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Growth rate in the dynamical dark energy models

Dark energy models with a slowly rolling cosmological scalar field provide a popular alternative to the standard, time-independent cosmological constant model. We study the simultaneous evolution of background expansion and growth in the scalar field model with the Ratra–Peebles self-interaction pot...

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Detalles Bibliográficos
Autores principales: Avsajanishvili, Olga, Arkhipova, Natalia A., Samushia, Lado, Kahniashvili, Tina
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Berlin Heidelberg 2014
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4445924/
https://www.ncbi.nlm.nih.gov/pubmed/26041971
http://dx.doi.org/10.1140/epjc/s10052-014-3127-5