Viscous effects in the dark sector of the universe

dc.creator	Fabris, J. C.
dc.creator	Caramês, T. R. P.
dc.creator	Wojnar, A.
dc.creator	Velten, H. E. S.
dc.date.accessioned	2021-06-22T17:25:51Z
dc.date.available	2021-06-22T17:25:51Z
dc.date.issued	2020
dc.description.abstract	Viscous properties are attributed to the dark sector of the Universe. They contribute to the accelerated expansion phase of the Universe and can alleviate existing tensions in the ΛCDM model at small scales. We provide a short review of recent efforts on this topic. Different viscous models for the dark sector are analysed both from theoretical and observational point of view.	pt_BR
dc.identifier.citation	FABRIS, J. C. et al. Viscous effects in the dark sector of the universe. International Journal of Modern Physics A, Singapore, v. 35, n. 02n03, 2040041, 2020. DOI: 10.1142/S0217751X20400412.	pt_BR
dc.identifier.uri	https://repositorio.ufla.br/handle/1/46549
dc.identifier.uri	https://www.worldscientific.com/doi/abs/10.1142/S0217751X20400412	pt_BR
dc.language	en_US	pt_BR
dc.publisher	World Scientific	pt_BR
dc.rights	openAccess	pt_BR
dc.source	International Journal of Modern Physics A	pt_BR
dc.subject	Cosmology	pt_BR
dc.subject	Dark matter	pt_BR
dc.subject	Dark energy	pt_BR
dc.subject	Viscosity	pt_BR
dc.subject	Cosmologia	pt_BR
dc.subject	Matéria escura	pt_BR
dc.subject	Energia escura	pt_BR
dc.subject	Viscosidade	pt_BR
dc.title	Viscous effects in the dark sector of the universe	pt_BR
dc.type	Artigo	pt_BR

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