Cosmic Crystallography of the Second Order

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dc.creatorFagundes, H. V.
dc.creatorGausmann, E.
dc.date2002-12-09
dc.date2003-01-14
dc.date.accessioned2026-07-07T02:06:48Z
dc.date.available2026-07-07T02:06:48Z
dc.descriptionThe cosmic crystallography method of Lehoucq et al. [1] produces sharp peaks in the distribution of distances between the images of cosmic sources. But the method cannot be applied to universes with compact spatial sections of negative curvature. We apply to these a second order crystallographic effect, as evidenced by statistical parameters.
dc.description14 pages, 9 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0212209
dc.identifierhttp://arxiv.org/abs/astro-ph/0212209
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5487
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCosmic Crystallography of the Second Order
dc.typetext

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