Microwave Background Anisotropy and Large Scale Structure in Warm Dark Matter Models

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dc.creatorBurns, Stephen D.
dc.date1997-11-25
dc.date.accessioned2026-07-07T02:25:15Z
dc.date.available2026-07-07T02:25:15Z
dc.descriptionLarge scale structure and microwave background anisotropies are studied for warm dark matter models. Two warm dark matter candidates are considered: gravitinos and sterile neutrinos. Linear large scale structure properties such as $σ_{8}$ and the excess power are calculated, as well as microwave background anisotropies. A rather robust feature of warm dark matter models is that the large scale structure properties are similar to those of mixed dark matter, but that the microwave background anisotropy is very similar to that of standard cold dark matter.
dc.description22 pages, 12 figures, 4 tables
dc.identifierhttps://arxiv.org/abs/astro-ph/9711304
dc.identifierhttp://arxiv.org/abs/astro-ph/9711304
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11853
dc.subjectAstrophysics
dc.titleMicrowave Background Anisotropy and Large Scale Structure in Warm Dark Matter Models
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