The cosmology of the nonsymmetric theory of gravitation

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dc.creatorProkopec, Tomislav
dc.creatorValkenburg, Wessel
dc.date2005-03-14
dc.date2006-03-27
dc.date.accessioned2026-07-07T06:37:08Z
dc.date.available2026-07-07T06:37:08Z
dc.descriptionWe show that during cosmological inflation the nonsymmetric metric tensor theory of gravitation develops a spectrum which is potentially observable by cosmic microwave background observations, and may be the most sensitive probe of the scale of cosmic inflation.
dc.description10 pages, 2 figures. The improved version to be published in Phys. Lett. B. Note change in authors
dc.identifierhttps://arxiv.org/abs/astro-ph/0503289
dc.identifierhttp://arxiv.org/abs/astro-ph/0503289
dc.identifierPhys.Lett. B636 (2006) 1-4
dc.identifierdoi:10.1016/j.physletb.2006.03.019
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/100288
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleThe cosmology of the nonsymmetric theory of gravitation
dc.typetext

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