The effective field theory of dark energy diagnostic of Linear Horndeski Theories After GW170817 and GRB170817A.

dc.contributor.authorPerenon, Louis
dc.contributor.authorVelten, Hermano Endlich Schneider
dc.date.accessioned2023-01-18T21:21:24Z
dc.date.available2023-01-18T21:21:24Z
dc.date.issued2019pt_BR
dc.description.abstractWe summarize the effective field theory of dark energy construction to explore observable predictions of linear Horndeski theories. We review the diagnostic of these theories on the correlation of the large-scale structure phenomenological functions: the effective Newton constant, the light deflection parameter, and the growth function of matter perturbations. We take this opportunity to discuss the evolution of the bounds the propagation speed of gravitational waves has undergone and use the most restrictive one to update the diagnostic.pt_BR
dc.identifier.citationPERENON, L.; VELTEN, H. E. S. The effective field theory of dark energy diagnostic of Linear Horndeski Theories After GW170817 and GRB170817A. Universe, v. 5, n. 6, 2019. Disponível em: <https://www.mdpi.com/2218-1997/5/6/138>. Acesso em: 06 jul. 2022.pt_BR
dc.identifier.doihttps://doi.org/10.3390/universe5060138pt_BR
dc.identifier.issn2218-1997
dc.identifier.urihttp://www.repositorio.ufop.br/jspui/handle/123456789/16004
dc.language.isoen_USpt_BR
dc.rightsabertopt_BR
dc.rights.licenseThis article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/). Fonte: o PDF do artigo.pt_BR
dc.subjectModified gravitypt_BR
dc.subjectLarge-scale structurespt_BR
dc.titleThe effective field theory of dark energy diagnostic of Linear Horndeski Theories After GW170817 and GRB170817A.pt_BR
dc.typeArtigo publicado em periodicopt_BR

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