Simulating Inhomogeneous Reionization

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dc.creatorNorman, Michael L.
dc.creatorPaschos, Paschalis
dc.creatorAbel, Tom
dc.date1998-07-28
dc.date.accessioned2026-07-07T02:27:28Z
dc.date.available2026-07-07T02:27:28Z
dc.descriptionWe describe an approach for incorporating radiative transfer into 3D hydrodynamic cosmological simulations. The method, while approximate, allows for a self-consistent treatment of self-shielding and shadowing, diffuse and point sources of radiation, and frequency dependent transfer. Applications include photodissociation, photoheating, and photoionization of the IGM.
dc.description8 pages, 0 figures. To appear in Proceedings of the Workshop on H_2 in the Early Universe, eds. F. Palla, E. Corbelli, and D. Galli, Memorie Della Societa Astronomica Italiana, in press (1998)
dc.identifierhttps://arxiv.org/abs/astro-ph/9807282
dc.identifierhttp://arxiv.org/abs/astro-ph/9807282
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12706
dc.subjectAstrophysics
dc.titleSimulating Inhomogeneous Reionization
dc.typetext

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