Status of non-Riemannian cosmology

Assad; Babourova; Blagojević; Brüggen; Buchbinder; Canale; Capozziello; Capozziello; Capozziello; Capozziello; Cartan; Chatterjee; de Oliveira; de Ritis; Demianski; Dirk Puetzfeld; Einstein; Fennelly; Garcia de Andrade; Gasperini; Gasperini; Goenner; Hammond; Hammond; Hehl; Hehl; Hehl; Hehl; Kao; Kerlick; Kerlick; Kopczyński; Kopczyński; Kunstatter; Maroto; Minkevich; Minkevich; Minkevich; Minkevich; Minkevich; Minkevich; Minkowski; Moffat; Nurgaliev; Obukhov; Obukhov; Obukhov; Palle; Palle; Poberii; Puetzfeld; Puetzfeld; Puetzfeld; Puetzfeld; Raychaudhuri; Smalley; Smalley; Stewart; Tafel; Trautman; Tsamparlis; Tsamparlis; Tucker; Vereshchagin; Weyl; Wolf

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Status of non-Riemannian cosmology

Abstract

We provide a brief chronological guide to the literature on non-Riemannian cosmological models. Developments in this field are traced back to the early seventies and are given in table form.Comment: 10 pages, 1 figure, to appear in the proceedings of the 6th UCLA Symposium on ''Sources and Detection of Dark Matter and Dark Energy in the Universe'', 4 references added, minor typos fixe

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Last time updated on 10/12/2019