On the area distance and the Riemannian geometry

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dc.creatorPalle, D.
dc.date1999-05-19
dc.date.accessioned2026-07-07T02:31:40Z
dc.date.available2026-07-07T02:31:40Z
dc.descriptionWe study an area distance in the Riemannian spacetime with expansion, vorticity and acceleration. It is shown that this observable depends on expansion, deceleration and acceleration parameters to third order in redshift, as well as on vorticity. Thus, the considerable acceleration or vorticity of the Universe can substantially influence the standard astronomical distance calibrators.
dc.description5 pages, LaTeX style
dc.identifierhttps://arxiv.org/abs/astro-ph/9905252
dc.identifierhttp://arxiv.org/abs/astro-ph/9905252
dc.identifierNuovo Cim. B115 (2000) 375-378
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14234
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn the area distance and the Riemannian geometry
dc.typetext

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