Placing limits on the spin-torsion fluctuation from the stability of Friedmann solution and COBE data

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dc.creatorde Andrade, L. C. Garcia
dc.date2000-07-14
dc.date.accessioned2026-07-07T01:54:24Z
dc.date.available2026-07-07T01:54:24Z
dc.descriptionThe gravitational stability of Friedmann metric with respect to homogeneous and isotropic perturbations in Einstein-Cartan cosmology is used together with the COBE data to place a limit on the spin-torsion primordial density fluctuation.Cosmological perturbations in Bianchi type III models are shown to have no contributions from torsion at the early stages of the Universe.
dc.descriptionLatex file
dc.identifierhttps://arxiv.org/abs/astro-ph/0007204
dc.identifierhttp://arxiv.org/abs/astro-ph/0007204
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1333
dc.subjectAstrophysics
dc.titlePlacing limits on the spin-torsion fluctuation from the stability of Friedmann solution and COBE data
dc.typetext

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