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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...
Autores principales: | Avsajanishvili, Olga, Arkhipova, Natalia A., Samushia, Lado, Kahniashvili, Tina |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Springer Berlin Heidelberg
2014
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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 |
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