Structure formation in the quintessential Universe

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dc.creatorLokas, Ewa L.
dc.date2001-12-03
dc.date2002-07-25
dc.date.accessioned2026-07-07T02:01:38Z
dc.date.available2026-07-07T02:01:38Z
dc.descriptionI review the main characteristics of structure formation in the quintessential Universe. Assuming equation of state w=p/\varrho=$const I provide a brief description of the background cosmology and discuss the linear growth of density perturbations, the strongly nonlinear evolution, the power spectra and rms fluctuations as well as mass functions focusing on the three values w=-1, -2/3 and -1/3. Finally I describe the presently available and future constraints on w.
dc.description11 pages, 6 figures, corrected description of strongly nonlinear evolution and other details
dc.identifierhttps://arxiv.org/abs/astro-ph/0112031
dc.identifierhttp://arxiv.org/abs/astro-ph/0112031
dc.identifierActa Phys.Polon. B32 (2001) 3643-3654
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3823
dc.subjectAstrophysics
dc.titleStructure formation in the quintessential Universe
dc.typetext

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