Inhomogeneities and the Intergalactic Distance-Redshift Relation

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dc.creatorKantowski, R.
dc.date1998-04-23
dc.date.accessioned2026-07-07T02:26:40Z
dc.date.available2026-07-07T02:26:40Z
dc.descriptionModifications in Friedmann-Lemaitre-Robertson-Walker (FLRW) Hubble diagrams caused by mass density inhomogeneities are used to illustrate possible effects on a determination of the mass parameter $Ω_m$ and the cosmological constant $Λ$. The values of these parameters inferred from a given set of observations depend on the fractional amount of matter in inhomogeneities and can differ from those obtained by using standard FLRW Hubble diagrams by as much as a factor of two.
dc.description4 pages, 2 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/9804249
dc.identifierhttp://arxiv.org/abs/astro-ph/9804249
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12370
dc.subjectAstrophysics
dc.titleInhomogeneities and the Intergalactic Distance-Redshift Relation
dc.typetext

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