Is the Lambda CDM Model Consistent with Observations of Large-Scale Structure?

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dc.creatorGawiser, Eric
dc.date2000-05-24
dc.date.accessioned2026-07-07T01:53:44Z
dc.date.available2026-07-07T01:53:44Z
dc.descriptionThe claim that large-scale structure data independently prefers the Lambda Cold Dark Matter model is a myth. However, an updated compilation of large-scale structure observations cannot rule out Lambda CDM at 95% confidence. We explore the possibility of improving the model by adding Hot Dark Matter but the fit becomes worse; this allows us to set limits on the neutrino mass.
dc.descriptionTo appear in Proceedings of "Sources and Detection of Dark Matter/Energy in the Universe", ed. D. B. Cline. 6 pages, including 2 color figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0005476
dc.identifierhttp://arxiv.org/abs/astro-ph/0005476
dc.identifierProc. of "Sources and Detection of Dark Matter and Dark Energy in the Universe," ed. D.B. Cline (Springer,Berlin) p.92 (2000)
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1068
dc.subjectAstrophysics
dc.titleIs the Lambda CDM Model Consistent with Observations of Large-Scale Structure?
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