T09:58:48Z
dc.date.available2023-01-11T09:58:48Z
dc.date.issued2019
dc.identifier.citationMolaro, 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/stz2171en_US
dc.identifier.issn2331-8422
dc.identifier.urihttp://hdl.handle.net/10566/8277
dc.description.abstractWe 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 approximationsen_US
dc.language.isoen_USen_US
dc.publisherOxford University Pressen_US
dc.subjectradiative transferen_US
dc.subjectdark agesen_US
dc.subjectreionizationen_US
dc.subjectfirst starsen_US
dc.titleArtist: Fast radiative transfer for large-scale simulations of the epoch of reionizationen_US
dc.typeArticleen_US


Files in this item

Thumbnail

This item appears in the following Collection(s)

Show simple item record