Going Nonlinear with Dark Energy Cosmologies

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dc.creatorLinder, Eric V.
dc.creatorWhite, Martin
dc.date2005-08-18
dc.date.accessioned2026-07-07T11:57:15Z
dc.date.available2026-07-07T11:57:15Z
dc.descriptionWe propose an efficient method for generating high accuracy (~1%) nonlinear power spectra for grids of dark energy cosmologies. Our prescription for matching matter growth automatically matches the main features of the cosmic microwave background anisotropy power spectrum, thus naturally including ``CMB priors''.
dc.description3 pages, 1 figure
dc.identifierhttps://arxiv.org/abs/astro-ph/0508401
dc.identifierhttp://arxiv.org/abs/astro-ph/0508401
dc.identifierPhys.Rev.D72:061304,2005
dc.identifierdoi:10.1103/PhysRevD.72.061304
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/205815
dc.subjectAstrophysics
dc.titleGoing Nonlinear with Dark Energy Cosmologies
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